The Strange Behavior of Critical Branched Polymers
d开头的表示识别、发现的英语单词
d开头的表示识别、发现的英语单词Detecting patterns in nature is always fascinating. Did you know that even the tiniest details can lead to groundbreaking discoveries?Discovery is often a matter of curiosity and persistence. Digging deeper into a subject, you might stumble upon something unexpected but incredibly valuable.Did you detect that strange noise coming from the attic? It could be a sign of something bigger, or maybe just a harmless creak. But the act of noticing is half the battle.When we delve into history, we discover hidden treasures. Documents that have lain forgotten for centuries can reveal fascinating insights into the past.Diving into a new hobby can be an exciting journey of self-discovery. You never know what skills or interests you might uncover along the way.Detecting trends in the market is crucial for businesses to stay ahead of the competition. Staying vigilant and informed can mean the difference between success and failure.Decoding the language of nature is a lifelong pursuit for many scientists. The more we understand, the more we realize how interconnected everything is.Designing an experiment to test a hypothesis is all about identifying the right variables and controls. It's the detective work that leads to scientific breakthroughs.Dreaming big often leads to unexpected discoveries. Sometimes, all it takes is a wild imagination to see things in a new way.Determining the authenticity of an artifact can be a daunting task, but for archaeologists, it's all part of the thrill of the chase. Each clue brings them closer to the truth.。
九年级英语小说情节理解高级单选题40题
九年级英语小说情节理解高级单选题40题1. In "Jane Eyre", when Jane first meets Mr. Rochester, where does it happen?A. In the gardenB. In the drawing - roomC. On the roadD. In the church答案:C。
在《简·爱》中,简第一次遇见罗切斯特先生是在她外出送信的路上。
这一情节是简和罗切斯特先生故事的开端,为后续两人的感情发展奠定了基础,体现了命运的偶然交织,也暗示了简独立自由的性格,她可以独自外出完成工作,而这种在路上的邂逅也为他们之后冲破阶级等障碍的爱情埋下伏笔。
2. In "Wuthering Heights", Heathcliff is often described as having a certain look in his eyes. What is it?A. A look of pure hatredB. A look of deep sorrowC. A look of wild passionD. A look of cold indifference答案:C。
在 呼啸山庄》中,希斯克利夫的人物形象特点是充满强烈的情感。
他对凯瑟琳的爱是热烈且疯狂的,这种疯狂的爱与恨贯穿他的一生。
他眼睛里常常表现出一种狂热的激情,这种激情推动着他在小说中的种种行为,如复仇等,这一描写与小说所表达的那种激烈的爱恨情仇的主旨相呼应。
3. In "Jane Eyre", why does Jane leave Thornfield Hall suddenly?A. She discovers Mr. Rochester is already marriedB. She gets a better job offer elsewhereC. She misses her old friends too muchD. She is frightened by a strange noise in the hall答案:A。
The
ห้องสมุดไป่ตู้
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The role of unsteadiness in direct initiation of gaseous detonations
By C H R I S A. E C K E T T, J A M E S J. Q U I R K† A N D J O S E P H E. S H E P H E R D‡
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C. A. Eckett, J. J. Quirk and J. E. Shepherd
detonation transition (DDT). The main variable believed to control the success or failure of direct initiation is the magnitude of the initial energy release, provided the energy deposition is sufficiently fast and the igniter sufficiently small. Experiments suggest that for a given combustible gas mixture at given uniform premixed initial conditions, the energy release must be above a certain level, known as the critical energy, to successfully initiate a detonation. The same arguments apply for direct initia
Breakdown of the Fermi liquid theory in heavy fermion compounds
a r X i v :c o n d -m a t /0211284v 1 [c o n d -m a t .s t r -e l ] 14 N o v 2002Breakdown of the Fermi liquid theory in heavy fermion compoundsC.P´e pin a ,1and P.Coleman b ,aSPhT,CEA-Saclay,l’Orme des Merisiers,91191Gif-sur-Yvette,France.bSerin Laboratory,Rutgers University,P.O.Box 849,Piscataway,NJ 08855-0849,USA.1.Experimental overview and theoretical insights 1.1.experimentsFermi liquid theory [1],developed by Landau in the mid 1950’s,provides the foundation for much of our current understanding of electron fluids.Accord-ing to the Landau Fermi Liquid theory (LFL),thermo-dynamic and transport properties of a metal at very low temperatures are described in terms of weakly in-teracting fermions,or “Landau quasiparticles”.Lan-dau quasiparticles consist of electrons,surrounded by a cloud of spin and charge polarization.They share the same quantum numbers as free electrons but their masses can be strongly renormalized by the back flow of the surrounding fluid.A striking example of the ro-bustness of the LFL is provided by heavy fermion be-havior,where the effective mass of the quasiparticles can be hundreds of times greater than that of a bare electron.The physical properties of this fluid follow cer-tain characteristic