[2013-SOSP]From ARIES to MARS Transaction Support for Next-Generation, Solid-State Drives
用英语介绍太阳系
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Neptune is the eighth and farthest planet from the Sun in our Solar System. Named for the Roman god of the sea, it is the fourthlargest planet by diameter(直径) and the third-largest by mass.
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The rings of Saturn are the most extensive (大规模) planetary ring(行星 环) system of any planet in the Solar System . They consist of countless (无数) small particles, ranging in size from micrometre to metres that form clumps(块) that in turn orbit about Saturn.
缺一张金星夜 空图
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Mars is the fourth planet from the Sun in the Solar System. It is often described as the “Red Planet”, as the iron oxide(氧 化铁) prevalent (普 遍)on its surface gives it a reddish (淡 红色) appearance.
** The Sun is the star at
the center of the Solar System. It has a diameter(直径) of about 1,392,000 km, . about 109 times that of Earth, and its mass accounts for about 99.86% of the total mass of the Solar System.
poetry
Genres
• • • • • • • • Narrative poetry Epic poetry Dramatic poetry Satirical poetry Lyric poetry Elegy Verse fable Prose poetry
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Narrative poetry is a genre of poetry that tells a story. Broadly it subsumes epic poetry, but the term "narrative poetry" is often reserved for smaller works, generally with more appeal to human interest.
• musical or incantatory effects
• Aristotle's Poetics • three genres of poetry—the epic, the comic, and the tragic
• Later aestheticians ----epic poetry, lyric poetry and dramatic poetry
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Another exemplar of English satirical poetry was Alexander Pope, who famously chided critics in his Essay on Criticism (1709). Dryden and Pope were writers of epic poetry, and their satirical style was accordingly epic; but there is no prescribed form for satirical poetry.
小学上册第8次英语第6单元期末试卷
小学上册英语第6单元期末试卷英语试题一、综合题(本题有100小题,每小题1分,共100分.每小题不选、错误,均不给分)1.My uncle is a great ____.2.I have a _____ for my birthday. (party)3.My cousin enjoys __________ (研究) different topics.4.My mom loves to __________ (阅读).5. A ______ is a plant that grows in very dry areas.6.Parrots love to eat ______ (水果).7.Which one is a pet?A. CowB. DogC. ChickenD. Horse8.The _____ of the Earth helps to regulate its temperature.9.Which of these is a reptile?A. FrogB. SnakeC. SparrowD. MouseB10.She has a _____ (funny) face.11.What is the name of the famous US landmark that celebrates freedom?A. The Great WallB. The ColosseumC. The Statue of LibertyD. The Eiffel TowerC The Statue of Liberty12.The horse drinks water from the ______ (水槽). It looks very ______ (口渴).13.I want to _____ (understand) plant biology.14.What is the name of the layer of atmosphere closest to Earth's surface?A. TroposphereB. StratosphereC. MesosphereD. Thermosphere15.What do you call the person who studies rocks?A. BiologistB. GeologistC. ChemistD. Physicist16.The chemical formula for cesium chloride is ______.17. A butterfly’s wings are covered in tiny ______.18.What is the name of the first artificial satellite launched into space?A. VoyagerB. SputnikC. ApolloD. Challenger19.The baby is _____ in the crib. (sleeping)20. A chemical that can act as a reducing agent is called a ______.21. A ____(community impact project) focuses on measurable outcomes.22.Salt is formed when an acid reacts with a ________.23.In the box, there are many ____ waiting to be played with. (玩具)24.My ________ (奶奶) makes the best cookies in the world.25.The chemical formula for sodium bromide is _______.26.The _____ (四季变化) influences plant life cycles.27.The _______ of light can create different colors when passing through a prism.28.I love to ___ in the pool. (swim)29.The city of New Delhi is the capital of _______.30.My dad is an amazing __________ (修理工).31.Which planet is known for its rings?A. MarsB. SaturnC. JupiterD. NeptuneB32.I think it's important to support local businesses by __________.33.There are many types of ______ (花朵) in spring.34.What do we call a young horse?A. CalfB. FoalC. KidD. Lamb35.Her birthday is _____ (in/on) June.36.What do we call the color of the ocean?A. BlueB. GreenC. BlackD. ClearA37.Which instrument has keys and is played with fingers?A. ViolinB. GuitarC. PianoD. Drums38.What do we call a person who acts in movies?A. ActorB. DirectorC. ProducerD. ScreenwriterA39.What is the name of the famous ancient city in Turkey?A. EphesusB. TroyC. CappadociaD. All of the above40.What do we call a person who sells vegetables?A. GrocerB. FarmerC. VendorD. All of the above41.How many senses do humans have?A. 4B. 5C. 6D. 7B42.He likes to _______ (draw/paint) pictures.43.What is the opposite of busy?A. FreeB. OccupiedC. EngagedD. Both A and BA44.The chemical formula for lithium hydroxide is ______.45.What do we call the study of the past?A. ArchaeologyB. AnthropologyC. HistoryD. SociologyC46.The _____ (树木) provide shade on hot days.47.Friction can generate ______.48.I like to ride my ___. (scooter)49.The chicken lays _____ eggs.50.My brother enjoys __________. (骑自行车)51.The ________ (team) is committed to success.52.What color do you get when you mix blue and yellow?A. GreenB. PurpleC. OrangeD. BrownA53.My _____ (舅舅) is a police officer.54.I read a _____ (书) before bed.55.What do we call the opposite of ‘young’?A. NewB. OldC. FreshD. Recent56.What do we call the science of studying the Earth's landforms and features?A. GeologyB. GeographyC. CartographyD. OceanographyA57.What do you call the process of water turning into vapor?A. EvaporationB. CondensationC. PrecipitationD. FiltrationA Evaporation58. A dilute solution has a ______ concentration of solute.59.She made a _____ drawing. (pretty)60.I saw a ________ in the sky.61.Which planet is known for its rings?A. EarthB. MarsC. SaturnD. Neptune62.My sister is my best _______ because we share everything and have fun together.63.I like to _______ new things.64.Which animal is known for its long trunk?A. GiraffeB. RhinoC. ElephantD. HippoC65.The ________ (环境变化研究) informs practices.66.The ________ was a significant event in the global historical context.67.In _____ (80), you can see the Northern Lights.68.My grandma loves to share her __________ (传统故事).69.My sister loves __________ (参与学校活动).70.The ________ was a leading advocate for equality in education.71.I enjoy _______ (收集) stickers.72.The main ingredient in baking soda is sodium _____.73.I love to watch the __________ fall from the sky in winter. (雪)74.I enjoy going ________ (滑冰) during winter.75.She is an _____ (演员) who stars in movies.76.My sister is my best _______ because we share everything.77.The ancient Silk Road was a trade route that connected _______ and Europe.78.What do you call the act of putting things away?A. StoringB. HidingC. DisposingD. OrganizingA79. A __________ is a type of bird known for its colorful feathers.80.What is the main purpose of a compass?A. Measure temperatureB. Show directionC. Tell timeD. Measure distanceB81.What is the color of a ripe strawberry?A. BlueB. GreenC. RedD. Yellow82.The capital of Thailand is ________ (泰国的首都是________).83.The process of ______ can change the landscape over time.84.Ostriches cannot _______ (飞).85.In a reaction, the enthalpy change can indicate whether heat is absorbed or _____.86.I have a _____ (map) of the city.87.What is the capital of Spain?A. BarcelonaB. MadridC. SevilleD. Valencia88.What do you call a vehicle that travels on tracks?A. CarB. TrainC. PlaneD. BoatB89.Which of these is a source of protein?A. BreadB. ChickenC. RiceD. PastaB90.Which of these is a mode of transportation?A. TableB. CarC. ChairD. Bed91.Which animal can live both in water and on land?A. FishB. DogC. FrogD. CatC92.What is 10 - 4?A. 5B. 6C. 7D. 893.The __________ (古罗马的建筑) still influences modern architecture.94.I enjoy watching the ______ in the sky.95.What do we call the place where we learn math, science, and history?A. LibraryB. SchoolC. OfficeD. Home96.Which fruit is known for having seeds on the outside?A. KiwiB. StrawberryC. BlueberryD. Raspberry97.Certain plants have developed ______ to attract specific pollinators. (某些植物发展出特定的特征来吸引特定的授粉者。
备战高考英语名校模拟真题速递(江苏专用)专题06 阅读理解之说明文10篇(第六期)(含解析)
备战高考英语名校模拟真题速递(江苏专用)第六期专题06 阅读理解之说明文10篇(2024·江苏南通·模拟预测)Mark Temple, a medical molecular (分子的) biologist, used to spend a lot of time in his lab researching new drugs for cancer treatments. He would extract DNA from cells and then add a drug to see where it was binding (结合) along the chemical sequence(序列). Before he introduced the drug, he’d look at DNA combination on a screen to see what might work best for the experiment, but the visual readout of the sequences was often unimaginably large.So Temple wondered if there was an easier way to detect favorable patterns. I realized I wanted to hear the sequence,” says Temple, who is also a musician. He started his own system of assigning notes to the different elements of DNA — human DNA is made of four distinct bases, so it was easy to start off with four notes — and made a little tune out of his materials. This trick indeed helped him better spot patterns in the sequences, which allowed him to make better choices about which DNA combinations to use.Temple isn’t the first person to turn scientific data into sound. In the past 40 years, researchers have gone from exploring this trick as a fun way to spot patterns in their studies tousing it as a guide to discovery. And the scientific community has come to realize that there’s some long-term value in this type of work. Temple, who from that first experiment has created his own algorithmic software to turn data into sound, believes the resulting music can be used to improve research and science communication.So Temple decided to add layers of sound to make the sonification (可听化) into songs. He sees a clear difference between “sonification” and “musification”. Using sound to represent data is scientific, but very different from using creative input to make songs. The musical notes from DNA may be melodic to the human ear, but they don’t sound like a song you’d listen to on the radio. So when he tried to sonify the virus, he added layers of drums and guitar, and had some musician friends add their own music to turn the virus into a full-blown post-rock song.Temple sees this work as an effective communication tool that will help a general audience understand complex systems in biology. He has performed his songs in public at concert halls in Australia.1.What is Mark Temple’s purpose in turning DNA data into sound?A.To help him fight boredom.B.To develop his creative ability.C.To make his drug more powerful.D.To aid the process of his experiments.2.What can we learn about Temple’s system?A.Its effect remains to be seen.B.It failed to work as expected.C.It is too complicated to operate.D.It has produced satisfying results.3.Why did Temple try to make the virus sound like real music when sonifying it?A.To get rid of public fear of the virus.B.To show h1s talent in producing music.C.To facilitate people’s understanding of science.D.To remind people or the roe or Science in art creation.4.What does the text mainly talk about?A.Why scientists are turning molecules into music.B.How scientists help the public understand science.C.Why music can be the best way to present science.D.How music helps scientists conduct their research.(2024·江苏南通·模拟预测)Phonics, which involves sounding out words syllable (音节) by syllable, is the best way to teach children to read. But in many classrooms, this can be a dirty word. So much so that some teachers have had to take phonics teaching materials secretly into the classroom. Most American children are taught to read in a way that study after study has found to be wrong.The consequences of this are striking. Less than half of all American adults were efficient readers in 2017. American fourth graders rank 15th on the Progress in International Literacy Study, an international exam.America is stuck in a debate about teaching children to read that has been going on for decades. Some advocate teaching symbol sound relationships (the sound k can be spelled as c, k, ck, or ch) known as phonics Others support an immersive approach (using pictures of cat to learn the word cat), known as “whole language”. Most teachers today, almost three out of four according to a survey by EdWeek Research Centre in 2019, use a mix of the two methods called “balanced literacy”.“A little phonics is far from enough.” says Tenette Smith, executive director of elementary education and reding at Mississippi’s education department. “It has to be systematic and explicitly taught.”Mississippi, often behind in social policy, has set an example here. In a state once blamed for its low reading scores, the Mississippi state legislature passed new literacy standards in 2013.Since then Mississippi has seen remarkable gains., Its fourth graders have moved from 49th (out of 50 states) to 20th on the National assessment of Educational Progress, a nationwide exam.Mississippi’s success is attributed to application of reading methods supported by a body of research known as the science of reading. In 1997 experts from the Department of Education ended the “reading war” and summed up the evidence. They found that phonics, along with explicit instruction in phonemic (音位的) awareness,fluency and comprehension, worked best.Yet over two decades on, “balanced literacy” is still being taught in classrooms. But advances in statistics and brain imaging have disproved the whole-language method. To the teacher who is an efficient reader, literacy seem like a natural process that requires educated guessing, rather than the deliberate process emphasized by phonics. Teachers can imagine that they learned to read through osmosis(潜移默化) when they were children. Without proper training, they bring this to classrooms.5.What do we learn about phonics in many American classrooms?A.It is ill reputed.B.It is mostly misapplied.C.It is totally ignored.D.It is seemingly contradictory.6.What has America been witnessing?A.A burning passion for improving teaching methods.B.A lasting debate over how to teach children to read.C.An increasing concern with children’s inadequacy in literacy.D.A forceful advocacy of a combined method for teaching reading.7.What’s Tenette Smith’s attitude towards “balanced literacy”?A.Tolerant.B.Enthusiastic.C.Unclear.D.Disapproving.8.According to the author what contributed to Mississippi’s success?A.Focusing on the natural process rather than deliberate training.B.Obtaining support from other states to upgrade teaching methods.C.Adopting scientifically grounded approaches to teaching reading.D.Placing sufficient emphasis upon both fluency and comprehension.(2024·江苏泰州·一模)A satellite is an object in space that orbits around another. It has two kinds — natural satellites and artificial satellites. The moon is a natural satellite that moves around the earth while artificial satellites are those made by man.Despite their widespread impact on daily life, artificial satellites mainly depend on different complicated makeups. On the outside, they may look like a wheel, equipped with solar panels or sails. Inside, the satellites contain mission-specific scientific instruments, which include whatever tools the satellites need to perform their work. Among them, high-resolution cameras and communication electronics are typical ones. Besides, the part that carries the load and holds all the parts together is called the bus.Artificial satellites operate in a systematic way just like humans. Computers function as the satellite’s brain, which receive information, interpret it, and send messages back to the earth. Advanced digital cameras serve asthe satellite’s eyes. Sensors are other important parts that not only recognize light, heat, and gases, but also record changes in what is being observed. Radios on the satellite send information back to the earth. Solar panels provide electrical power for the computers and other equipment, as well as the power to move the satellite forward.Artificial satellites use gravity to stay in their orbits. Earth’s gravity pulls everything toward the center of the planet. To stay in the earth’s orbit, the speed of a satellite must adjust to the tiniest changes in the pull of gravity. The satellite’s speed works against earth’s gravity just enough so that it doesn’t go speeding into space or falling back to the earth.Rockets carry satellites to different types and heights of orbits, based on the tasks they need to perform. Satellites closer to the earth are in low-earth orbit, which can be 200-500 miles high. The closer to the earth, the stronger the gravity is. Therefore, these satellites must travel at about 17,000 miles per hour to keep from falling back to the earth, while higher-orbiting satellites can travel more slowly.9.What is Paragraph 2 of the text mainly about?A.The appearance of artificial satellites.B.The components of artificial satellites.C.The basic function of artificial satellites.D.The specific mission of artificial satellites.10.What is the role of computers in artificial satellites?A.Providing electrical power.B.Recording changes observed.C.Monitoring space environment.D.Processing information received.11.How do artificial satellites stay in their orbits?A.By relying on powerful rockets to get out of gravity.B.By orbiting at a fixed speed regardless of gravity’s pull.C.By changing speed constantly based on the pull of gravity.D.By resisting the pull of gravity with advanced technologies.12.Why do satellites in higher-earth orbit travel more slowly?A.They are more affected by earth’s gravity.B.They take advantage of rockets more effectively.C.They have weaker pull of gravity in higher orbits.D.They are equipped with more advanced instruments.(2024·江苏泰州·一模)The human body possesses an efficient defense system to battle with flu viruses. The immune system protects against the attack of harmful microbes (微生物) by producing chemicals called antibodies, which are programmed to destroy a specific type of microbe. They travel in the blood and search the body for invaders (入侵者). When they find an invasive microbe, antibodies attack and destroy any cell thatcontains the virus. However, flu viruses can be a terrible enemy. Even if your body successfully fights against the viruses, with their ability to evolve rapidly, your body may have no protection or immunity from the new ones.Your body produces white blood cells to protect you against infectious diseases. Your body can detect invading microbes in your bloodstream because they carry antigens in their proteins. White blood cells in your immune system, such as T cells, can sense antigens in the viruses in your cells. Once your body finds an antigen, it takes immediate action in many different ways. For example, T cells produce more antibodies, call in cells that eat microbes, and destroy cells that are infected with a virus.One of the best things about the immune system is that it will always remember a microbe it has fought before and know just how to fight it again in the future. Your body can learn to fight so well that your immune system can completely destroy a virus before you feel sick at all.However, even the most cautious people can become infected. Fortunately, medical scientists have developed vaccines (疫苗), which are weakened or dead flu viruses that enter a person’s body before the person gets sick. These viruses cause the body to produce antibodies to attack and destroy the strong viruses that may invade during flu season.13.Why does flu pose a threat to the immune system?A.Microbes contain large quantities of viruses.B.Antibodies are too weak to attack flu viruses.C.The body has few effective ways to tackle flu.D.It’s hard to keep pace with the evolution of viruses.14.What does the underlined word “antigens” refer to in Paragraph 2?A.The cell protecting your body from viruses.B.The matter serving as the indicator of viruses.C.The antibodies helping to fight against viruses.D.The substance destroying cells infected with viruses.15.How do vaccines defend the body against the flu viruses?A.They strengthen the body’s immune system.B.They battle against weakened or dead viruses.C.They help produce antibodies to wipe out viruses.D.They expose the body to viruses during flu season.16.Which of the following is a suitable title for the text?A.Antibodies Save Our Health.B.Vaccines Are Of Great Necessity.C.Infectious Flu Viruses Are Around.D.Human Body Fights Against Flu Viruses.(23-24高三下·江苏扬州·开学考试)A recent study, led by Professor Andrew Barron, Dr. HaDi MaBouDi, and Professor James Marshall, illustrates how evolution has fine-tuned honey bees to make quick judgments while minimizing danger.“Animal lives are full of decisions,” says Professor Barron. “A honey bee has a brain smaller than a sesame (芝麻) seed. And yet it can make decisions faster and more accurately than’ we can. A robot programmed to do a bee’s job would need the backup of a supercomputer.”Bees need to work quickly and efficiently. They need to make decisions. Which flower will have a sweet liquid? While they’re flying, they face threats from the air. While landing, they’re vulnerable to potential hunter, some of which pretend to look like flowers.Researchers trained 20 bees to associate each of the five different colored “flower disks” with their visit history of reward and punishment. Blue flowers always had sugar juice. Green flowers always had a type of liquid with a bitter taste for bees. Other colors sometimes had glucose (葡萄糖). “Then we introduced each bee to a ‘garden’ with artificial ‘flowers’. We filmed each bee and timed their decision-making process,” says Dr. MaBouDi. “If the bees were confident that a flower would have food, they quickly decided to land on it, taking an average of 0.6 seconds. If they were confident that a flower wouldn’t have food, they made a decision just as quickly. If unsure, they took on average 1.4 seconds, and the time reflected the probability that a flower had food.”The team then built a computer model mirroring the bees’ decision-making process. They found the structure of the model looked very similar to the physical layout of a bee brain. “AI researchers can learn much from bees and other ‘simple’ animals. Millions of years of evolution has led to incredibly efficient brains with very low power requirements,” says Professor Marshall who co-founded a company that uses insect brain patterns to enable machines to move autonomously, like nature.17.Why does Professor Andrew Barron mention “a supercomputer”?A.To illustrate how a honey bee’s brain resemble each other.B.To explain how animals arrive at informed decisions fast.C.To demonstrate how a robot could finish a honey bee’s job.D.To emphasize how honey bees make decisions remarkably.18.Which of the following can best replace “vulnerable to” underlined in paragraph 3?A.Easily harmed by.B.Highly sensitive to.C.Deeply critical to.D.Closely followed by.19.What influenced the speed of trained bees in making decisions?A.Their judgments about reward and punishment.B.Their preference for the colors of flower disks.C.Their confirmation of food’s presence and absence.D.Their ability to tell real flowers from artificial ones.20.What message does Professor James Marshall want to give us?A.The power of bee brains is underestimated.B.Biology can inspire future AI.C.Autonomous machines are changing nature.D.AI should be far more efficient.(23-24高三下·江苏扬州·开学考试)Are you frequently overwhelmed by the feeling that life is leaving you behind, particularly when you look through social media sites and see all the exciting things your friends are up to? If so, you are not alone.FOMO, or Fear of Missing Out, refers to the perception that other people’s lives are superior to our own, whether this concerns socializing, accomplishing professional goals or generally having a more deeply fulfilling life. It shows itself as a deep sense of envy, and constant exposure to it can have a weakening effect on our self-respect. The feeling that we are always being left out of fundamentally important events, or that our lives are not living up to the image pictured by others, can have long-term damaging psychological consequences.While feelings of envy and inadequacy seem to be naturally human, social media seems to have added fuel to the fire in several ways. The reason why social media has such a triggering effect is tied to the appeal of social media in the first place: these are platforms which allow us to share only the most glowing presentations of our accomplishments, while leaving out the boring aspects of life. While this kind of misrepresentation could be characterized as dishonest, it is what the polished atmosphere of social media seems to demand.So how do we avoid falling into the trap of our own insecurities? Firstly, consider your own social media posts. Have you ever chosen photos or quotes which lead others to the rosiest conclusions about your life? Well, so have others and what they’ve left hidden is the fact that loneliness and boredom are unavoidably a part of everyone’s day-to-day life, and you are not the only one feeling left out. Secondly, learn to appreciate the positives. You may not be a regular at exciting parties or a climber of dizzying peaks, but you have your health, a place to live, and real friends who appreciate your presence in their lives. Last of all, learn to shake things off. We are all bombarded daily with images of other people’s perfection, but really, what does it matter? They are probably no more real than the most ridiculous reality TV shows.21.What can frequently experiencing FOMO lead to?A.Harm to one’s feeling of self-value.B.A more satisfying and fulfilling social life.C.Damage to one’s work productivity.D.Less likelihood of professional success.22.What does the author suggest in the third paragraph?A.The primary reason for FOMO is deeply rooted in social media.B.Our own social media posts help us feel much more confident.C.People who don’t share posts on social media are more bored.D.Social media’s nature enhances envious feelings and self-doubt.23.Why does the author mention reality TV shows in the last paragraph?A.To emphasize how false what we see on social media can be.B.To indicate how complicated social media has turned to.C.To figure out how popular and useful social media has been.D.To point out how educational value reality TV shows reflect.24.Which is the best title for the text?A.Myths and misconceptions about FOMO B.FOMO: what it is and how to overcome itC.How FOMO is changing human relationships D.We’re now all in the power of “FOMO addiction”(23-24高三上·江苏泰州·阶段练习)While Huawei’s official website does not call Mate 60 Pro a 5G smartphone, the phone’s wideband capabilities are on par with other 5G smartphones, raising a related question: As a leader in 5G technology, has Huawei managed to develop a 5G smartphone on its own?The answer is not simple. Huawei, as a pioneer in global 5G communication equipment, has played a leading role in the commercialization of 5G technology, with its strong system design and fields such as baseband chips (基带芯片), baseband processors and 5G modems.However, basebands and modems are not the only aspects that define 5G wireless communication. The stability and high-quality signals of a 5G smartphone also depend on other critical components such as RF transceivers (射频收发器) and RF front ends and antennas (天线) . These components are largely dominated by four US high-tech giants—Qualcomm, Avago Technologies, Ansem and Qorvo—which account for a surprising global market share.Huawei has faced significant challenges in getting critical components because of the sanctions imposed by the United States which are primarily responsible for the inability of the Chinese company to launch 5G smartphones in the past three years. However, Mate 60 Pro, despite not being labeled a 5G device, exhibits mobile network speeds comparable to Apple’s latest 5G-enabled devices, offering a stable communication experience. This suggests Huawei has, over the past three years, overcome the 5G development and production limits due to the US sanctions by cooperating with domestic partners, and establishing an independent and controllable stable supply chain.Considering that Huawei has not explicitly marketed this device as a 5G smartphone, it is possible that it isyet to fully overcome some key core technological and componential shortcomings. For the time being, we can consider Huawei’s Mate 60 Pro as 4.99G. But when combined with the satellite communication capabilities of Mate 60 Pro, it is clear Huawei has been trying to find more advanced wireless communication solutions for smartphones and making significant progress in this attempt. This should be recognized as a remarkable endeavor, even a breakthrough.25.What do the underlined words “on par with” mean in Paragraph 1?A.as poor as.B.as good as.C.worse than.D.better than.26.Why was it tough for Huawei to develop a 5G smartphone three years ago?A.Its system design and fields needed to be updated.B.It only focused on the commercialization of 5G technology.C.It was unwilling to cooperate with high-tech giants in America.D.It lacked critical components mainly controlled by US high-tech giants.27.What does Paragraph 4 centre on?A.The US sanctions.B.Critical components.C.Apple’s latest 5G-enabled devices.D.Progress in Mate 60 Pro.28.What is the text mainly about?A.Huawei faced with significant challengesB.Huawei’s Mate 60 Pro—a 5G smartphoneC.Huawei’s Mate 60 Pro—a remarkable breakthroughD.Huawei leading in global 5G communication equipment(23-24高三上·江苏无锡·期末)Blue-light-filtering glasses (滤蓝光眼镜) have become an increasingly popular solution for protecting our eyes from electronic screens’ near-inescapable glow — light that is commonly associated with eyestrain (眼疲劳). In recent years they’ve even become fashion statements that are recognized by celebrities and ranked in style guides. But a recent review paper shows such glasses might not be as effective as people think.The paper, published last week in Cochrane Database of Systematic Reviews, analyzed data from previous trials that studied how blue-light-filtering glasses affect vision tiredness and eye health. The study’s authors found that wearing blue-light-filtering glasses does not reduce the eyestrain people feel after using computers.“It’s an excellent review,” says Mark Rosenfield, a professor at the State University of New York College of Optometry, who was not involved in the study. “The conclusions are no surprise at all. There have been a number of studies that have found exactly the same thing, that there’s just no evidence that blue-blocking glasses have anyeffect on eyestrain.” He adds that the new review reinforces the fact that there is virtually no evidence that blue-blocking glasses affect eyestrain despite them being specifically marketed for that purpose. As for using blue-light-filtering eyeglasses for eye health, for now, Rosenfield says, “there’s nothing to support people buying them”.The strain we may feel while staring at our phone or computer screen too long is likely to be caused by multiple factors, such as bad habits or underlying conditions, an associate professor of vision science at the University of Melbourne, Downie says. She argues that how we interact with digital devices contributes more to eyestrain than screens’ blue light does. Changing the frequency and duration of screen usage and distancing one’s eyes from the screens might be more important in reducing discomfort, Downie says. She adds that people who experience eyestrain should see a doctor to assess whether they have an underlying health issue such as far-sightedness or dry eye disease.29.What can we know about blue-light-filtering glasses from the text?A.They can improve eyesight.B.They may not reduce eyestrain.C.They can promote eye health.D.They can help to cure eye diseases.30.What can we infer from paragraph 2?A.A great many professors were involved in the study.B.Blue-blocking glasses on the market are harmful to eyes.C.The finding of the study comes as a surprise to the public.D.Data from previous trials help the study a lot.31.What does the underlined word “reinforces” mean in paragraph 3?A.Denies.B.Opposes.C.Strengthens.D.Evaluates.32.What should we do if we suffer from eyestrain according to Downie?A.Wear blue-light-filtering glasses.B.Have an examination in the hospital.C.Stop staring at the screen for ever.D.Focus on the frequency of phone usage.(2024·江苏连云港·一模)Not all birds sing, but several thousand species do. They sing to defend their territory and croon (柔声唱) to impress potential mates. “Why birds sing is relatively well-answered,” says Iris Adam, a behavioral neuroscientist. However, the big question for her was why birds sing so much.“As soon as you sing, you reveal yourself,” Adam says. “Like, where you are and where your territory is.” In a new study published in the journal Nature Communications, Adam and her co-workers offer a new explanation for why birds take that risk. They may have to sing a lot every day to give their vocal (发声的) muscles the regular exercise they need to produce top-quality songs. To figure out whether the muscles that produce birdsongsrequire daily exercise, Adam designed an experiment on zebra finches-the little Australian songbirds.She prevented them from singing for a week by keeping them in the dark cage almost around the clock. Light is what galvanizes the birds to sing, so she had to work to keep them from warbling (鸣叫). “The first two or three days, it’s quite easy,” she says. “But the longer the experiment goes, the more they are like, ‘I need to sing.’” At that point, she’d tap the cage and tell them to stop singing.After a week, the birds’ singing muscles lost half their strength. But Adam wondered whether that impacted the quality of songs. When she played a male’s song before and after the seven days of darkness, she couldn’t hear a difference. But when Adam played it to a group of female birds, six out of nine preferred the song that came from a male who’d been using his singing muscles daily.Adam’s conclusion shows that “songbirds need to exercise their vocal muscles to produce top-performance songs. If they don’t sing, they lose performance, and their songs get less attractive to females.” This may help explain songbirds’ continuous singing.It’s a good rule to live by, whether you’re a bird or a human-practice makes perfect, at least when it comes to singing one’s heart out.33.According to Iris Adam, birds sing so much to ______.A.warn other birds of risks B.produce more songsC.perform perfectly in singing D.defend their territory34.What does the underlined word “galvanizes” in Paragraph 3 mean?A.Prepares.B.Stimulates.C.Forbids.D.Frightens.35.What do we know about the caged birds in the experiment?A.They lost the ability to sing.B.They strengthened their muscles.C.Their songs showed no difference.D.Their songs became less appealing.36.What may Iris Adam agree with?A.The songbirds live on music.B.The songbirds are born singers.C.Daily exercise keeps birds healthy.D.Practice makes birds perfect singers.(23-24高三上·江苏扬州·期末)Sometimes called “Earth’s twin,” Venus is similar to our world in size and composition. The two rocky planets are also roughly the same distance from the sun, and both have an atmosphere. While Venus’s cold and unpleasant landscape does make it seem far less like Earth, scientists recently detected another striking similarity between the two, the presence of active volcanoes.When NASA’s Magellan mission mapped much of the planet with radar in the 1990sit revealed an。