power-law dependences on temper-T=γ0log[T 0m∗(T).On the hot lines,the electrons are strongly perturbed by the magneticfluctuations and their life time is strongly suppressed.More precisely in three dimensions the imaginary partof the self-energy varies likeΣH∼ω.Their effectivemass experiences a logarithmical increase with temper-ature.Away from the hot lines however,the scatteringof the electrons offthe critical modes is strongly sup-pressed-the magneticfluctuations getting massive.Within the3D SDW scenario,the hot lines are notwide enough to destabilize the FL theory.In this situ-ation,the critical contributions to the free energy andthe specific heat coefficient are given by√F∼T5/2and C/T=γ0−this scenario,the2D SDW[16,17],the dimension of the spinfluid(2D)is lower than the one of the con-duction electrons(3D).Within this assumption afi-nite region of the Fermi surface is hot,as shown in figure1,right.This intuitively corresponds to an“in-finite”width of the hot lines.This situation-a fully anisotropic magnet-,while difficult to realize experi-mentally,is strong enough to destabilize the FL the-ory,accounting for the logarithmic divergence of the specific heat coefficient with temperature as well as the linear in T resistivity.Two important remarks are due here.First,this scenario is remarkably sensitive to magnetic anisotropy.If the2D spinfluid retains a small inter-plane coupling,then Fermi liquid behavior will recover at temperature scales smaller than the in-terlayer coupling.The second comment relates to the upper critical dimension.Close to an antiferromagnetic instability at zero temperature,the system experiences strongfluctuations in time which scale with respect to the length likeτ∼ξz.z is the dynamical exponent of the QCP,and is equal to2for the antiferromagnet. The effective dimension of the system is now D=d+z, where d is the number of spacial dimensions for the spinfluid.In the2D SDW scenario,D=2+2=4so the effective lagrangian lies at its upper critical dimen-sion,implying marginal coupling constants.This fea-ture wouldn’t be enough to account for the anomalous exponents observed in the magnetic susceptibility. 2.A study of YbRh2Si2:the breakdown of the 2D SDW scenarioIn the next section,we would like to discuss new insights into the the mechanism by which the heavy quasiparticle may disintegrate at the QCP,revealed by recent studies of the compound YbRh2(Si1−x Ge x)2 [18,19].The undoped(x=0)compound lies remark-ably close to a QCP,with a tiny antiferromagnetic or-dering temperature T N=70mK[11]that can be sup-pressed to zero by a small magneticfield of just B c= 0.06T perpendicular to the easy axis.By allowing tiny amount of Germanium into the crystal,it is possible tofine-tune the N´e el temperature T N and the critical field B c to zero,without appreciably increasing the dis-order in the material.The materials can then be con-trollably driven back into the FL state by application of a small magneticfield.2.1.The upturn in the specific heatSeveral unusual features are revealed at criticality. In addition to the previously observed logarithmic in-crease when lowering the temperature,the specific heat coefficientγshows a strong upturn below30mK(figure 2).The electronic nature the upturn has been checked first by carefully removing the nuclear contribution, second by the observation that under a small magnetic field,the electronic contribution in the FL phase grad-ually saturates the upturns,as one gets closer to the QCP.Such an upturn of electronic nature reveals aC el/T(Jmol-1K-2)T (K)Fig. 2.Strong upturn in the specific heat coefficient of YbRh2(Si1−x Ge x)2for x=0.05[19].One observes how the upturnfills in as one reaches the QCP by decreasing the ap-plied magneticfield.strong departure from any SDW scenario,where the maximum possible increase of the specific heat coeffi-cient is logarithmic.More specifically,the behavior of γcan be cast into the formγ(T,B)=B−αΦ(Tis the residual resistivity),below a characteristic tem-perature T ∗F .The temperature at which the T 2behav-ior,characteristic of the Landau FL theory appears,sets the crossover between the heavy fermion regime and the quantum critical regime.Inside the FL phase,even though the quantum fluctuations are not strong enough to destabilize the FL,the electron undergoes virtual scattering offthe critical magnetic modes.The variation of A (B )close to the QCP provides insight into these virtual excitations.Initial measurements on germinium doped Y bRh 2Si 2−x Ge x show that A (B )∼1/(B −B c )in the approach to the QCP.Over a wide range of field,the Kadowaki Woods ratio is found to be approximately constant,with a value K =A/(γ0)2≈5.8µΩcmK 2mol 2/J(9)is found to agree within 40%with the empirical Kad-owaki Woods ratio.More recent measurements closer to the QCP show a slow upturn in K at very small val-ues of B −B c .