高中英语文学体裁单选题80题(含答案)
高中英语文学体裁单选题80题(含答案)1.Which of the following is a characteristic of lyric poetry?A. Tells a long narrative storyB. Focuses on a single emotional momentC. Describes historical events in detailD. Presents arguments and debates答案:B。
解析:抒情诗的特点是聚焦于单一的情感瞬间。
选项A 是叙事诗的特点;选项C 更倾向于史诗的特点;选项D 不是诗歌常见的主要特点。
2.Poetry that uses regular rhyme and meter is called:A. Free verse poetryB. Blank verse poetryC. Sonnet poetryD. Rhymed poetry答案:D。
解析:使用有规律的押韵和格律的诗歌被称为押韵诗。
选项 A 自由诗不强调押韵和格律;选项 B 无韵诗虽有格律但不押韵;选项C 十四行诗只是一种特定形式的诗歌,不一定是所有押韵有格律的诗歌都叫十四行诗。
3.Which poet is known for his use of imagism in poetry?A. William WordsworthB. T.S. EliotC. Ezra PoundD. Robert Frost答案:C。
解析:埃兹拉·庞德以意象派诗歌闻名。
威廉·华兹华斯是浪漫主义诗人;T.S.艾略特的诗歌风格较为复杂多样但不是以意象派闻名;罗伯特·弗罗斯特是自然主义诗人。
4.The form of poetry that consists of three lines with a specific syllable count is:A. HaikuB. SonnetC. LimerickD. Ballad答案:A。
the exploration of mars雅思阅读解析
the exploration of mars雅思阅读解析For centuries,explorers have risked their lives venturing into the unknown for reasons that were to varying degrees economic and nationalistic,Columbus went west to look for better trade routes to the Orient and to promote the greater glory of Spain.Lewis and Clark journeyed into the American wilderness to find out what the U.S.had acquired when it purchased Louisiana,and the Apollo astronauts rocketed to the moon in a dramatic show of technological muscle during the cold war.Although their missions blended commercial andpolitical-military imperatives,the explorers involved all accomplished some science simply by going where no scientists had gone before.Today Mars looms as humanity's next great terra incognita(未探明之地).And with doubtful prospects for a short-term financial return,with the cold war a rapidly fading memory and amid a growing emphasis on international cooperation in large space ventures,it is clear that imperatives other than profits or nationalism will have to compel human beings to leave their tracks on the planet'sreddish surface.Could it be that science,which has long played a minor role in exploration,is at last destined to take a leading role?The question naturally in vites a couple of others:Are there experiments that only human could do on Mars?Couldthose experiments provide insights profound enough to justify the expense of sending people across interplanetary space?With Mars the scientific stakes are arguably higher than they have ever been.The issue of whether life ever existed on the planet,and whether it persists to thisday,has been highlighted by mounting evidence thatthe Red Planet once had abundant stable,liquid water and by the continuing controversy over suggestions the bacterial fossils rode to Earth on a meteorite(陨石)from Mars.A mor conclusive answer about life on Mars,past or present,would give researchers invaluable data about the range of conditions under which a planet can generate the complex chemistry that leads to life.If it could be establishedthat life arose independently on Mars and Earth,the finding would provide the first concrete clues in one of the deepest mysteries in all of science:the prevalence of life in the universe.1.For What purposes did the explorers go the unknown places in the past?2.In the exploration of Mars,_still remains uncertain.3.What has long been regarded as unimportant in the past explorations?4.What has been found on a meteorite from Mars?5.The conditions under which life originates would be revealed with the proof of_on Mars.答案:1.[For economic and nationalistic purposes.][定位]根据explorers go to unknown查找到全文首句。
中央财经大学
10
Children born to serve the country (cont.d)
• Maintained the birth rate to maintain military power
Until 30 years old all men lived in one house and were not full-fledged citizens free to live with their wives, to make clandestine marriage instill an early burning love Physical training of bare boys and girls together in a place to draw and allure young men to marry while men who would not marry walked bare outside. Fathers of 3 exempt from military service The state would find another younger mate for a childless wife. • No jealousy • Children were not private to any men but common to the common
中国经济与管理研究院
March 28 & April 6 & 13, 2008 2008年3月28日和4月6和13日
1
Socrates (苏格拉底)
Taught, but not for money like the Sophists. Like the Sophists’, his pupils were from aristocratic party. Taught and sought knowledge by the method of dialectic (question & answer, first practiced by Zeno 芝诺) in dialogues
Entropy changes in the clustering of galaxies in a
Vol.3, No.1, 65-68 (2011)doi:10.4236/ns.2011.31009Natural ScienceEntropy changes in the clustering of galaxies in an expanding universeNaseer Iqbal1,2*, Mohammad Shafi Khan1, Tabasum Masood11Department of Physics, University of Kashmir, Srinagar, India; *Corresponding Author:2Interuniversity Centre for Astronomy and Astrophysics, Pune, India.Received 19 October 2010; revised 23 November 2010; accepted 26 November 2010.ABSTRACTIn the present work the approach-thermody- namics and statistical mechanics of gravitating systems is applied to study the entropy change in gravitational clustering of galaxies in an ex-panding universe. We derive analytically the expressions for gravitational entropy in terms of temperature T and average density n of the par-ticles (galaxies) in the given phase space cell. It is found that during the initial stage of cluster-ing of galaxies, the entropy decreases and fi-nally seems to be increasing when the system attains virial equilibrium. The entropy changes are studied for different range of measuring correlation parameter b. We attempt to provide a clearer account of this phenomena. The entropy results for a system consisting of extended mass (non-point mass) particles show a similar behaviour with that of point mass particles clustering gravitationally in an expanding uni-verse.Keywords:Gravitational Clustering; Thermodynamics; Entropy; Cosmology1. INTRODUCTIONGalaxy groups and clusters are the largest known gravitationally bound objects to have arisen thus far in the process of cosmic structure formation [1]. They form the densest part of the large scale structure of the uni-verse. In models for the gravitational formation of struc-ture with cold dark matter, the smallest structures col-lapse first and eventually build the largest structures; clusters of galaxies are then formed relatively. The clus-ters themselves are often associated with larger groups called super-clusters. Clusters of galaxies are the most recent and most massive objects to have arisen in the hiearchical structure formation of the universe and the study of clusters tells one about the way galaxies form and evolve. The average density n and the temperature T of a gravitating system discuss some thermal history of cluster formation. For a better larger understanding of this thermal history it is important to study the entropy change resulting during the clustering phenomena be-cause the entropy is the quantity most directly changed by increasing or decreasing thermal energy of intraclus-ter gas. The purpose of the present paper is to show how entropy of the universe changes with time in a system of galaxies clustering under the influence of gravitational interaction.Entropy is a measure of how disorganised a system is. It forms an important part of second law of thermody-namics [2,3]. The concept of entropy is generally not well understood. For erupting stars, colloiding galaxies, collapsing black holes - the cosmos is a surprisingly or-derly place. Supermassive black holes, dark matter and stars are some of the contributors to the overall entropy of the universe. The microscopic explanation of entropy has been challenged both from the experimental and theoretical point of view [11,12]. Entropy is a mathe-matical formula. Standard calculations have shown that the entropy of our universe is dominated by black holes, whose entropy is of the order of their area in planck units [13]. An analysis by Chas Egan of the Australian National University in Canberra indicates that the col-lective entropy of all the supermassive black holes at the centers of galaxies is about 100 times higher than previ-ously calculated. Statistical entropy is logrithmic of the number of microstates consistent with the observed macroscopic properties of a system hence a measure of uncertainty about its precise state. Statistical mechanics explains entropy as the amount of uncertainty which remains about a system after its observable macroscopic properties have been taken into account. For a given set of macroscopic quantities like temperature and volume, the entropy is a function of the probability that the sys-tem is in various quantumn states. The more states avail-able to the system with higher probability, the greater theAll Rights Reserved.N. Iqbal et al. / Natural Science 3 (2011) 65-6866 disorder and thus greater the entropy [2]. In real experi-ments, it is quite difficult to measure the entropy of a system. The technique for doing so is based on the thermodynamic definition of entropy. We discuss the applicability of statistical mechanics and thermodynam-ics for gravitating systems and explain in what sense the entropy change S – S 0 shows a changing behaviour with respect to the measuring correlation parameter b = 0 – 1.2. THERMODYNAMIC DESCRIPTION OF GALAXY CLUSTERSA system of many point particles which interacts by Newtonian gravity is always unstable. The basic insta-bilities which may occur involve the overall contraction (or expansion) of the system, and the formation of clus-ters within the system. The rates and forms of these in-stabilities are governed by the distribution of kinetic and potential energy and the momentum among the particles. For example, a finite spherical system which approxi-mately satisfies the viral theorem, contracts slowlycompared to the crossing time ~ ()12G ρ- due to the evaporation of high energy particles [3] and the lack of equipartition among particles of different masses [4]. We consider here a thermodynamic description for the sys-tem (universe). The universe is considered to be an infi-nite gas in which each gas molecule is treated to be agalaxy. The gravitational force is a binary interaction and as a result a number of particles cluster together. We use the same approximation of binary interaction for our universe (system) consisting of large number of galaxies clustering together under the influence of gravitational force. It is important to mention here that the characteri-zation of this clustering is a problem of current interest. The physical validity of the application of thermody-namics in the clustering of galaxies and galaxy clusters has been discussed on the basis of N-body computer simulation results [5]. Equations of state for internal energy U and pressure P are of the form [6]:(3122NTU =-)b (1) (1NTP V=-)b (2) b defines the measuring correlation parameter and is dimensionless, given by [8]()202,23W nb Gm n T r K Tτξ∞=-=⎰,rdr (3)W is the potential energy and K the kinetic energy ofthe particles in a system. n N V = is the average num-ber density of the system of particles each of mass m, T is the temperature, V the volume, G is the universalgravitational constant. (),,n T r ξ is the two particle correlation function and r is the inter-particle distance. An overall study of (),n T r ξ has already been dis-cussed by [7]. For an ideal gas behaviour b = 0 and for non-ideal gas system b varies between 0 and 1. Previ-ously some workers [7,8] have derived b in the form of:331nT b nT ββ--=+ (4) Eq.4 indicates that b has a specific dependence on the combination 3nT -.3. ENTROPY CALCULATIONSThermodynamics and statistical mechanics have been found to be equal tools in describing entropy of a system. Thermodynamic entropy is a non-conserved state func-tion that is of great importance in science. Historically the concept of entropy evolved in order to explain why some processes are spontaneous and others are not; sys-tems tend to progress in the direction of increasing en-tropy [9]. Following statistical mechanics and the work carried out by [10], the grand canonical partition func-tion is given by()3213212,1!N N N N mkT Z T V V nT N πβ--⎛⎫⎡=+ ⎪⎣Λ⎝⎭⎤⎦(5)where N! is due to the distinguishability of particles. Λrepresents the volume of a phase space cell. N is the number of paricles (galaxies) with point mass approxi-mation. The Helmholtz free energy is given by:ln N A T Z =- (6)Thermodynamic description of entropy can be calcu-lated as:,N VA S T ∂⎛⎫=- ⎪∂⎝⎭ (7)The use of Eq.5 and Eq.6 in Eq.7 gives()3120ln ln 13S S n T b b -⎛⎫-=-- ⎪ ⎪⎝⎭- (8) where S 0 is an arbitary constant. From Eq.4 we write()31bn b T β-=- (9)Using Eq.9, Eq.8 becomes as3203ln S S b bT ⎡⎤-=-+⎢⎣⎦⎥ (10)Again from Eq.4All Rights Reserved.N. Iqbal et al. / Natural Science 3 (2011) 65-68 6767()13221n b T b β-⎡⎤=⎢⎣⎦⎥ (11)with the help of Eq.11, Eq.10 becomes as()011ln ln 1322S S n b b b ⎡-=-+-+⎡⎤⎣⎦⎢⎥⎣⎦⎤ (12) This is the expression for entropy of a system consist-ing of point mass particles, but actually galaxies have extended structures, therefore the point mass concept is only an approximation. For extended mass structures we make use of softening parameter ε whose value is taken between 0.01 and 0.05 (in the units of total radius). Following the same procedure, Eq.8 becomes as()320ln ln 13N S S N T N b Nb V εε⎡⎤-=---⎢⎥⎣⎦(13)For extended structures of galaxies, Eq.4 gets modi-fied to()()331nT R b nT R εβαεβαε--=+ (14)where α is a constant, R is the radius of a cell in a phase space in which number of particles (galaxies) is N and volume is V . The relation between b and b ε is given by: ()11b b b εαα=+- (15) b ε represents the correlation energy for extended mass particles clustering gravitationally in an expanding uni-verse. The above Eq.10 and Eq.12 take the form respec-tively as;()()3203ln 111bT b S S b b ααα⎡⎤⎢⎥-=-+⎢⎥+-+-⎢⎥⎣⎦1 (16) ()()()120113ln ln 2111b b b S S n b b ααα⎡⎤-⎡⎤⎢⎥⎣⎦-=-++⎢⎥+-+-⎢⎥⎣⎦1 (17)where2R R εεεα⎛⎫⎛⎫=⎪ ⎪⎝⎭⎝⎭(18)If ε = 0, α = 1 the entropy equations for extended mass galaxies are exactly same with that of a system of point mass galaxies approximation. Eq.10, Eq.12, Eq.16and Eq.17 are used here to study the entropy changes inthe cosmological many body problem. Various entropy change results S – S 0 for both the point mass approxima-tion and of extended mass approximation of particles (galaxies) are shown in (Figures 1and2). The resultshave been calculated analytically for different values ofFigure 1. (Color online) Comparison of isothermal entropy changes for non-point and point mass particles (galaxies) for an infinite gravitating system as a function of average relative temperature T and the parameter b . For non-point mass ε = 0.03 and R = 0.06 (left panel), ε = 0.04 and R = 0.04 (right panel).All Rights Reserved.N. Iqbal et al. / Natural Science 3 (2011) 65-68 68Figure 2. (Color online) Comparison of equi-density entropy changes for non-point and point mass particles (galaxies) for an infinite gravitating system as a function of average relative density n and the parameter b. For non-point mass ε= 0.03 and R = 0.04.R (cell size) corresponding to different values of soften-ing parameter ε. We study the variations of entropy changes S – S0with the changing parameter b for differ-ent values of n and T. Some graphical variations for S – S0with b for different values of n = 0, 1, 100 and aver-age temperature T = 1, 10 and 100 and by fixing value of cell size R = 0.04 and 0.06 are shown. The graphical analysis can be repeated for different values of R and by fixing values of εfor different sets like 0.04 and 0.05. From both the figures shown in 1 and 2, the dashed line represents variation for point mass particles and the solid line represents variation for extended (non-point mass) particles (galaxies) clustering together. It has been ob-served that the nature of the variation remains more or less same except with some minor difference.4. RESULTSThe formula for entropy calculated in this paper has provided a convenient way to study the entropy changes in gravitational galaxy clusters in an expanding universe. Gravity changes things that we have witnessed in this research. Clustering of galaxies in an expanding universe, which is like that of a self gravitating gas increases the gases volume which increases the entropy, but it also increases the potential energy and thus decreases the kinetic energy as particles must work against the attrac-tive gravitational field. So we expect expanding gases to cool down, and therefore there is a probability that the entropy has to decrease which gets confirmed from our theoretical calculations as shown in Figures 1 and 2. Entropy has remained an important contributor to our understanding in cosmology. Everything from gravita-tional clustering to supernova are contributors to entropy budget of the universe. A new calculation and study of entropy results given by Eqs.10, 12, 16 and 17 shows that the entropy of the universe decreases first with the clustering rate of the particles and then gradually in-creases as the system attains viral equilibrium. The gravitational entropy in this paper furthermore suggests that the universe is different than scientists had thought.5. ACKNOWLEDGEMENTSWe are thankful to Interuniversity centre for Astronomy and Astro-physics Pune India for providing a warm hospitality and facilities during the course of this work.REFERENCES[1]Voit, G.M. (2005) Tracing cosmic evolution with clus-ters of galaxies. Reviews of Modern Physics, 77, 207- 248.[2]Rief, F. (1965)Fundamentals of statistical and thermalphysics. McGraw-Hill, Tokyo.[3]Spitzer, L. and Saslaw, W.C. (1966) On the evolution ofgalactic nuclei. Astrophysical Journal, 143, 400-420.doi:10.1086/148523[4]Saslaw, W.C. and De Youngs, D.S. (1971) On the equi-partition in galactic nuclei and gravitating systems. As-trophysical Journal, 170, 423-429.doi:10.1086/151229[5]Itoh, M., Inagaki, S. and Saslaw, W.C. (1993) Gravita-tional clustering of galaxies. Astrophysical Journal, 403,476-496.doi:10.1086/172219[6]Hill, T.L. (1956) Statistical mechanics: Principles andstatistical applications. McGraw-Hill, New York.[7]Iqbal, N., Ahmad, F. and Khan, M.S. (2006) Gravita-tional clustering of galaxies in an expanding universe.Journal of Astronomy and Astrophysics, 27, 373-379.doi:10.1007/BF02709363[8]Saslaw, W.C. and Hamilton, A.J.S. (1984) Thermody-namics and galaxy clustering. Astrophysical Journal, 276, 13-25.doi:10.1086/161589[9]Mcquarrie, D.A. and Simon, J.D. (1997) Physical chem-istry: A molecular approach. University Science Books,Sausalito.[10]Ahmad, F, Saslaw, W.C. and Bhat, N.I. (2002) Statisticalmechanics of cosmological many body problem. Astro-physical Journal, 571, 576-584.doi:10.1086/340095[11]Freud, P.G. (1970) Physics: A Contemporary Perspective.Taylor and Francis Group.[12]Khinchin, A.I. (1949) Mathamatical Foundation of statis-tical mechanics. Dover Publications, New York.[13]Frampton, P., Stephen, D.H., Kephar, T.W. and Reeb, D.(2009) Classical Quantum Gravity. 26, 145005.doi:10.1088/0264-9381/26/14/145005All Rights Reserved.。
Dark matter and structure formation a review
a r X i v :0801.1091v 1 [a s t r o -p h ] 7 J a n 2008Dark matter,density perturbations and structure formationA.Del Popolo 1,2,31Bo ˘g azi ¸c i University,Physics Department,80815Bebek,Istanbul,Turkey2Dipartimento di Matematica,Universit`a Statale di Bergamo,via dei Caniana,2,24127,Bergamo,ITALY 3Istanbul Technical University,Ayazaga Campus,Faculty of Science and Letters,34469Maslak/ISTANBUL,TurkeyAbstract —-This paper provides a review of the variants of dark matter which are thought to be fundamental components of the universe and their role in origin and evolution of structures and some new original results concerning improvements to the spherical collapse model.In particular,I show how the spherical collapse model is modified when we take into account dynamical friction and tidal torques.1.INTRODUCTIONThe origin and evolution of large scale structure is today the outstanding problem in cosmology.This is the most fundamental question we can ask about the universe whose solution should help us to better understand problems as the epoch of galaxy formation,the clustering in the galaxy distribution,the amplitude and form of anisotropies in the microwave background radiation.Several has been the ap-proaches and models trying to attack and solve this problem:no one has given a final answer.The leading idea of all structure formation theories is that structures was born from small perturbations in the other-wise uniform distribution of matter in the early Universe,which is supposed to be,in great part,dark (matter not detectable through light emission).With the term Dark Matter cosmologists indicate an hypothetic material component of the universe which does not emit directly electromagnetic radiation (unless it decays in particles having this property ([1],but also see [2])).Dark matter,cannot be revealed directly,but nevertheless it is necessary to postulate its existence in order to explain the discrepancies between the observed dynamical proper-ties of galaxies and clusters of galaxies and the theoretical predictions based upon models of these objects assuming that the only matter present is the visible one.If in the space were present a diffused material component having gravitational mass,but unable to emit electromagnetic radiation in significative quantity,this discrepancy could be eliminated ([3]).The study of Dark Matter has as its finality the explanation of formation of galaxies and in general of cosmic structures.For this reason,in the last decades,the origin of cosmic structures has been “framed”in models in which Dark Matter constitutes the skeleton of cosmic structures and supply the most part of the mass of which the same is made.There are essentially two ways in which matter in the universe can be revealed:by means of radiation,by itself emitted,or by means of its gravitational interaction with baryonic matter which gives rise to cosmic structures.Electromagnetic radiation permits to reveal only baryonic matter.In the second case,we can only tell that we are in presence of matter that interacts by means of gravitation with the luminous mass in the universe.The original hypotheses on Dark Matter go back to measures performed by Oort ([4])of the surface density of matter in the galactic disk,which was obtained through the study of the stars motion in direction orthogonal to the galactic plane.The result obtained by Oort,which was after him named “Oort Limit”,gave a value of ρ=0.15M 0pc −3for the mass density,and a mass,in the region studied,superior to that present in stars.Nowadays,we know that the quoted discrepancy is due to the presence of HI in the solarclusters (a Cluster)and the total mass contained in galaxies of the same clusters.These and other researches from the thirties to now,have confirmed that a great part of the mass in the universe does not emit radiation that can be directly observed.1.1Determination of Ωand Dark MatterThe simplest cosmological model that describes,in a suf-ficient coherent manner,the evolution of the universe,from 10−2s after the initial singularity to now,is the so called Standard Cosmological Model (or Hot Big Bang model).It is based upon the Friedmann-Robertson-Walker (FRW)met-ric,which is given by:ds 2=c 2dt 2−a (t )2dr 22g ik R =−8πGa 2˙a 2+k3ρ(4)2¨a a 2+k2 the components of the today universe are galaxies.If weassume that galaxies motion satisfy Weyl([9])postulate,the velocity vector of a galaxy is given by u i=(1,0,0,0),and then the system behaves as a system made of dust forwhich we have p=0.Only two of the three Friedmannequations are independent,because thefirst connectsdensity,ρto the expansion parameter a(t).The characterof the solutions of these equations depends on the valueof the curvature parameter,k,which is also determinedby the initial conditions by means of Eq. 3.The solutionto the equations now written shows that ifρis largerthanρc=3H2ρc .In this case,theconditionΩ=1corresponds to k=0,Ω<1corresponds to k=−1,andΩ>1corresponds to k=1.1The value ofΩcan be calculated in several ways.The most common methods are the dynamical methods,in which the effects of gravity are used,and kinematics methods sensible to the evolution of the scale factor and to the space-time geometry.The results obtained forΩwith these different methods are summarized in the following.Dynamical methods:(a)Rotation curves:The contribution of spiral galaxies to the density in the universe is calculated by using their rotation curves and the third Kepler ing the last it is possible to obtain the mass of a spiral galaxy from the equation:M(r)=v2r/G(6) where v is the velocity of a test particle at a distance r from the center and M(r)is the mass internal to the circular orbit of the particle.In order to determine the mass M is necessary to have knowledge of the term v2in Eq.(6)and this can be done from the study of the rotation curves through the21cm line of HI.Rotation curves of galaxies are characterized by a peak reached at distances of some Kpcs and a behavior typicallyflat for the regions at distance larger than that of the peak.A peculiarity is that the expected Keplerian fall is not observed.This result is consistent with extended haloes containing masses till10times the galactic mass observed in the optical ([10]).The previous result is obtained assuming that the halo mass obtained with this method is distributed in a spherical region so that we can use Eq.(6)and that we neglect the tidal interaction with the neighboring galaxies which tend to produce an expansion of the halo.After M and the luminosity of a series of elliptical galaxies is determined,the contribution to the density of the universeL>ℓwhereℓis the luminosity per unit volume due to galaxies and can be obtained from the galactic luminosity functionφ(L)dL,which describes the number of galaxies per Mpc3and luminosity range L,L+dL.The value that is usually assumed forℓis ℓ=2.4h108L bo Mpc−3.The arguments used lead to a value ofΩg for the luminous parts of spiral galaxies ofΩg≤0.01, while for haloesΩh≥0.03−0.1.The result shows that the halo mass is noteworthy larger than the galactic mass observable in the optical([11]).(b)Virial theorem:In the case of non spiral galaxies and clusters,the mass can be obtained using the virial theorem2T+V=0,withT∼=3c≈Ω0.6λρ(9) ([13]).Then given the overdensityδρρcan be ob-tained from the overdensity of galaxiesδn gρ=δn g3 (d)Kinematic methods:These methods are based upon the use of relations be-tween physical quantities dependent on cosmological param-eters.An example of those relations is the relation luminos-ity distance-redshift:H0d L=z+1F the luminosity distance,L the absolute luminos-ity,and F theflux.By means of the relations luminosity-redshift,angle-redshift,number of objects-redshift,it is possible to determine the parameter of deceleration q0=−¨a0a0=100hkm/Mpcs are the scale factor and the Hubble constant,nowadays).At the same time q0is connected toΩby means of q0=Ω•Growth rate offlparisons of presentday structure withfluctuations at the last scatteringof the cosmic microwave background(CMB)or withhigh redshift objects of the young universe.The methods and current estimates are summarized in Table3.The estimates based on virialized objects typi-cally yield low values ofΩm∼0.2−0.3.The global mea-sures,large-scale structure and cosmicflows typically indi-cate higher valuesofΩm∼0.4−1.Bahcall et al.([17]),showed that the evolution of the number density of rich clusters of galaxies breaks the degen-eracy betweenΩ(the mass density ratio of the universe)and σ8(the normalization of the power spectrum),σ8Ω0.5≃0.5, that follows from the observed present-day abundance of rich clusters.The evolution of high-mass(Coma-like)clus-ters is strong inΩ=1,low-σ8models(such as the standard biased CDM model withσ8≃0.5),where the number den-sity of clusters decreases by a factor of∼103from z=0 to z≃0.5;the same clusters show only mild evolution in low-Ω,high-σ8models,where the decrease is a factor of ∼10.This diagnostic provides a most powerful constraint onΩ.Using observations of clusters to z≃0.5−1,the authors found only mild evolution in the observed cluster abundance,andΩ=0.3±0.1andσ8=0.85±0.15(for Λ=0models;forΩ+Λ=1models,Ω=0.34±0.13). ferreira et al.([18]),proposed an alternative method to estimate v12directly from peculiar velocity samples,which contain redshift-independent distances as well as galaxy red-shifts.In contrast to other dynamical measures which de-termineβ≡Ω0.6σ8,this method can provide an estimate of Ω0.6σ28for a range ofσ8whereΩis the cosmological density parameter,whileσ8is the standard normalization for the power spectrum of densityfluctuations.Melchiorri([19]),used the angular power spectrum of the Cosmic Microwave Background,measured during the North American testflight of the BOOMERANG experiment,to constrain the geometry of the universe.Within the class of Cold Dark Matter models,theyfind that the overall frac-tional energy density of the universe,Ω,is constrained to be0.85≤Ω≤1.25at the68%confidence level. Branchini([20]),compared the density and velocityfields as extracted from the Abell/ACO clusters to the corre-spondingfields recovered by the POTENT method from the Mark III peculiar velocities of galaxies.Quantitative comparisons within a volume containing∼12independent samples yieldβc≡Ω0.6/b c=0.22±0.08,where b c is the cluster biasing parameter at15h−1Mpc.If b c∼4.5,as in-dicated by the cluster correlation function,their result is consistent withΩ∼1.(f)Inflation:It is widely supposed that the very early universe experi-enced an era of inflation(see[21],[22],[13]).By‘inflation’one means that the scale factor has positive acceleration,¨a>0,corresponding to repulsive gravity and3p<−ρ. During inflation aH=˙a is increasing,so that comoving scales are leaving the horizon(Hubble distance)rather than entering it,and it is supposed that at the beginning of in-flation the observable universe was well within the horizon. The inflationary hypothesis is attractive because it holds out the possibility of calculating cosmological quantities, given the Lagrangian describing the fundamental interac-tions.The Standard Model,describing the interactions up to energies of order1T eV,is not viable in this context be-cause it does not permit inflation,but this should not be re-garded as a serious setback because it is universally agreed4mology.The nature of the required extension is not yet known,though it is conceivable that it could become known in the foreseeable future.But even without a specific model of the interactions(ie.,a specific Lagrangian),the inflation-ary hypothesis can still offer guidance about what to expect in cosmology.More dramatically,one can turn around the theory-to-observation sequence,to rule out otherwise rea-sonable models.The importance of inflation is connected to:a)the origin of density perturbations,which could origi-nate during inflation as quantumfluctuations,which be-come classical as they leave the horizon and remain so on re-entry.The original quantumfluctuations are of exactly the same type as those of the electromagneticfield,which give rise to the experimentally observed Casimir effect. b)One of the most dramatic and simple effects is that there is nofine-tuning of the initial value of the density parame-terΩ=8πρ/3m2P l H2.From the Friedmann equation,Ωis given byΩ−1=(K3An argument has been given forΩ0very close to1on the basis of effects on the cmb anisotropy from regions far outside the observable simplest one([21])invokes a scalarfield,termed the infla-tonfield.An alternative([23])is to invoke a modification of Einstein gravity,and combinations of the two mecha-nisms have also been proposed.During inflation however, the proposed modifications of gravity can be abolished by redefining the spacetime metric tensor,so that one recovers the scalarfield case.We focus on it for the moment,but modified gravity models will be included later in our survey of specific models.In comoving coordinates a homogeneous scalarfieldφwith minimal coupling to gravity has the equation of motion¨φ+3H˙φ+V′(φ)=0(13) Its energy density and pressure areρ=V+12˙φ2(15)If such afield dominatesρand p,the inflationary condition 3p<ρis achieved provided that thefield rolls sufficiently slowly,˙φ2<V(16)Practically all of the usually considered models of inflation satisfy three conditions.First,the motion of thefield is overdamped,so that the‘force’V′balances the‘friction term’3H˙φ,˙φ≃−116π V′38π8πV′′5 in which they are satisfied and we are adopting that nomen-clature here.Practically all of the usually considered modelsof inflation satisfy the slow-roll conditions more or less well.It should be noted that thefirst slow-roll condition is ona quite different footing from the other two,being a state-ment about the solution of thefield equation as opposed toa statement about the potential that defines this equation.What we are saying is that in the usually considered modelsone can show that thefirst condition is an attractor solu-tion,in a regime typically characterized by the other twoconditions,and that moreover reasonable initial conditionsonφwill ensure that this solution is achieved well beforethe observable universe leaves the horizon.It is importantto remember that there are strong observational limits forthe parameters previously introduced(e.g.ǫ,η).For ex-ample[27]studied the possible contribution of a stochasticgravitational wave background to the anisotropy of the cos-mic microwave background in cold and mixed dark matter(CDM and MDM)models.This contribution was testedagainst detections of CMB anisotropy at large and inter-mediate angular scales.The bestfit parameters(i.e.thosewhich maximize the likelihood)are(with95%confidence)n S=1.23+0.17−0.15andR(n S)=C T2π2f(n S)=2.4+3.4−2.2(23)wheref(n S)=Γ(3−n S)Γ(3+n SΓ2(4−n S2)(24)The previous constraintfixes the value ofǫas well that ofη2η=n s−1+2ǫ(25) Theyfind that by including the possibility of such back-ground in CMB data analysis it can drastically alter the conclusion on the remaining cosmological parameters.More stringent constraints on some of the previous parameters are given in section1.12.(h)Conclusions:We have seen the possible values ofΩusing different meth-ods.We have to add that Cosmologists are“attracted”by a value ofΩ0=1.This value ofΩis requested by infla-tionary theory.The previous data lead us to the following hypotheses:i)Ω0<0.12;in this case one can suppose that the uni-verse is fundamentally made of baryonic matter(black holes; Jupiters;white dwarfs).ii)Ω0>0.12;in this case in order to have aflat universe,it is necessary a non-baryonic component.