[19]Constancy of the Kadowaki woods ratio implies that the transport scattering rate scalesstrictly with the square of the renomalized T ∗F (B )of the heavy electron fluid.A truly field independent Kad-owaki Woods ratio would indicate that the momentum dependence of the scattering amplitude does not renor-malize with T ∗F(B ).2.3.The 2D SDW scenario is ruled outThis set of data allows us to rule out the 2D SDWscenario.While the 2d SDW scenario leads to the re-sult A ∝1/(B −B c )as observed experimentally,the soft 2D spin fluctuations produce only a small renor-malization in the heavy electron density of states with γ∝ln 1/(B −B c ).This would give a strongly diver-gent Kadowaki Woods ratio in the approach to the QCP:K SDW ∝1/ (B −B c )ln 2(B −B c ) .The weak field dependence of the Kadowaki Woods ratio suggests that the most singular quasiparticle scattering ampli-tudes have a far weaker momentum dependence than expected in a spin density wave scenario.3.The breakup of the heavy electron-is therea preformed Kondo effect at the QCP?The study of YbRh 2(Si 2−x Ge x )reveals a very un-usual property.While the specific heat coefficient ex-periences a strong upturn below T =30mK ,there is no reflection of this sudden loss of entropy in the trans-port properties:the resistivity stays linear in T for the whole temperature regime.This suggests that the degrees of freedom associated with the upturn in thespecific heat are not involved in the charge transport.What is the origin of this separation?One of the challenges here is to understand the clear separation between the single ion Kondo temper-ature T K ,which clearly remains finite at the QCP,andthe renormalized T ∗F (B )which is driven continuously to zero.Burdin et al.[20]have suggested the analogy with pre-formed pairs in a superconductor,according to which T K is the temperature at which pre-formedlocal Kondo singlets develop and T ∗F is the scale at which phase coherence sets in to form mobile quasi-particles.By analogy one can consider the QCP in heavy fermions as a king of preformed scenario for the Kondo effect.In such a picture,the presence of very strong antiferromagnetic fluctuations close to a QCP dephases the heavy fermion composite quasi-particles at increasingly low temperatures,as one gets closer to the QCP.Eventually at the QCP the coherence tem-perature is driven to zero,leading to the disintegration of the heavy composite electron.We would like to thank N.Andrei,J.Custers,P.Gegenwart and F.Steglich,for for discussions related to this work.This research is supported in part by the National Science Foundation grant nsf-dmr 9983156(PC).References[1]ndau,Sov.Phys.JETP 3(1957)920.[2]H.von L¨o hneysen,J.Phys.Cond.Mat.8(1996)9689.[3]A.Sidorov et al.,Phys.Rev.Lett.89(2002)157004;[4]N.D.Mathur et al.,Nature ,394,39(1998).[5]M.Grosche et al.,J.Phys.Cond.Mat.12(2000)533.[6]P.Gegenwart et al.,Phys.Rev.Lett.82(1999)1293.[7]F.Steglich et al.,Z.Phys.B 103(1997)235.[8]Y.Aoki et al.,J.Phys.Soc.Japan 66(1997)2993.[9]A.Schroeder et al.,Nature 407(2000)351.[10]S.R.Julian et al.,J.Phys.Cond.Mat.8(1996)9675.[11]O.Trovarelli et al.,Phys.Rev.Lett.85(2000)626.[12]Q.Si et al.,Nature 413,(2001)804.[13]P.Coleman et al.,J.Phys.Cond.Mat.13(2001)R723.[14]J.Hertz,Phys.Rev.B 14(1976)1165.[15]lis,Phys.Rev.B 48(1993)7183.[16]A.Rosch,Phys.Rev.Lett.79(1997)159.[17]I.Paul and G.Kotliar Phys.Rev.B 64(2001)184414.[18]P.Gegenwart et al.,Phys.Rev.Lett.89(2002)56402.[19]J.Custers et al.,to be published (2003).[20]S.Burdin et al.,Phys.Rev.Lett.85(2000)1048.4。
String Theory in Two Dimensions
2024上海静安区高三英语二模
静安区2023学年第二学期期中教学质量调研高三英语试卷(完卷时间:120分钟满分:140分)2024年4月考生注意:1. 试卷满分140分,完卷时间120分钟。
2. 本调研设试卷和答题纸两部分,全卷共12页。
所有答题必须涂(选择题)或写(非选择题)在答题纸上,做在试卷上一律不得分。
第I 卷(共100分)I. Listening ComprehensionSection ADirections: In Section A, you will hear ten short conversations between two speakers. At the end of each conversation,a question will be asked about what was said. The conversations and the questions will be spoken only once. After you hear a conversation and the question about it,read the four possible answers on your paper,and decide which one is the best answer to the question you have heard.1. A. At a grocery store. B. At a florist's stand.C. At a bank counter.D. At an electronic shop.2. A. Sign up for a fitness class. B. Shop for fitness equipment.C. Have a fitness test.D. Watch a fitness video.3. A. Pay the ticket right away. B. Challenge the ticket.C. Ignore the ticket.D. Apologize to the parking officer.4. A. She is available on Saturday. B. She will cancel her dentist appointment.C. She can not cover the man's shift.D. She forgot about the shift.5. A. The woman had better give him an extension on the deadline.B. The woman had better draft the proposal by herself.C. The woman had better approve the proposal.D. The woman had better give insights on the budget section.6. A. She doesn't like animals from the shelter.B. She prefers buying pets from breeders.C. She thinks adopting a pet is a bad idea.D. She supports the idea of adopting a pet.7. A. Either of them is an experienced chef.B. Both of them have experienced failures in the kitchen.C. Neither of them are fond of cooking.D. Both of them are concerned about the new recipe.8. A. Bungee jumping is safeB. Bungee jumping is thrilling.C. Bungee jumping might have risks.D. Bungee jumping is sure to be regrettable.9. A. The man should borrow the book several days later.B. The woman urgently needs the book back.C. The man does not need to return the book quickly.D. The woman is unwilling to lend the man the book.10. A. The woman's parents will not appreciate a surprise party.B. The woman should prioritize her parents' preferences for the party.C The man dislikes the idea of a surprise party.D. The woman should plan a party based on her own preferences.Section BDirections: In Section B,you will hear two short passages and one longer conversation. After each passage or conversation,you will be asked several questions. The passages and the conversation will be read twice,but the questions will be spoken only once. When you hear a question,read the four possible answers on your paper and decide which one would be the best answer to the question you have heard.Questions 11 through I3 are based on the following speech.11. A. A pupil in need of help. B. A person promising to donate money.C. A member from a charity.D. A teacher in the Semira Region.12. A. 10%. B. 35%. C. 50%. D. 65%.13. A. To train teachers for the disabled. B. To help a pupil with special needs.C. To pay for a walking holiday.D. To organize a charity club for the disabled.Questions 14 through 16 are based on the following passage.14. A. To distract other students from doing well.B. To impress his friends with the shining ring.C. To improve his chances in the exam.D. To honor his grandfather by wearing a ring.15. A. By having enough time for breaks.B. By breaking down learning into portions.C. By informing teachers of the study habits.D. By wearing lucky objects.16. A. Start revision ahead of time.B. Reward oneself during revision.C. Consider different learning styles.D. Stay up late for the exam.Questions 17 through 20 are based on the following conversation.17. A. To inquire about travel recommendations.B. To discuss cultural festivals in Southeast Asia.C. To plan a solo travel adventure to Thailand.D To learn about Mr. Patel's travel experiences.18. A. Europe and Africa. B. Thailand and VietnamC. South America and Australia.D. Japan and China.19. A. Solely cultural exploration.B. Primarily outdoor adventures.C. A mix of cultural and outdoor experiences.D. Luxurious and private accommodations.20. A. It is ideal for meeting fellow travelers.B. It offers exclusive travel experiences.C. It is a more comfortable and secure stay.D. It offers authentic cultural immersion.II. Grammar and VocabularySection ADirections:After reading the passage below,fill in the blanks to make the passages coherent and grammatically correct.For the blanks with a given word,fill in each blank with the proper form of the given word;for the other blanks,use one word that best fits each blank.Beethov-hen's first symphonyOn a grey Friday morning at a Hawke's Bay farm,members of New Zealand's symphony orchestra dressed in black to perform their latest composition in front of a large crowd.The music contained many marks of traditional classical music,but as it began,the instruments started to make loud,rough sounds more commonly __21__(hear)in chicken coops than in an auditorium.However,no feathers were angered by this departure from tradition, ___22__the audience that gathered to listen to the concert last week was,in fact,a couple of thousand chickens.The piece of music-Chook Symphony No. 1-__23__(create)specifically for the birds out of an unlikely partnership between the orchestra and an organic free-range chicken farm which wanted a piece of chicken-friendly music to enrich its flocks' lives.