Ωb=1is excluded by several reasons(see[28],[13].The remaining possibilities are:1)existence of a smooth component withΩ=0.8.The test of a smooth component can be done with kinematic methods.2)Existence of a cosmological term,absolutely smooth to whom correspond an energy densityρvac=Λsthe number of particles per unit comoving volume and we remember that n is the number density of species and s the entropy density, we obtain a contribution of the species to the actual density of the universe asΩh2=0.28Y(T f)(m6limits([13]).The solution to the problem was proposed by Peccei-Quinn in1977([36])in terms of a spontaneous sym-metry breaking scheme.To this symmetry breaking should be associated a Nambu-Goldstone boson:the axion.Theaxion mass ranges between10−12ev-1Gev.In cosmology there are two ranges of interest:10−6ev≤m a≤10−3ev; 3ev≤m a≤8ev.Axion production in the quoted range can originate due to a series of astrophysical processes([13])and several are the ways these particles can be detected. Nevertheless the effort of researchers expecially in USA, Japan and Italy,axions remain hypothetical particles. They are in any case the most important CDM candidates.In the following,I am going to speak about the basic ideas of structure formation.I shall write about density perturbations,their spectrum and evolution,about correla-tion functions and their time evolution,etc.1.3Origin of structuresObserving our universe,we notice a clear evidence of in-homogeneity when we consider small scales(Mpcs).In clus-ters density reaches values of103times larger than the av-erage density,and in galaxies it has values105larger than the average density([13]).If we consider scales larger than 102Mpcs universe appears isoptric as it is observed in the radio-galaxies counts,in CMBR,in the X background([11]). The isotropy at the decoupling time,t dec,at which matter and radiation decoupled,universe was very homogeneous, as showed by the simple relation:δρT(28)([13])4.The difference between the actual universe and that at decoupling is evident.The transformation between a highly homogeneous universe,at early times,to an highly local non homogeneous one,can be explained supposing that at t dec were present small inhomogeneities which grow up because of the gravitational instability mechanism([37]). Events leading to structure formation can be enumerated as follows:(a)Origin of quantumfluctuations at Planck epoch.(b)Fluctuations enter the horizon and they grow linearly till recombination.(c)Perturbations grow up in a different way for HDM and CDM in the post-recombination phase,till they reach the non-linear phase.(d)Collapse and structure formation.Before t dec inhomogeneities in baryonic components could not grow because photons and baryons were strictly cou-pled.This problem was not present for the CDM compo-nent.Then CDM perturbations started to grow up before those in the baryonic component when universe was mat-ter dominated.The epoch t eq≈4.4∗1010(Ω0h2)−2sec,at which matter and radiation density are almost equal,can be considered as the epoch at which structures started to form.The study of structure formation is fundamentally an initial value problem.Data necessary for starting this study are:1)Value ofΩ0.In CDM models the value chosen for this parameter is1,in conformity with inflationary theory pre-dictions.2)The values ofΩi for the different components in the uni-verse.For example in the case of baryons,nucleosynthesis gives us the limit0.014≤Ωb≤0.15whileΩW IMP S≈0.9.3)The perturbation spectrum and the nature of pertur-bations(adiabatic or isocurvature).The spectrum gener-ally used is that of Harrison-Zeldovich:P(k)=Ak n with n=1.The perturbation more used are adiabatic or curva-ture.This choice is dictated from the comparison between theory and observations of CMBR anisotropy.1.4The spectrum of density perturbationIn order to study the distribution of matter density in the universe it is generally assumed that this distribution is given by the superposition of plane waves independently evolving,at least until they are in the linear regime(this means till the overdensityδ=ρ−ρthe average density in the volume and withρ(r)the density in r,it is possible to define the density contrast as:δ(r)=ρ(r)−l(and similar conditions for the other components)and for the periodicity conditionδ(x,y,L)=δ(x,y,0)(and similar conditions for the other components). Fourier coefficientsδk are complex quantities given by:δk=1σ2)(32)([28]).The quantityσthat is present in Eq.(32)is the variance of the densityfield and is defined as:σ2=<δ2>= k<|δk|2>=1(2π)3 P(k)d3k=17It can be defined as the joint probability of finding an over-density δin two distinct points of space:ξ(r ,t )=<δ(r ,t )δ(r +x ,t )>(35)([38]),where averages are averageson anensemble obtainedfromseveralrealizations ofuniverse.Correlation functioncan be expressed as the joint probability of finding a galaxy in a volume δV 1and another in a volume δV 2separated by a distance r 12:δ2P =n 2V [1+ξ(r 12)]δV 1δV 2(36)where n V is the average number of galaxies per unit volume.The concept of correlation function,given in this terms,can be enlarged to the case of three or more points.Correlation functions have a fundamental role in the study of clustering of matter.If we want to use this function for a complete description of clustering,one needs to know the correlation functions of order larger than two ([39]).By means of correlation functions it is possible to study the evolution of clustering.The correlation functions are,in fact,connected one another by means of an infinite system of equations obtained from moments of Boltzmann equa-tion which constitutes the BBGKY (Bogolyubov-Green-Kirkwood-Yvon)hierarchy ([40]).This hierarchy can be transformed into a closed system of equation using closure conditions.Solving the system one gets information on cor-relation functions.In order to show the relation between perturbation spec-trum and two-points correlation function,we introduce inEq.(35),Eq.(30),recalling that δ∗k =δ(−k )and taking the limit V u →∞,the average in the Eq.(35)can be expressed in terms of the integral:ξ(r )=12π2k 2P (k )sin (kr )b (t p )2T 2(k ;t f )P (k ;t p )(39)where b(t)is the law of grow of perturbations,in the linear regime.In the case of CDM models the transfer function is:T (k )= 1+ ak +(bk )1.5+(ck )2 ν−1S=3ρr−δρmT−δρm8The distribution function f that appears in the previous equations cannot be obtained from observations.It is possi-ble to measure moments of f (density,average velocity,etc.).We want now to obtain the evolution equations for δ.Forthis reason,we start integrating Eq.(44)on p and after using Eq.(43),we get:a 3ρb∂δa 2▽p fd 3p =0(45)If we define velocity as:v =pfd 3p(46)and introduce it in Eq.(45)we get:ρb ∂δa▽(ρv )=0(47)We can now multiply Eq.(44)for p and integrate it on the momentum:∂ma 2∂βp αp βfd 3p +a 3ρ(x ,t )φ,α=0(48)this last in Eq.(45)leaves us with:∂2δa ∂δa2▽[(1+δ)▽φ]+1ma 2fd 3p(50)the equation for the evolution of overdensity becomes:∂2δa ∂δa 2▽[(1+δ)▽φ]+1∂t 2+2˙a ∂t=4πGρb δ(52)This equation in an Einstein-de Sitter universe (Ω=1,Λ=0)has the solutions:δ+=A +(x )t2a 2=82(1−Ω0)(cosh η−1)(55)t (η)=Ω0a 2=823t.(57)Before concluding this section,we want to find an ex-pression for the velocity field in the linear ingthe equation of motion p =ma 2˙x ,d pdt+v ˙a a=Gρb ad 3xδ(x ,t )x −x ′4π∂|x ′−x |(59)([38]).This solution is valid just as that for δin the linear regime.At time t =t 0this regime is valid on scales larger than 8h −1Mpc .1.7Non-linear phaseLinear evolution is valid only if δ<<1or similarly,if the mass variance,σ,is much less than unity.When this condi-tion is no longer verified (e.g.,if we consider scales smaller than 8h −1Mpc),it is necessary to develope a non-linear theory.In regions smaller than 8h −1Mpc galaxies are not a Poisson distribution but they tend to cluster.If one wants to study the properties of galactic structures or clusters of galaxies,it is necessary to introduce a non-linear theory of clustering.A theory of this last item is too complicated to be developed in a purely theoretical fashion.The problem can be faced assuming certain approximations that simpli-fies it ([47])or as often it is done,by using N-Body simu-lations of the interesting system.The approximations are often used to furnish the initial data to simulations.In the simulations,a large number of particles are randomly dis-tributed in a sphere,in the points of a cubic grid,in order to eliminate small scale noise.The initial spectrum is ob-tained perturbing the initial positions by means of a super-position of plane waves having random distributed phases and wave vector ([48]).Obviously,the universe is considered in expansion (or comoving coordinates are used),and then the equation of motion of particles are numerically solved.For what concerns the analytical approximations one of the most used is that of [47].This gives a solution to the prob-lem of the grow of perturbations in an universe with p =0not only in the linear regime but even in the mildly non-linear regime.In this approximation,one supposes to have particles with initial position given in Lagrangian coordi-nates q .The positions of particles,at a given time t,are given by:9 where x indicates the Eulerian coordinates,p(q)describesthe initial densityfluctuations and b(t)describes their growin the linear phase and it satisfies the equation:d2bdtdadt =dbρ ∂q jρ δjk+b(t)∂p k3p(q)= k i k3exp(i kq)(67)([28]),that leads us back to the linear theory.In other words,Ze‘ldovich approximation is able to reproduce the linear theory,and is also able to give a good approximationin regions withδρρ>>ing the expression for p(q),theJacobian in Eq.(64)is a real matrix and symmetric that can be diagonalized.With this p(q)the perturbed density can be written as:ρ(q,t)=(1−b(t)λ1(q))(1−b(t)λ2(q))(1−b(t)λ3(q))(68) whereλ1,λ2,λ3are the three eigenvalues of the Jacobian, describing the expansion and contraction of mass along the principal axes.From the structure of the last equation,we notice that in regions of high density Eq.(68)becomes infinite and the structure of collapse in a pancake,in a filamentary structure or in a node,according to values of eigenvalues.Some N-body simulations([49])tried to ver-ify the prediction of Ze‘ldovich approximation,using initial conditions generated using a spectrum with a cut-offat low frequencies.The results showed a good agreement between theory and simulations,for the initial phases of the evolu-tion(a(t)=3.6).Going on,the approximation is no more valid starting from the time of shell-crossing.After shell-crossing,particles does not oscillate any longer around the structure but they pass through it making it vanish.This problem has been partly solved supposing that particles, before reaching the singularity they sticks the one on the other,due to a dissipative term that simulates gravity and then collects on the forming structure.This model is known as“adesion-model”([50]).Summarizing,Zel’dovich approximation gives a description of the transition between linear and non-linear phase.It 1.8Quasi-linear regimeWe have seen in the previous section that in the case of regions of dimension smaller than8h−1Mpc,the linear theory is no more a good approximation and a new theory is needed or N-body simulations.Non-linear theory is able to calculate quantities as the formation redshift of a given class of objects as galaxies and clusters,the number of bound objects having masses larger than a given one,the average virial velocity and the correlation function.It is possible to get an estimate of the given quantities as that of other not cited,using an intermediate theory between the linear and non-linear theory:the quasi-linear theory. This last is obtained adding to the linear theory a model of gravitational collapse,just as the spherical collapse model.Important results that the theory gives is the bottom-up formation of structures(in the CDM model). Other important results are obtained if we identify density peaks in linear regime with sites of structure formation. Two important papers in the development of this theory are[51]and that of[52].This last paper is an application of the ideas of the quasi-linear theory to the CDM model. The principles of this approach are the following:•Regions of mass larger than M that collapsed can be identified with regions where the density contrast evolved according to linear regime,δ(M,x),has a value larger than a threshold,δc.•After collapse regions does not fragment.The major drawbacks of the theory,as described in[52]are fundamentally the fact that the estimates that can be ob-tained by means of this theory depends on the threshold δc,on the ratio between thefiltering mass and that of ob-jects and from other parameters.Nevertheless,this theory has helped cosmologists in obtaining estimate of important quantities as those previously quoted,and at same time give evidences that leads to exclude very low values for spectrum normalization.1.9Spherical CollapseSpherical symmetry is one of the few cases in which grav-itational collapse can be solved exactly([53];[38]).In fact, as a consequence of Birkhoff’s theorem,a spherical pertur-bation evolves as a FRW Universe with density equal to the mean density inside the perturbation.The simplest spherical perturbation is the top-hat one, i.e.a constant overdensityδinside a sphere of radius R; to avoid a feedback reaction on the background model,the overdensity has to be surrounded by a spherical underdense shell,such to make the total perturbation vanish.The evo-lution of the radius of the perturbation is then given by a Friedmann equation.The evolution of a spherical perturbation depends only on its initial overdensity.In an Einstein-de Sitter background, any spherical overdensity reaches a singularity(collapse)at afinal time:t c=3π3δ(t i) −3/2t i.(69) By that time its linear density contrast reaches the value:3/2。
英语词源中一些广为流传的故事
英语词源中一些广为流传的故事1.An Apple of Discord争斗之源;不和之因;祸根An Apple of Discord直译为“纠纷的苹果”,出自荷马史诗Iliad中的希腊神话故事传说希腊阿耳戈英雄(Argonaut)珀琉斯(Peleus)和爱琴海海神涅柔斯的女儿西蒂斯(Thetis)在珀利翁山举行婚礼,大摆宴席。
他们邀请了奥林匹斯上(Olympus)的诸神参加喜筵,不知是有意还是无心,惟独没有邀请掌管争执的女神厄里斯(Eris)。
这位女神恼羞成怒,决定在这次喜筵上制造不和。
于是,她不请自来,并悄悄在筵席上放了一个金苹果,上面镌刻着“属于最美者”几个字。
天后赫拉(Hera),智慧女神雅典娜(Athena)、爱与美之神阿芙罗狄蒂(Aphrodite),都自以为最美,应得金苹果,获得“最美者”称号。
她们争执不下,闹到众神之父宙斯(Zeus)那里,但宙斯碍于难言之隐,不愿偏袒任何一方,就要她们去找特洛伊的王子帕里斯(Paris)评判。
三位女神为了获得金苹果,都各自私许帕里斯以某种好处:赫拉许给他以广袤国土和掌握富饶财宝的权利,雅典娜许以文武全才和胜利的荣誉,阿芙罗狄蒂则许他成为世界上最美艳女子的丈夫。
年青的帕里斯在富贵、荣誉和美女之间选择了后者,便把金苹果判给爱与美之神。
为此,赫拉和雅典娜怀恨帕里斯,连带也憎恨整个特洛伊人。
后来阿芙罗狄蒂为了履行诺言,帮助帕里斯拐走了斯巴达国王墨涅俄斯的王后——绝世美女海伦(Helen),从而引起了历时10年的特洛伊战争。
不和女神厄里斯丢下的那个苹果,不仅成了天上3位女神之间不和的根源,而且也成为了人间2个民族之间战争的起因。
因此,在英语中产生了an apple of discord这个成语,常用来比喻any subject of disagreement and contention;the root of the trouble;dispute等意义这个成语最初为公元2世纪时的古罗马历史学家马克·朱里·尤斯丁(Marcus Juninus Justinus)所使用,后来广泛的流传到欧洲许多语言中去,成为了一个国际性成语。
小学上册I卷英语第一单元综合卷[有答案]
小学上册英语第一单元综合卷[有答案]英语试题一、综合题(本题有100小题,每小题1分,共100分.每小题不选、错误,均不给分)1.What is the name of the fairy tale character who climbed a beanstalk?A. JackB. JillC. HanselD. Gretel答案:A2.Which one is a vegetable?A. AppleB. CarrotC. BananaD. Grape答案:B3.The __________ (历史的趋势) can inform policymaking.4. A ______ (蜥蜴) can change colors to blend in.5.h Revolution began in _______. (1789年) The Fren6. A cat loves to chase _______ and play.7.What is 2 x 3?A. 5B. 6C. 7D. 8答案:B8. A solution with a low concentration of solute is said to be _______.9.My dad inspires me to be __________ (勇敢的) in life.10.The __________ (历史的重构) allows for fresh interpretations.11.The gas we breathe in is called ______.12. A caterpillar turns into a ______.13.My uncle is a fantastic __________ (厨师).14.My favorite game is ______ (tag).15.My sister is a passionate __________ (科学爱好者).16.What is the name of the famous detective created by Arthur Conan Doyle?A. Hercule PoirotB. Miss MarpleC. Sherlock HolmesD. Sam Spade答案:C17.What is the largest continent on Earth?A. AfricaB. AsiaC. EuropeD. Antarctica18.What is the capital city of Saudi Arabia?A. RiyadhB. JeddahC. MeccaD. Medina19.I enjoy going to the ______ (博物馆) with my family. We learn about history and see ______ (古老的东西).20. A _____ (自然景观) can inspire artists.21.The city of Muscat is the capital of _______.22.What is the capital of Vietnam?A. HanoiB. Ho Chi Minh CityC. Da NangD. Nha Trang23.The ________ (植物体) functions harmoniously.24.The boy is a good ________.25.I like to have fun with my ____.26.在中国,________ (traditions) 如端午节和中秋节有着深厚的文化意义。
send your name to mars
send your name to marsMy name is Liu Xiyu and I am sending it all the way to Mars!It is an exciting and momentous milestone in space exploration when human beings can come into contact with other planets, and I am very honored to be part of this incredible journey to the Red Planet. During the years of long studied and research, scientists has been trying to furthering our understanding of our solar system and making human beings’ dream come true. Now this dream of NASA is working hand in hand with the advancement in technology, We can see the light of our dreams flicker in the darkness of stars in the night sky.After countless experiments, preparation and planning over the decades, it is now time for the next big step.To send my name to Mars. I am incredibly excited to be part of this journey to Mars and to send my name alongside other thousands of names as part of this mission. I take this opportunity to make history and possibly leave my mark in the universe.It is certainly no ordinary mission that we are finally sending my name to Mars. This is the first ever journey into the unknown, specifically tailoredto explore the Red Planet. The Mars mission is expected to launch in July or August of 2020 from the Kennedy Space Center in Florida.I am sure that I will never forget the feeling of inspiration and adventure when my name is finally in space.I feel so honored to be part of the mission that is going to take us one step closer to our understanding of the planets in the universe.My name is now forever connected to the universe, leaving a legacy that will last for generations. I say a final farewell to my name as it is to be sent to a whole new world, willing and ready to be explored. Sending my name to Mars is a remarkable and unforgettable event that I, Liu Xiyu, will take to heart for all eternity.。
Unit 6 Space and Beyond Starting out 课件
our solar system. • _J_u_p_i_te_r__ is a gas giant, which is the biggest and spins the fastest. • _S_a_t_u_r_n__ is a gas giant and Titan is its biggest moon. • _U__ra_n_u_s__ is an icy gas giant, the coldest planet in the solar system. • _N_e_p_t_u_n_e_ is an icy gas giant, which is the farthest planet from the
Look at the timeline and answer the questions.