“We've been playing classical music for the chickens for some years now because ___24 ___ is well researched that the music can calm the chickens down,”says Ben Bostock,one of the two brothers who__25(own)the Bostock Brothers farm. Research has shown animals can respond positively to classical music,and chickens are particularly responsive to baroque(巴洛克格),according to some studies.The composer,Hamish Oliver,__26__used the baroque tradition as a starting point and drew inspiration from composers such as Corelli,Bach,and Schnitke,wanted the piece to be playful by including sounds from a chicken's world. “The trumpet imitates the c hicken …the woodwind instruments are the cluckiest,especially if you take the reeds off. ”The early stages of composition were spent _______(test)out which instruments and sounds the chickens responded to best.“They didn't like any big banging. ”Bostock said,adding that when the birds respond positively to themusic,they tend__28__(wander)farther among the trees. Bostock now hopes chicken farmers around the world will use the piece of music to calm their own birds.For Oliver,having input from the farmers about __ 29__the chickens were responding to particular sounds and instruments was a highlight of the project.The symphony has searched exhaustively __30__any other examples of orchestras making music specifically for chickens and believes this to be a world-first,says Peter Biggs,the orchestra's chief executive.Section BDirections :Complete the following passage by using the words in the box. Each word can only be used once. Note thatA new way to reduce poachingResearchers are working on a pilot program backed by Russia's Rosatom Corp to inject rhino horns(犀牛角)with radioactive material,a strategy that could discourage consumption and make it easier to detect illegal trade.Poachers(偷猎者)killed 394 rhinos in South Africa for their horns last year,government data shows,with public and private game __31__lacking the resources needed to monitor vast tracts of land and protect the animals that live there.While the toll was a third lower than in 2019 and the sixth __32_drop,illegal hunting remains the biggest threat to about 20,000 of the animals in the country —the world's biggest population.Thousands of__33__sensors along international borders could be used to detect a small quantity of radioactive material____34___into the horns,according to James Larkin,a professor at the University of Witswatersrand in Johannesburg,who has a background in radiation protection and nuclear security. “A whole new_35_of people could be able to detect the illegal movement of rhino horn,"he said. Some alternate methods of discouraging poaching,including poisoning, dyeing and removing the horns,have raised a variety of opinions as to their virtue and efficacy.Known as The Rhisotope Project,the new anti-poaching __36__started earlier this month with the injection of an amino acid(氨基酸)into two rhinos' horns in order to detect whether the compound will move into the animals' bodies. Also,__37__studies using computer modeling and a replica rhino head will be done to determine a safe dose of radioactive material. Rhino horn is used in traditional medicine,as it is believed to cure disease such as cancer,__38__as a show of wealth and given as gifts."If we make it radioactive, these people will be hesitant to buy it,"Larkin said. "We're pushing on the whole supply chain. "Besides Russia's state-owned nuclear company,the University of Witwatcrsrand. scientists and private rhino owners are involved in the project. If the method is ___39__feasible,it could also be used to curb illegal trade in elephant ivory.“Once we have developed the whole project and got to the poi nt where we completed the proof of concept,then we will be making this whole idea ____40_to whoever wants to use it. " Larkin said.III. Reading ComprehensionSection ADirections: For each blank in the following passages there are four words or phrases marked A, B. C and D. Fill in each blank with the word or phrase that best fits the context.City air is in a sorry state. It is dirty and hot. Outdoor pollution kills 4. 2m people a year, according to the World Health Organization. Concrete and tarmac meanwhile,absorb the sun's rays rather than reflecting them back into space,and also ___41 ___plants which would otherwise cool things down by evaporative transpiration(蒸腾作用). The never-ceasing__42_of buildings and roads thus tums urban areas into heat islands,discomforting residents and worsening dangerous heatwaves.A possible answer to the twin problems of pollution and heat is trees. Their leaves may destroy at least some chemical pollutants and they certainly __43__tiny particles floating in the air. which are then washed to the ground by rain. Besides transpiration,they provide __44___.To cool an area effectively, trees must be planted in quantity. Two years ago, researchers at the University of Wisconsin found that American cities need 40%tree___45___to cut urban heat back meaningfully. Unfortunately,not all cities —and especially not those now springing up in the world's poor and middle-income countries —are __46___with parks, private gardens or a sufficient number of street trees. And the problem is likely to get worse. At the moment,55%of people live in cities. By 2050 that share is expected to reach 68%.One group of botanists believe they have at least a partial ___47___to this lack of urban vegetation. It is to plant miniature simulacra(模拟物)of natural forests, ecologically engineered for rapid growth. Over the course of a career that began in the 1950s,their leader,Miyawaki Akira, a plant ecologist at Yokohama National University in Japan. has developed a way to do this starting with even the most___ 48___deserted areas. And the Miyawaki method is finding increasing___ 49___around the world.Dr Miyawaki's insight was to deconstruct and rebuild the process of ecological succession, by which ___50___land develops naturally into mature forest. Usually,the first arrival is grass, followed by small trees and,finally. larger ones.The Miyawaki method___51 ___some of the early phases and jumps directly to planting the kinds of species found in a mature wood.Dr Miyawaki has__52__the planting of more than 1,500 of these miniature forests,first in Japan,then in other parts of the world. Wherever they are planting,though,gardeners are not restricted to__53 __nature's recipe book to the letter. Miyawaki forests can be customized to local requirements. A popular choice__54__ is to include more fruit trees than a natural forest might support,thus creating an orchard that requires no maintenance.If your goal is to better your __55__surroundings,rather than to save the planet from global warming,then Dr Miyawaki might well be your man.41. A. thrive B. nourish C. displace D. raise42. A. assessment B. maintenance C. spread D. replacement43. A. release B. trap C. reflect D. dissolve44. A. attraction B. shadow C. interaction D. shade45. A. consumption B. coverage C. interval D. conservation46. A. blessed B. lined C. piled D. fascinated47. A. treatment B. obstacle C,warning D. solution48. A. unnoticed B. unpromising C. untested D. unfading49. A. criticism B. favor C. sponsor D. anxiety50. A. bare B. graceful C. faint D. mysterious51. A highlights B. skips C. improves D. pushes52. A. accessed B. spotted C. supervised D. ranked53. A. disturbing B. balancing C. following D. reducing54. A. for example B. in essence C. on the other hand D. after all55. A. suburban B. leisure C. scenic D. immediateSection BDirections: Read the following three passages. Each passage is followed by several questions or unfinished statements. For each of them there are four choices marked A,B,C and D. Choose the one that fits best according to the information given in the passage you have read.(A)From Marie Tussaud's Chamber of Horrors to Disneyland's Haunted Mansion(鬼屋)to horror-themed escape rooms,haunted house attractions have terrified and delighted audiences around the world for more than 200 years.These attractions turn out to be good places to study fear. They help scientists understand the body's response to fright and how we perceive some situations as enjoyably thrilling and others as truly terrible. One surprising finding;having friends close at hand in a haunted house might make you more jumpy,not less so.Psychologist and study co-author Sarah Tashjian,who is now at the University of Melbourne, and her team conducted their research with 156 adults,who each wore a wireless wrist sensor during their visit. The sensor measured skin responses linked to the body's reactions to stress and other situations. When the sensor picked up,for example,greater skin conductance —that is,the degree to which the skin can transmit an electric current —that was a sign that the body was more aroused and ready for fight or flight. In addition to this measure,people reported their expected fear (on a scale of 1 to 10)before entering the haunted house and their experienced fear (on the same scale)after completing the haunt.The scientists found that people who reported greater fear also showed heightened skin responses. Being with friends,Tashjian and her colleagues further found,increased physiological arousal during the experience,which was linked to stronger feelings of fright. In fact,the fear response was actually weaker when people went through the house in the presence of strangers.Other investigators have used haunted houses to understand how fear and enjoyment can coexist. In a 2020 study led by Marc Malmdorf Andersen,a member of the Recreational Fear Lab at Aarhus University in Denmark,scientists joined forces with Dystopia Haunted