3. What do you know about China’s future plans for space exploration?
Answer the questions after watching.
2. Where are the Asteroid Belt and the Kuiper Belt in the solar system?
The Asteroid Belt lies between Mars and Jupiter. The Kuiper Belt exists just beyond the orbit of Neptune.
Rocket
Manned /unmanned spacecraft
小学上册第二次英语第五单元综合卷[有答案]
小学上册英语第五单元综合卷[有答案]英语试题一、综合题(本题有50小题,每小题1分,共100分.每小题不选、错误,均不给分)1 Photosynthesis is the process by which plants convert sunlight into ______.2 What is the main function of the heart?A. DigestionB. CirculationC. RespirationD. Excretion答案: B3 What is the capital city of Japan?A. OsakaB. KyotoC. TokyoD. Hiroshima答案:C4 The first human to break the sound barrier was ______ (查尔斯·杨)。
5 The mouse is afraid of the _________ (猫).6 What do you call the act of making something dirty?A. CleaningB. MessingD. Organizing答案: C7 What is the opposite of clear?A. CloudyB. DirtyC. OpaqueD. Foggy8 I like to ______ at the library. (read)9 Astronomy clubs often host _______ nights for stargazing.10 My friend is a ______. She loves to act in plays.11 (64) is the fastest river in the world. The ____12 What do you call the person who studies the stars?A. GeologistB. AstronomerC. BiologistD. Chemist13 What do you call the person who plays a musical instrument?A. ArtistB. MusicianC. PerformerD. Composer答案:B14 The process of condensation is the opposite of _______.15 Which of these is a primary color?B. OrangeC. PurpleD. Blue答案: D16 What color is the grass?A. BlueB. GreenC. YellowD. Red答案:B17 My dad drives a ______ (car).18 My favorite game is ______ (象棋).19 The _______ (狮子) is king of the jungle.20 What is the process of a caterpillar turning into a butterfly called?A. MetamorphosisB. EvolutionC. TransformationD. Development答案:A21 The chemical formula for sodium acetate is ______.22 My favorite type of ________ (饮品) is lemonade.23 Which of these can fly?A. DogB. CatD. Fish24 Which instrument has keys and is played by pressing them?A. GuitarB. ViolinC. PianoD. Drums答案: C. Piano25 The owl hunts for _______ (食物) at night.26 What is the capital of the Bahamas?A. NassauB. FreeportC. Marsh HarbourD. George Town答案: A27 The _______ has deep roots in the ground.28 We can play ________ (游戏名称) with our ________ (玩具).29 The ancient city of Rome is known for its _______.30 My dad teaches me how to ride a ____ (bike).31 What do we call the person who studies geology?A. GeologistB. BiologistC. ChemistD. Physicist32 The ______ is a skilled photographer.33 What instrument is used to measure temperature?A. BarometerB. ThermometerC. SpeedometerD. Altimeter34 The ________ (symposium) features experts.35 What is the symbol for silver?A. AgB. AuC. PbD. Fe36 Temperature measures how hot or ______ something is.37 What do we call the place where we can see many different kinds of fish?A. AquariumB. ZooC. MuseumD. Park答案: A38 What shape is a stop sign?A. CircleB. TriangleC. SquareD. Octagon39 What is the primary function of leaves?A. To absorb waterB. To make foodC. To support the plantD. To store nutrients答案:B40 We should respect all _____ (自然环境).41 The baby likes to play with ___. (toys)42 I enjoy watching the _______ (小动物) at the zoo.43 I watch the clouds float across the ______ (天空).44 What is the name of the famous flower known for its beauty and scent?A. RoseB. TulipC. LilyD. Daffodil答案:A45 What do you call the process of watering plants?A. IrrigationB. CultivationC. FertilizationD. Pruning46 des were a series of religious ________ (战争). The Dead47 What do we call a baby sheep?A. KidB. LambC. CalfD. Foal答案:B48 The invention of ________ changed how people interact.49 What is the color of an orange?A. BlueB. OrangeC. GreenD. Purple答案:B50 What do we call the study of the relationships between organisms and their environments?a. Ecologyb. Biologyc. Zoologyd. Botany答案:a51 I see a ___ (car/truck) on the road.52 The __________ is a famous city known for its beaches and resorts. (迈阿密)53 What is the capital of Thailand?A. BangkokB. HanoiC. ManilaD. Kuala Lumpur54 She is a friendly ________.55 The baby is _____ in its crib. (sleeping)56 The __________ (历史博物馆) preserves artifacts.57 What color do you get when you mix red and white?A. BlueB. PinkC. PurpleD. Green答案:B58 The flowers are _____ in the sunshine. (smiling)59 What is the name of the famous art museum in Paris?A. Louvre MuseumB. Musée d'OrsayC. Centre PompidouD. Musée de l'Orangerie答案: A. Louvre Museum60 The ______ (小鸟) is perched on a ______ (电线), singing a sweet song.61 What is the main ingredient in bread?A. FlourB. SugarC. RiceD. Salt62 My pet _____ loves to cuddle.63 I saw a ladybug on a ______.64 What is the visible surface of the sun called?A. CoreB. AtmosphereC. PhotosphereD. Chromosphere65 I enjoy playing ______ (桌面游戏) with my family.66 What is the name of the animal that can change its color?A. ChameleonB. TigerC. ElephantD. Lion答案: A67 Which planet is known as the Blue Planet?A. MarsB. EarthC. NeptuneD. Uranus答案:B68 Butterflies come from ______.69 The ant carries food much larger than its own ______ (身体).70 The ancient Greeks contributed to the development of _____ and science.71 How many wheels does a bicycle have?A. 1B. 2C. 3D. 4答案: B. 272 What is the name of the famous American actress known for "The Devil Wears Prada"?A. Anne HathawayB. Meryl StreepC. Emily BluntD. Sandra Bullock答案:B73 My favorite game is ________ (国际象棋). I play it with my ________ (兄弟).74 What sound does a cow make?A. MeowB. MooC. BarkD. Quack答案: B75 What do you call a person who studies the weather?A. MeteorologistB. ClimatologistC. GeologistD. Historian答案:A76 My brother is known for his __________ (幽默感).77 I love to ________ with my family.78 ________ (植物生长调控) is studied in labs.79 Which fruit is green on the outside and red on the inside?A. KiwiB. WatermelonC. GrapesD. Peach答案: B. Watermelon80 The _____ (植物发展) plays a role in global food security.81 What is the currency used in the USA?A. EuroB. DollarC. PoundD. Yen82 What is the name of the sweet substance produced by bees?A. Maple SyrupB. HoneyC. JamD. Molasses答案:B83 The parrot mimics sounds it hears from ______ (主人).84 The atomic weight of an element is measured in ______.85 An indicator is a substance that changes color in response to _____.86 The ________ loves to play.87 An ant is very _______ (勤劳).88 The chemical symbol for calcium is _______.89 What is the name of the famous ship that sank in 1912?A. Queen MaryB. TitanicC. LusitaniaD. Britannic90 The __________ (历史的深度) enriches insight.91 I like to go ________ on Sundays.92 The sky is _______ (明亮的) today.93 What is the capital of Nepal?A. KathmanduB. PokharaC. BiratnagarD. Lalitpur94 What do we call a person who studies climate?A. ClimatologistB. MeteorologistC. Environmental ScientistD. Ecologist答案: A95 When I was younger, my favorite toy was a ________ (玩具名). I played with it every day until it broke. Then, I felt very ________ (形容词).96 A _____ (鸟) sings beautifully every morning in the tree.97 What do we call a large area of land with grass?A. ForestB. PrairieC. DesertD. Swamp98 What do you call a person who studies plants?A. BotanistB. ZoologistC. EcologistD. Biologist答案:A99 My dad is very _______ (形容词) about his hobbies. 他总是 _______ (动词). 100 How many hours are in a day?A. 12B. 24C. 36D. 48。
小学上册第11次英语第一单元期中试卷
小学上册英语第一单元期中试卷英语试题一、综合题(本题有100小题,每小题1分,共100分.每小题不选、错误,均不给分)1.The __________ is cool and refreshing during the summer. (海洋)2.I like to play with my ________ under the sun.3.What is the name of the famous American author known for his horror stories?A. Edgar Allan PoeB. Mark TwainC. Ernest HemingwayD. F. Scott Fitzgerald答案:A4.What is the capital of Afghanistan?A. KabulB. KandaharC. HeratD. Mazar-i-Sharif答案:A5.What is the capital of France?A. LondonB. BerlinC. ParisD. Rome答案:C6.What is the name of the famous landmark in Sydney?A. Opera HouseB. Harbour BridgeC. Bondi BeachD. Uluru答案:A7.What is the name of the famous explorer known for his voyages to the New World?A. Ferdinand MagellanB. Christopher ColumbusC. Marco PoloD. Vasco da Gama8.I love to watch ______ cartoons.9.Planting trees is a great way to combat ______ (全球变暖).10. A cactus can survive in _____ (干旱) conditions.11.The __________ (历史的图景) paints a broad picture.12.The chemical formula for lithium hydroxide is _______.13.Which of these animals can swim?A. CatB. DogC. FishD. Bird14.What is the color of a stop sign?A. GreenB. YellowC. BlueD. Red15.The chemical formula for table salt is ______.16.What is the name of the famous river in Egypt?A. NileB. AmazonC. YangtzeD. Mississippi答案:A17.What is the name of the bright star in the night sky?A. MoonB. SunC. SiriusD. North Star18.The chemical symbol for chromium is ______.19.__________ are important for the production of synthetic materials.20.What is the opposite of "day"?A. NightB. NoonC. MorningD. Evening答案:A Night21.I find ________ (历史) fascinating and exciting.22.How many seconds are in a minute?A. 30B. 60C. 90D. 120答案:B23.What is the primary color of a fire?A. YellowB. RedC. OrangeD. All of the above答案:D All of the above24.What do you call a person who makes clothes?A. DesignerB. TailorC. StylistD. Seamstress答案:B25. A substance that donates electrons is called a ______ agent.26.We will go _____ (shopping/working) tomorrow.27.The Earth's surface is shaped by both gradual and ______ changes.28.What do we call the act of building trust?A. Confidence-BuildingB. ReliabilityC. CredibilityD. All of the Above答案:D29.The capital of Trinidad and Tobago is ________ (特立尼达和多巴哥的首都是________).30.The capital of Vanuatu is _______.31.What is the sound of a sheep?A. MeowB. BarkC. BaaD. Moo答案:C32.My favorite animal is a ______ (海豹) because they are playful.33.What is the name of the famous American holiday celebrated with fireworks?A. ThanksgivingB. Independence DayC. Labor DayD. Memorial Day34.The _______ (The War in Afghanistan) began in 2001 following the 9/11 attacks.35.What do we call the natural habitat of an organism?A. EcosystemB. EnvironmentC. NicheD. Community答案:C36.What do we celebrate on July 4th in the United States?A. ThanksgivingB. Independence DayC. ChristmasD. Halloween37.My friend is very __________ (有天赋).38.Chemical changes often involve the formation or breaking of ________.39.The ancient Sumerians are credited with creating the first system of ______ (文字).40.I have a collection of toy _____ from around the world.41.What is the largest organ in the human body?A. HeartB. BrainC. SkinD. Liver答案:C Skin42.The __________ (历史的文化传递) enriches society.43.My brother is a ______. He wants to be an astronaut.44.My dog has a loud _______ (叫声).45.The process of breaking down glucose is called ______.46.The chemical formula for ytterbium chloride is _____.47.The __________ (历史的推动) inspires change.48.We make _____ (沙拉) for lunch.49.Tectonic plates float on the ______ layer of the Earth.50.I love to watch _____ (小动物) explore their surroundings.51.The first American flag was sewn by _______ Ross.52.The Great Fire of London destroyed much of the city in ________.53. A compound that can donate protons is called an ______.54.Neutralization reactions produce water and a _____.55.The ancient Egyptians invented _______ for writing. (象形文字)56.The stars are _______ (在闪烁).57.My sister wants a pet ______ (小狗).58.What do we call the person who creates software?A. EngineerB. ProgrammerC. ScientistD. Designer59.I can’t wait to try out my new __________ (玩具名).60.I like to draw _____ in my sketchbook.61. A solution that contains a weak base is called a ______ solution.62.The element with atomic number is __________.63.The ______ is the center of an atom.64.The ______ (田野) is full of blooming flowers.65.What is the name of the famous American holiday celebrated in December?A. ChristmasB. ThanksgivingC. New Year'sD. Independence Day答案:A66.My cousin is a great __________ (手工艺者).67. A solution that contains more solute than it can hold is called a _____ solution.68.What do you call a large, thick jungle?A. ForestB. SavannaC. RainforestD. Woodland答案:C69.What is the name of the famous clock tower in London?A. Big BenB. Eiffel TowerC. Statue of LibertyD. Colosseum答案:A70.The Magna Carta was signed in _______.71.She has a ________ (great) sense of humor.72.The __________ was a significant period of change in Europe. (文艺复兴)73.What is the color of a clear sky?A. GrayB. BlueC. WhiteD. Black74.My ___ (小狗) loves to cuddle.75. A ______ (鱼) can be colorful and beautiful.76.What is the capital of Tajikistan?A. DushanbeB. KhujandC. KulobD. Bokhtar77.I like to watch the _____ (蚂蚁) working together to build their home. 我喜欢看蚂蚁一起工作,建造它们的家。
小学下册第九次英语第3单元测验试卷
小学下册英语第3单元测验试卷考试时间:90分钟(总分:140)A卷一、综合题(共计100题共100分)1. 填空题:A __________ (绿色化学) aims to reduce environmental impact through sustainable practices.2. 选择题:What is the name of the famous river in Egypt?A. AmazonB. NileC. MississippiD. Yangtze答案:B. Nile3. 填空题:My mom is a __________ (心理健康顾问).4. 选择题:Which food is made from milk?A. BreadB. CheeseC. RiceD. Pasta答案:B5. 选择题:What is the name of the process of making ice cream?A. WhippingB. ChurningC. StirringD. Cooking答案:B6. 填空题:I find ________ (药物) very interesting.How many zeros are in one hundred?A. OneB. TwoC. ThreeD. Four8. 填空题:I have a robot ____ that does tricks. (玩具名称)9. 填空题:A parrot can ________________ (说话).10. 填空题:The ______ (植物的适应性) is vital in changing climates.11. 填空题:I love going to ______ (夏令营) during the summer. It’s a chance to make new friends and try new activities.12. 填空题:The country known for pyramids and pharaohs is ________ (埃及).13. 选择题:What is the name of the famous American civil rights activist known for her role in the Montgomery Bus Boycott?A. Rosa ParksB. Harriet TubmanC. Michelle ObamaD. Angela Davis答案: A. Rosa Parks14. 填空题:I love listening to ______ (音乐) while doing my homework. It helps me concentrate and feel ______ (愉快).15. 听力题:I see _____ (clouds/stars) in the sky.16. 选择题:What is the largest planet in our Solar System?A. SaturnB. JupiterC. EarthD. MarsI like to climb trees and look at _______ (我喜欢爬树,看_______).18. 填空题:Planting _____ (香料) can enhance our cooking.19. 听力题:The capital of Ghana is __________.20. 填空题:Did you see the _____ (小鸟) taking a bath?21. 选择题:What is the name of the story about a girl who befriends seven dwarfs?A. CinderellaB. Snow WhiteC. RapunzelD. Aladdin答案: B22. 听力题:The chemical symbol for nitrogen is ______.23. 听力题:A beaker is a common piece of ______ glassware.24. y of Paris ended the War of ________ (1812). 填空题:The Trea25. 选择题:What do we call a person who creates jewelry?A. JewelerB. GoldsmithC. SilversmithD. Artisan答案: A26. 填空题:The __________ was a movement that changed art and culture in Europe. (文艺复兴)27. 选择题:How many legs does a dog have?A. 2B. 3C. 4D. 5The _____ (森林) is home to diverse plant life.29. 填空题:The ancient Greeks created the concept of ______ (哲学).30. 选择题:What do you call a person who studies history?A. HistorianB. ArchaeologistC. AnthropologistD. Sociologist答案:A31. 填空题:The parrot mimics sounds from its ______ (主人).32. 选择题:What is a group of stars called?A. GalaxyB. UniverseC. Solar SystemD. Constellation答案: D33. 听力题:The gas released during photosynthesis is ______.34. 选择题:What do you call a fear of spiders?A. ArachnophobiaB. ClaustrophobiaC. AcrophobiaD. Agoraphobia答案: A35. 选择题:What is the name of the sweet food made from chocolate and nuts?A. FudgeB. CandyC. BrownieD. Cookie答案: CWhich gas do we breathe in?A. Carbon DioxideB. NitrogenC. OxygenD. Helium37. 填空题:Turtles are very _______ (慢).38. 填空题:We planted a ________ in our backyard.39. 选择题:What is the opposite of 'fast'?A. QuickB. SlowC. RapidD. Speedy答案:B40. 填空题:The _____ (大象) is known for its intelligence.41. 听力题:The ____ is a fierce predator found in the wild.42. 填空题:I love visiting museums to see ________ (古董) toys from the past. They tell a ________ (故事).43. 填空题:I like to create adventures with my toy ________ (玩具名称).44. 填空题:The first person to fly solo across the Atlantic was ______ (厄哈特).45. 填空题:My friend is very __________ (机智).46. 填空题:I love to design my own _________ (玩具) for my friends.47. 填空题:I want to be a __________ (作家) when I grow up.What is the name of the famous scientist known for his contributions to chemistry?A. Antoine LavoisierB. Dmitri MendeleevC. Robert BoyleD. Marie Curie答案: A49. 选择题:What is the chemical formula for table salt?A. NaClB. KClC. CaCO3D. NaHCO3答案: A50. 听力题:I like to _______ (play) the drums.51. 选择题:What is the process of turning a liquid into a solid called?A. MeltingB. FreezingC. BoilingD. Evaporating答案: B52. 填空题:I enjoy creating art with my _________ (玩具颜料).53. 填空题:The _____ (狐狸) is clever and sly.54. 选择题:What is the name of the famous painting by Vincent van Gogh?A. The Last SupperB. Starry NightC. Mona LisaD. The Scream答案:B55. 选择题:What do you call a person who studies stars?A. BiologistB. AstronomerC. ChemistD. Geologist答案:B56. 填空题:A _______ (金鱼) can live for many years.57. 选择题:How many states are there in the United States?A. 48B. 50C. 52D. 54答案: B58. 选择题:What is the main source of energy for the Earth?A. MoonB. StarsC. SunD. Wind59. 填空题:The signing of the Treaty of Versailles ended ________.60. 填空题:We should protect our _____ (自然) environment.61. 听力题:The element with the symbol Ti is __________.62. 选择题:What do we call a young male horse?A. ColtB. FoalC. FillyD. Stallion答案:A63. 填空题:Australia is known as the __________. (大洋洲)64. 填空题:My mom enjoys _______ (动词) during the weekends. 她会 _______ (动词).The ______ (小鸟) finds a safe spot to rest in the tree.66. 填空题:The __________ (历史的社会构成) shapes our identities.67. 填空题:A _______ (鲨鱼) is a powerful predator.68. 听力题:The ______ helps protect the body from bacteria.69. 选择题:What do we call the place where you go to see animals?A. ZooB. FarmC. AquariumD. Circus70. 填空题:_____ (sunflowers) follow the sun across the sky.71. 填空题:I made a ________ out of paper for the school project.72. 听力题:The antelope runs swiftly, dodging predators in the ____.73. 填空题:I like to _______ (与朋友一起)去健身房。