House. The Danish atraction includes such terrifying experiences as being chased by "Mr. Piggy",a large, chain-saw-wielding man wearing a bloody butcher's apron and pig mask. People between the ages of 12 and 57 were video recorded at peak moments during the attraction,wore heart-rate monitors throughout and reported on their experience. People's fright was tied to large-scale heart-rate fluctuations;their enjoyment was linked to small-scale ones. The results suggest that fear and enjoyment can happen together when physiological arousal is balanced "just right".56. Studing haunted house attractions helps scientists to learn about _____.A. the psychological effects of fear on individualsB. the history of horror-themed entertainmentC. the body's response to material rewardsD. the impact of technology on people's enjoyment57. How did Sarah Tashjian and her team conduct their research on haunted house experiences? A. By surveying participants.B. By analyzing historical records.C. By employing wireless wrist sensors.D. By using virtual reality simulations.58. What did Tashjian and her colleagues discover in their study?A. Being with fiends elevated level of physiological arousal.B. The fear reaction was stronger in the company of strangers.C. Psychological effect was unrelated to intensified feelings of fright.D. Those reporting lightened fear showed increased skin responses.59,It can be concluded from the 2020 study led by Marc Malmdorf Andersen that ____.A. fear and enjoyment can not happen at the same timeB. large-scale heart-rate fluctuations were linked to enjoymentC. the age of the participants was not related to the study's findingsD. fear and enjoyment can coexist under certain conditions(B)Is an electric vehicle right for you?Many people will ask themselvesthat question for the first time this year.Prices are falling,battery range is risingand mainstream brands are adding new EVs at a breakneck pace.Here are three things anybody seriously considering buying an EV should know:1. The price to install a 240v chargerAnybody who owns an electric vehicle needs a 240-volt charger at home. With one,you can recharge overnight,so you start every day with the equivalent of a full tank.Just a few years ago,home 240v EV chargers cost $2,500-$3,000,including installation,but prices have declined as competition grows with the number of EVs on the road.2. The time it takes to chargeAbout 80%of miles driven in EVs are powered by electricity charged at home,but you'll need to charge elsewhere occasionally. That's when charging time becomes a big deal,but how long it takes depends on a couple of factors.First,voltage from the charger. Getting 250 miles of range in seven hours from a 240v charger is fine when you're charging overnight at home,but it's a deal breaker if you're going 300 miles for a weekend getaway. In that case,you'll want to look for a 400v DC fast charger. They're not as common as 240v public chargers yet,but they're becoming more widespread.There's another factor:the on-board charger. It regulates how fast the battery can accept electricity. A vehicle with a higher-capacity on-board charger accepts electricity faster.3. Where to chargeGood route-planning apps will help you find chargers on a road trip.“Most people have no idea how many public charging stations are within,say,a 10-or 15- mile radius(半径)because they're small,people don't look for them or even don't know what to look for,and they're rarely signposted,"said journalist John Voelcker,who has studied EVs and charging exhaustively.4. On the horizonIf an EV doesn't meet your needs now, watch this space. They're coming closer,but large numbers of gasoline vehicles will remain in production for years. Beyond that,companies will keep making spare parts for oil-burners for decades.60. Which of the following statements is TRUE according to the passage?A. The price of installing a home EV charger has remained stable in the past few years.B. It's quite easy to identify the public charging stations with the help of striking signposts.C. Popular brands are introducing new EVs at an incredibly fast rate.D. An electric vehicle can't provide the same amount of energy as a completely filled fuel tank.61. The underlined phrase "watch this space" in the last paragraph probably means" _______ ”.A. give up the plan to purchase an EVB. make space for an EVC. find an alternative to EVD. keep an eye out for future developments62. This passage is mainly intended to _______ .A illustrate the factors charging time depends onB. offer advice on purchasing an electric vehicleC. look forward to the future of electric vehiclesL explain the reason for the falling prices of electric