Mars_the_red_planet
Earth and Mars Comparison
Image Courtesy of NASA/JPL-Caltech
The Mars Global Surveyor
The Mars Global Surveyor left Earth on Nov. 7, 1996, and arrived at Mars on Sept. 12, 1997. Its mission was extended several times until NASA lost contact with it in 2006. MGS mapped the planet from pole to pole, revealing many ancient signs of water, such as gullies and hematite (a mineral that forms in water).
Viking
This color picture of the Martian horizon was taken by Viking 1 on July 24, 1976.
1990s: Better, faster, cheaper
(FBC missions)
Mars Observer launched to the planet on Sept. 25, 1992. It was lost just before it was supposed to achieve orbit on Aug. 21, 1993. The loss was painful ,in 1990s dollars, it was supposed to cost $212 million. The final tally was estimated at $813 million. This was one of the factors that sparked a new move within NASA to create ―better, faster, cheaper‖ (FBC) missions that would take advantage of advanced computer electronics and new team management techniques to reduce costs.
2013年考研外语阅读理解第三篇全文翻译
2013年考研外语阅读理解第三篇全文翻译注释:未来总是隐藏在迷雾中,借助已有的知识推测未来贯穿于整个已知的和我可以预见的人类文明史,尤其在工业化和信息化革命大幅度提升人类改造自然的能力并带来相当严重的后果之后,注重实证的西方科学体系甚至产生了过去干脆叫神棍的未来学。
人类的未来如何,甚至于人类能否存在到下个世纪甚至下个十年,争议一直不断,但我始终相信一点,在明天,在黑暗之后,太阳照常升起the sun rises as usual。
我在本文翻译中大量使用了意译,并在后面给出了直译,强烈提示,意译是一种很高的翻译技巧,按照考研判分的标准,如果采用意译,基本可以肯定是要么满分要么零分,如果自己的水平没有足够的把握,绝不要轻易使用。
Up until a few decades ago, our visions of the future were largely - though by no means uniformly - glowingly positive. Science and technology would cure all the ills of humanity, leading to lives offulfillment and opportunity for all.曾经,人类的未来似乎一片光明(意译,直译为前景辽阔,蒸蒸日上,只是发展各异)。
科技的发展必定能治愈顽疾,满足需求,提供契机。
Now utopia has grown unfashionable, as we have gained a deeper appreciation of the range of threats facing us, from asteroid strike to epidemic flu and to climate change. You might even be tempted to assume that humanity has little future to look forward to.然而如今梦想已成灰(utopia乌托邦,unfashionable过时的),我们要面对的是更可怕的现实,彗星撞地球、重度流感,甚至气候变更。
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From ARIES to MARS:Transaction Support forNext-Generation,Solid-State DrivesJoel Coburn∗Trevor Bunker∗Meir Schwarz Rajesh Gupta Steven SwansonDepartment of Computer Science and EngineeringUniversity of California,San Diego{jdcoburn,tbunker,rgupta,swanson}@AbstractTransaction-based systems often rely on write-ahead log-ging(W AL)algorithms designed to maximize perfor-mance on disk-based storage.However,emerging fast, byte-addressable,non-volatile memory(NVM)technolo-gies(e.g.,phase-change memories,spin-transfer torque MRAMs,and the memristor)present very different perfor-mance characteristics,so blithely applying existing algo-rithms can lead to disappointing performance.This paper presents a novel storage primitive,called editable atomic writes(EAW),that enables sophisticated, highly-optimized W AL schemes in fast NVM-based stor-age systems.EAWs allow applications to safely access and modify log contents rather than treating the log as an append-only,write-only data structure,and we demonstrate that this can make implementating complex transactions simpler and more efficient.We use EAWs to build MARS,a W AL scheme that provides the same as features ARIES[26] (a widely-used W AL system for databases)but avoids mak-ing disk-centric implementation decisions.We have implemented EAWs and MARS in a next-generation SSD to demonstrate that the overhead of EAWs is minimal compared to normal writes,and that they pro-vide large speedups for transactional updates to hash tables, B+trees,and large graphs.In addition,MARS outperforms ARIES by up to3.7×while reducing software complexity.∗Now working at Google Inc.Permission to make digital or hard copies of part or all of this work for personal or classroom use is granted without fee provided that copies are not made or distributed for profit or commercial advantage and that copies bear this notice and the full citation on thefirst page.Copyrights for third-party components of this work must be honored.For all other uses,contact the Owner/Author.Copyright is held by the Owner/Author(s).SOSP’13,Nov.3–6,2013,Farmington,Pennsylvania,USA.ACM978-1-4503-2388-8/13/11./10.1145/2517349.25227241IntroductionEmerging fast non-volatile memory(NVM)technologies, such as phase change memory,spin-torque transfer memory, and the memristor promise to be orders of magnitude faster than existing storage technologies(i.e.,disks andflash). Such a dramatic improvement shifts the balance between storage,system bus,main memory,and CPU performance and will force designers to rethink storage architectures to maximize application performance by exploiting the speed of these memories.Recent work focuses on optimizing read and write performance in these systems[6,7,41].But these new memory technologies also enable new approaches to ensuring data integrity in the face of failures.File systems,databases,persistent object stores,and other applications rely on strong consistency guarantees for per-sistent data structures.Typically,these applications use some form of transaction to move the data from one con-sistent state to another.Most systems implement transac-tions using software techniques such as write-ahead logging (WAL)or shadow paging.These techniques use sophisti-cated,disk-based optimizations to minimize the cost of syn-chronous writes and leverage the sequential bandwidth of disk.For example,WAL-based systems write data to a log before updating the data in-place,but they typically delay the in-place updates until they can be batched into larger se-quential writes.NVM technologies provide very different performance characteristics,and exploiting them requires new ap-proaches to providing transactional guarantees.NVM stor-age arrays provide parallelism within individual chips,be-tween chips attached to a memory controller,and across memory controllers.In addition,the aggregate bandwidth across the memory controllers in an NVM storage array will outstrip the interconnect(e.g.,PCIe)that connects it to the host system.This paper presents a novel WAL scheme,called Modified ARIES Redesigned for SSDs(MARS),optimized for NVM-based storage.The design of MARS reflects an examination of ARIES[26],a popular W AL-based recovery algorithm for databases,in the context of these new memories.MARS provides the same high-level features for implementing effi-cient and robust transactions as ARIES,but without any of the disk-based design decisions ARIES incorporates.To support MARS,we designed a novel multi-part atomic write primitive,called editable atomic writes(EAW).An EAW consists of a set of redo log entries,one per object to be modified,that the application can freely update mul-tiple times in-place in the log prior to commit.Once com-mitted,the SSD hardware copies thefinal values from the log to their target locations,and the copy is guaranteed to succeed even in the presence of power or host system fail-ures.EAWs make implementing ARIES-style transactions simpler and faster,giving rise to MARS.EAWs are also a useful building block for other applications that must pro-vide strong consistency guarantees.The EAW interface supports atomic writes to multiple portions of the storage array without alignment or size re-strictions,and the hardware shoulders the burden for log-ging and copying data to enforce atomicity.This interface safely exposes the logs to the application and allows it to manage the log space directly,providing theflexibility that sophisticated W AL schemes like MARS require.In con-trast,recent work on atomic write support forflash-based SSDs[29,30]hides the logging in theflash translation layer (FTL).Consequently,ARIES-style logging schemes must write data to both a software-accessible log and to itsfinal destination,resulting in higher bandwidth consumption and lower performance.We implemented EAWs in a prototype PCIe-based stor-age array[6].Microbenchmarks show that they reduce latency by2.9×compared to using normal synchronous writes to implement a traditional W AL protocol,and EAWs increase effective bandwidth by between2.0and3.8×by eliminating logging pared to non-atomic writes,EAWs reduce effective bandwidth just1-8%and in-crease latency by just30%.We use EAWs to implement MARS,to implement sim-ple on-disk persistent data structures,and to modify Mem-cacheDB[10],a persistent version of memcached.MARS improves performance by3.7×relative to our baseline ver-sion of ARIES.EAWs speed up our ACID key-value stores based on a hash table and a B+tree by1.5×and1.4×,re-spectively,relative to a software-based version,and EAWs improve performance for a simple online scale-free graph query benchmark by1.3×.Furthermore,performance for EAW-based versions of these data structures is only15% slower than non-transactional versions.For MemcacheDB, replacing Berkeley DB with an EAW-based key-value store improves performance by up to3.8×.The remainder of this paper is organized as follows.In Section2,we describe the memory technologies and storage system that our work targets.Section3examines ARIES in the context of fast NVM-based storage and describes EAWs and MARS.Section4describes our implementation of EAWs in hardware.Section5evaluates EAWs and their impact on the performance of MARS and other persistent data structures.Section6places this work in the context of prior work on support for transactional storage.In Section7, we discuss the limitations of our approach and some areas for future work.Section8summarizes our contributions. 2Storage technologyFast NVMs will catalyze changes in the organization of stor-age arrays and in how applications and the OS access and manage storage.This section describes the architecture of the storage system that our work targets and the memory technologies it uses.Section4describes our implementa-tion in more detail.Fast non-volatile memories such as phase-change mem-ories(PCM)[3],spin-transfer torque[15]memories,and the memristor differ fundamentally from conventional disks and from theflash-based SSDs that are beginning to replace them.The most important features of NVMs are their per-formance(relative to disk andflash)and their simpler inter-face(relative toflash).Predictions by industry[19]and academia[3,15]suggest that NVMs will have bandwidth and latency characteristics similar to DRAM.This means they will be between500and 1500×faster thanflash and50,000×faster than disk.In addition,technologies such as PCM will have a significant density and cost-per-bit advantage(estimated2to4×)over DRAM[3,33].These device characteristics require storage architectures with topologies and interconnects capable of exploiting their low latency and high bandwidth.Modern high-end SSDs often attach to the host via PCIe, and this approach will work well for fast NVMs too.PCIe bandwidth is scalable and many high end processors have nearly as much PCIe bandwidth as main memory band-width.PCIe also offers scalable capacity since any num-ber and type of memory channels(and memory controllers) can sit behind a PCIe endpoint.This makes a PCIe-attached architecture a natural candidate for capacity-intensive appli-cations like databases,graph analytics,or caching.Mul-tiple hosts can also connect to a single device over PCIe, allowing for increased availability if one host fails.Finally, the appearance of NVMExpress[27]-based SSDs(e.g.,In-tel’s Chatham NVMe drive[11])signals that PCIe-attached SSDs are a likely target design for fast NVMs in the near term.A consequence of PCIe SSDs’scalable capacity is that their internal memory bandwidth will often exceed their PCIe bandwidth(e.g.,8:1ratio in our prototype SSD).Un-likeflash memory where many chips can hang off a single bus,the low latency of fast NVMs requires minimal loading on data buses connecting chips and memory controllers.As a result,large capacity devices must spread storage across many memory channels.This presents an opportunity to ex-ploit this surfeit of internal bandwidth by offloading tasks to the storage device.Alternately,fast NVMs can attach directly to the proces-sor’s memory bus,providing the lowest latency path to stor-age and a simple,memory-like interface.However,reduced latency comes at a cost of reduced capacity and availability since the pin,power,and signaling constraints of a com-puter’s memory channels will limit capacity and fail-over will be impossible.In this work,we focus on PCIe-attached storage archi-tectures.Our baseline storage array is the Moneta-Direct SSD[6,7],which spreads64GB of DRAM across eight memory controllers connected via a high-bandwidth ring. Each memory controller provides4GB/s of bandwidth for a total internal bandwidth of32GB/s.An8-lane PCIe1.1 interface provides a2GB/s full-duplex connection(4GB/s total)to the host system.The prototype runs at250MHz on a BEE3FPGA prototyping system[2].The Moneta storage array emulates advanced non-volatile memories using DRAM and modified memory controllers that insert delays to model longer read and write latencies. We model phase-change memory(PCM)in this work and use the latencies from[23](48ns and150ns for reads and writes,respectively,to the memory array inside the memory chips).The techniques we describe would also work in STT-MRAM or memristor-based systems.Unlikeflash,PCM(as well as other NVMs)does not re-quire a separate erase operation to clear data before a write. This makes in-place updates possible and,therefore,elim-inates the complicatedflash translation layer that manages a map between logical storage addresses and physicalflash storage locations to provide the illusion of in-place updates. PCM still requires wear-leveling and error correction,but fast hardware solutions exist for both of these[31,32,35]. Moneta uses start-gap wear leveling[31].With fast,in-place updates,Moneta is able to provide low-latency,high-bandwidth access to storage that is limited only by the PCIe interconnect between the host and the device.3Complex Transaction Support in Fast SSDsThe design of ARIES and other data management systems (e.g.,journalingfile systems)relies critically on the atom-icity,durability,and performance properties of the underly-ing storage hardware.Data management systems combine these properties with locking protocols,rules governing the order of updates,and other invariants to provide application-level transactional guarantees.As a result,the semantics and performance characteristics of the storage hardware play a key role in determining the implementation complexity and overall performance of the complete system.We have designed a novel multi-part atomic write prim-itive,called editable atomic writes(EAW),that supports complex logging protocols like ARIES-style write-ahead logging.In particular,EAWs make it easy to support transaction isolation in a scalable way while aggressively leveraging the performance of next-generation,non-volatile memories.This feature is missing from existing atomic write interfaces[29,30]designed to accelerate simpler transaction models(e.g.,file metadata updates in journaling file systems)onflash-based SSDs.This section describes EAWs,presents our analysis of ARIES and the assumptions it makes about disk-based stor-age,and describes MARS,our reengineered version of ARIES that uses EAWs to simplify transaction processing and improve performance.3.1Editable atomic writesThe performance characteristics of disks and,more recently, SSDs have deeply influenced most WAL schemes.Since se-quential writes are much faster than random writes,W AL schemes maintain their logs as append-only sets of records, avoiding long-latency seeks on disks and write amplifica-tion inflash-based SSDs.However,for fast NVMs,there is little performance difference between random and sequen-tial writes,so the advantages of an append-only log are less clear.In fact,append-and write-only logs add complexity because systems must construct and maintain in-memory copies that reflect the operations recorded in the log.For large database transactions the in-memory copies can ex-ceed available memory,forcing the database to spill this data onto disk.Consequently,the system may have three copies of the data at one time:one in the log,the spilled copy,and the data itself.However,if the log data resides in a fast NVM storage system,spilling is not necessary–the updated version of the data resides in the log and the sys-tem reads or updates it without interfering with other writes to the log.Realizing this capability requires a newflexi-ble logging primitive which we call editable atomic writes (EAW).EAWs use write-ahead redo logs to combine multiple writes to arbitrary storage locations into a single atomic op-eration.EAWs make it easy for applications to provide iso-lation between transactions by keeping the updates in a log until the atomic operation commits and exposing that log to the application so that a transaction can see its own updates and freely update that data multiple times prior to commit. EAWs are simple to use and strike a balance between imple-mentation complexity and functionality while allowing our SSD to leverage the performance of fast NVMs.EAWs require the application to allocate space for the log (e.g.,by creating a logfile)and to specify where the redo log entry for each write will reside.This avoids the need to statically allocate space for log storage and ensures that the application knows where the log entry resides so it can modify it as needed.The implementation of EAWs is spread across the storage device hardware and system software.Hardware support in the SSD is responsible for logging and copying data to guar-antee atomicity.Applications use the EAW library interface to perform common IO operations by communicating di-Command DescriptionLogWrite(TID,file,offset,data,len,logfile,logoffset)Record a write to the log at the specified log offset.After commit,copy the data to the offset in thefile.Commit(TID)Commit a transaction.AtomicWrite(TID,file,offset,data,len,logfile,logoffset)Create and commit a transaction containing asingle write.NestedTopAction(TID,logfile,logoffset)Commit a nested top action by applying the logfrom a specified starting point to the end.Abort(TID)Cancel the transaction entirely,or perform aPartialAbort(TID,logfile,logoffset)partial rollback to a specified point in the log.Table1:EA W commands.These commands perform multi-part atomic updates to the storage array and help support user-level transactions.rectly with hardware,but storage management policy deci-sions still reside in the kernel andfile system.Below,we describe how an application initiates an EAW, commits it,and manages log storage in the device.We also discuss how the EAW interface makes transactions robust and efficient by supporting partial rollbacks and nested top actions.Then,we outline how EAWs help simplify and accelerate ARIES-style transactions.In Sections4and5 we show that the hardware required to implement EAWs is modest and that it can deliver large performance gains. Creating transactions Applications execute EAWs us-ing the commands in Table1.Each application access-ing the storage device has a private set of64transaction IDs(TIDs)1,and the application is responsible for track-ing which TIDs are in use.TIDs can be in one of three states:F REE(the TID is not in use),P ENDING(the trans-action is underway),or C OMMITTED(the transaction has committed).TIDs move from C OMMITTED to F REE when the storage system notifies the host that the transaction is complete.To create a new transaction with TID,T,the application passes T to LogWrite along with information that spec-ifies the data to write,the ultimate target location for the write(i.e.,afile descriptor and offset),and the location for the log data(i.e.,a logfile descriptor and offset).This opera-tion copies the write data to the logfile but does not modify the targetfile.After thefirst LogWrite,the state of the transaction changes from F REE to P ENDING.Additional calls to LogWrite add new writes to the transaction.The writes in a transaction are not visible to other trans-actions until after commit.However,a transaction can read its own data prior to commit by explicitly reading from the locations in the log containing that data.After an initial LogWrite to a storage location,a transaction may update that data again before commit by issuing a(non-logging) 1This is not a fundamental limitation but rather an implementation de-tail of our prototype.Supporting more concurrent transactions increases resource demands in the FPGA implementation.A custom ASIC imple-mentation(quickly becoming commonplace in high-end SSDs)could eas-ily support100s of concurrent transactions.write to the corresponding log location.Committing transactions The application commits the transaction with Commit(T).In response,the storage ar-ray assigns the transaction a commit sequence number that determines the commit order of this transaction relative to others.It then atomically applies the LogWrite s by copy-ing the data from the log to their target locations.When the Commit command completes,the transaction has logically committed,and the transaction moves to the C OMMITTED state.If a system failure should occur after a transaction logically commits but before the systemfin-ishes writing the data back,then the SSD will replay the log during recovery to roll the changes forward.When log application completes,the TID returns to F REE and the hardware notifies the application that the transaction finished successfully.At this point,it is safe to read the updated data from its target locations and reuse the TID. Robust and efficient execution The EAW interface pro-vides four other commands designed to make transactions robust and efficient throughfiner-grained control over their execution.The AtomicWrite command creates and com-mits a single atomic write operation,saving one IO opera-tion for singleton transactions.The NestedTopAction command is similar to Commit but instead applies the log from a specified offset up through the tail and allows the transaction to continue afterwards.This is useful for opera-tions that should commit independent of whether or not the transaction commits(e.g.,extending afile or splitting a page in a B-tree),and it is critical to database performance under high concurrency.Consider an insert of a key into a B-tree where a page split must occur to make room for the key.Other concurrent insert operations might either cause an abort or be aborted themselves,leading to repeatedly starting and aborting a page split.With a NestedTopAction,the page split oc-curs once and the new page is immediately available to other transactions.The Abort command aborts a transaction,releasing all resources associated with it,allowing the applicationFeature BenefitsFlexible storage Supports varying length data managementFine-grained locking High concurrencyPartial rollbacks via Robust and efficient savepoints transactionsOperation logging High concurrency lock modes Recovery Simple and robust recovery independenceTable2:ARIES features.Regardless of the storage tech-nology,ARIES must provide these features to the rest of the system.to resolve conflicts and ensure forward progress.The PartialAbort command truncates the log at a specified location,or savepoint[16],to support partial rollback.Par-tial rollbacks are a useful feature for handling database in-tegrity constraint violations and resolving deadlocks[26]. They minimize the number of repeated writes a transaction must perform when it encounters a conflict and must restart. Storing the log The system stores the log in a pair of ordi-naryfiles in the storage device:a logfile and a log metadata file.The logfile holds the data for the log.The application creates the logfile just like any otherfile and is responsi-ble for allocating parts of it to LogWrite operations.The application can access and modify its contents at any time. The log metadatafile contains information about the tar-get location and log data location for each LogWrite.The contents of the log metadatafile are privileged,since it con-tains raw storage addresses rather thanfile descriptors and offsets.Raw addresses are necessary during crash recov-ery whenfile descriptors are meaningless and thefile sys-tem may be unavailable(e.g.,if thefile system itself uses the EAW interface).A system daemon,called the metadata handler,“installs”log metadatafiles on behalf of applica-tions and marks them as unreadable and immutable from software.Section4describes the structure of the log meta-datafile in more detail.Conventional storage systems must allocate space for logs as well,but they often use separate disks to improve perfor-mance.Our system relies on the log being internal to the storage device,since our performance gains stem from uti-lizing the internal bandwidth of the storage array’s indepen-dent memory banks.3.2Deconstructing ARIESThe ARIES[26]framework for write-ahead logging and recovery has influenced the design of many commercial databases and acts as a key building block in providing fast,flexible,and efficient ACID transactions.Our goal is to build a W AL scheme that provides all of ARIES’features but without the disk-centric design decisions.At a high level,ARIES operates as follows.Before mod-ifying an object(e.g.,a row of a table)in storage,ARIES records the changes in a persistent log.To make recovery ro-bust and to allow disk-based optimizations,ARIES records both the old version(undo)and new version(redo)of the data.ARIES can only update the data in-place after the log reaches storage.On restart after a crash,ARIES brings the system back to the exact state it was in before the crash by applying the redo log.Then,ARIES reverts the effects of any uncommitted transactions active at the time of the crash by applying the undo log,thus bringing the system back to a consistent state.ARIES has two primary goals:First,it aims to provide a rich interface for executing scalable,ACID transactions. Second,it aims to maximize performance on disk-based storage systems.ARIES achieves thefirst goal by providing several im-portant features to higher-level software(e.g.,the rest of the database),listed in Table2,that make it useful to a variety of applications.For example,ARIES offersflexible stor-age management by supporting objects of varying length. It also allows transactions to scale with the amount of free disk storage space rather than with available main memory. Features like operation logging andfine-grained locking im-prove concurrency.Recovery independence makes it possi-ble to recover portions of the database even when there are errors.Independent of the underlying storage technology, ARIES must export these features to the rest of the database. To achieve high performance on disk-based systems, ARIES incorporates a set of design decisions(Table3)that exploit the properties of disk:ARIES optimizes for long,se-quential accesses and avoids short,random accesses when-ever possible.These design decisions are a poorfit for fast NVMs that provide fast random access,abundant internal bandwidth,and ample parallelism.Below,we describe the design decisions ARIES makes that optimize for disk and how they limit the performance of ARIES on an NVM-based storage device.No-force In ARIES,the system writes log entries to the log(a sequential write)before it updates the object itself(a random write).To keep random writes off the critical path, ARIES uses a no-force policy that writes updated pages back to disk lazily after commit.In fast NVM-based stor-age,random writes are no more expensive than sequential writes,so the value of no-force is much lower.Steal ARIES uses a steal policy to allow the buffer man-ager to“page out”uncommitted,dirty pages to disk dur-ing transaction execution.This lets the buffer manager sup-port transactions larger than the buffer pool,group writes to-gether to take advantage of sequential disk bandwidth,and avoid data races on pages shared by overlapping transac-tions.However,stealing requires undo logging so the sys-tem can roll back the uncommitted changes if the transaction aborts.As a result,ARIES writes both an undo log and a redo log to disk in addition to eventually writing back the data inDesign option Advantage for disk Implementation Alternative for MARSNo-force Eliminate synchronous Flush redo log entries Force in hardwarerandom writes to storage on commit at memory controllers Steal Reclaim buffer space Write undo log entries before Hardware does in-place updates Eliminate random writes writing back dirty pages Log always holds latest copyAvoid false conflictsPages Simplify recovery and ARIES performs updates on pages Hardware uses pagesbuffer management Page writes are atomic Software operates on objects Log Sequence Simplify recovery ARIES orders updates to Hardware enforces ordering Numbers(LSNs)Enable high-level features storage using LSNs with commit sequence numbers Table3:ARIES design decisions.ARIES relies on a set disk-centric optimizations to maximize performance on disk-based storage.However,these optimizations are a poorfit for fast NVM-based storage,and we present alternatives to them in MARS.place.This means that,roughly speaking,writing one logi-cal byte to the database requires writing three bytes to stor-age.For disks,this is a reasonable tradeoff because it avoids placing random disk accesses on the critical path and gives the buffer manager enormousflexibility in scheduling the random disk accesses that must occur.For fast NVMs,how-ever,random and sequential access performance are nearly identical,so this trade-off needs to be re-examined. Pages and Log Sequence Numbers(LSNs)ARIES uses disk pages as the basic unit of data management and recov-ery and uses the atomicity of page writes as a foundation for larger atomic writes.This reflects the inherently block-oriented interface that disks provide.ARIES also embeds a log sequence number(LSN)in each page to establish an ordering on updates and determine how to reapply them dur-ing recovery.As recent work[37]highlights,pages and LSNs com-plicate several aspects of database design.Pages make it difficult to manage objects that span multiple pages or are smaller than a single page.Generating globally unique LSNs limits concurrency and embedding LSNs in pages complicates reading and writing objects that span multiple pages.LSNs also effectively prohibit simultaneously writ-ing multiple log entries.Advanced NVM-based storage arrays that implement EAWs can avoid these problems.The hardware motivation for page-based management does not exist for fast NVMs, so EAWs expose a byte-addressable interface with a much moreflexible notion of atomicity.Instead of an append-only log,EAWs provide a log that can be read and written throughout the life of a transaction.This means that undo logging is unnecessary because data will never be written back in-place before a transaction commits.Also,EAWs implement ordering and recovery in the storage array itself, eliminating the need for application-visible LSNs.3.3Building MARSMARS is an alternative to ARIES that implements the same features but reconsiders ARIES’design decisions in the context of fast NVMs and EAW operations.Like ARIES,MARS plays the role of the logging component of a database storage manager such as Shore[5,20].MARS differs from ARIES in three key ways.First, MARS relies on the storage device,via EAW operations, to apply the redo log at commit time.Second,MARS elim-inates the undo log that ARIES uses to implement its page stealing mechanism but retains the benefits of stealing by re-lying on the editable nature of EAWs.Third,MARS aban-dons the notion of transactional pages and instead operates directly on objects while relying on the hardware to guaran-tee ordering.MARS uses LogWrite operations for transactional up-dates to objects(e.g.,rows of a table)in the database.This provides several advantages.Since LogWrite does not update the data in-place,the changes are not visible to other transactions until commit.This makes it easy for the database to implement isolation.MARS also uses Commit to efficiently apply the log.This change means that MARS“forces”updates to stor-age on commit,unlike the no-force policy traditionally used by mit executes entirely within the SSD,so it can utilize the full internal memory bandwidth of the SSD (32GB/s in our prototype)to apply the commits and avoid consuming IO interconnect bandwidth and CPU resources. When a large transaction cannotfit in memory,ARIES can safely page out uncommitted data to the database tables because it maintains an undo log.MARS has no undo log but must still be able to page out uncommitted state.In-stead of writing uncommitted data to disk at its target loca-tion,MARS writes the uncommitted data directly to the redo log entry corresponding to the LogWrite for that location. When the system issues a Commit for the transaction,the SSD will write the updated data into place.By making the redo log editable,the database can use the log to hold uncommitted state and update it as needed. In MARS,this is critical in supporting robust and complex transactions.Transactions may need to update the same data multiple times and they should see their own updates prior to。