vehicles(C)Flinging brightly coloured objects around a screen at high speed is not what computers' central processing units were designed for. So manufacturers of arcade machines invented the graphics-processing unit (GPU),a set of circuits to handle video games' visuals in parallel to the work done by the central processor. The GPU's ability to speed up complex tasks has since found wider uses:video editing, cryptocurency mining and most recently,the training of artificial intelligence.AI is now disrupting the industry that helped bring it into being. Every part of entertainment stands to be affected by generative AI,which digests inputs of text,image,audio or video to create new outputs of the same. But the games business will change the most,argues Andreessen Horowitz,a venture-capital(VC)firm. Games interactivity requires them to be stuffed with laboriously designed content:consider the 30 square miles of landscape or 60 hours of music in “Red Dead Redemption 2”a recent cowboy adventure. Enlisting Al assistants to chum it out could drastically shrink timescales and budgets.AI represents an "explosion of opportunity"and could drastically change the landscape of game development. Making a game is already easier than it was:nearly 13,000 titles were published last year on Steam,a games platform,almostdouble the number in 2017. Gaming may soon resemble the music and video industries in which most new content on Spotify or YouTube is user-generated. One games executive predicts that small firms will be the quickest to work out what new genres are made possible by Al. Last month Raja Koduri,an executive at Intel,left the chip maker to found an Al-gaming startup.Don't count the big studios out,though. If they can release half a dozen high-quality titles a year instead of a couple,it might chip away at the hit-driven nature of their business,says Josh Chapman of Konvoy,a gaming focused VC firm. A world of more choices also favors those with big marketing budgets. And the giants may have better answers to the mounting copyright questions around Al. If generative models have to be trained on data to which the developer has the rights,those with big back-catalogues will be better placed than startups. Trent Kaniuga,an artist who has worked on games like "Fortnite",said last month that several clients had updated their contracts to ban Al-generated ant.If the lawyers don't intervene,unions might. Studios diplomatically refer to Al assistants as “co-pilots”,not replacements for humans.63. The original purpose behind the invention of the graphics-processing unit (GPU)was to______A. speedup complex tasks in video editing and cryptocurency miningB. assist in the developing and training of artificial intelligenceC. disrupt the industry and create new outputs using generative AID. offload game visual tasks from the central processor64. How might the rise of AI-gaming startups affect the development of the gaming industry?A. It contributes to the growth of user-generated content.B. It facilitates blockbuster dependency on big studios.C. It decreases collaboration between different stakeholders in the industry.D. It may help to consolidate the gaming market under major corporations.65. What can be inferred about the role of artificial intelligence in gaming?A. AI favors the businesses with small marketing budgets.B. AI is expected to simplify game development processes.C. AI allows startups to gain an edge over big firms with authorized data.D. AI assistants may serve as human substitutes for studios.66. What is this passage mainly about?A. The evolution of graphics-processing units (GPUs).B. The impact of generative AI on the gaming industry.C. The societal significance of graphics-processing units(GPUs).D. The challenges generative AI presents to gaming studios.Section CDirections: Read the following passage. Fill in each blank with a proper sentence given in the box. Each sentence can beTime to end Santa's 'naughty list'?Many of us have magical memories of Santa secretly bringing gifts and joy to our childhood homes —but is there a darker side to the beloved Christmas tradition?I was —and I'm happy to admit it —a loyal believer of Santa. I absolutely loved the magic of Christmas,especially Santa Claus,and my parents went above and beyond to encourage it. However,as I begin to construct my own Santa Claus myth for my daughter,I can't help but feel guilty. Could it undermine her trust in me?_____67______Backin1978,a study published in the American Journal of Orthopsychiatry(矫正精神医学)found that 85%of four-year-olds said they believed in Santa. In 2011,research published in the Journal of Cognition and Development found that 83%of 5-year-olds claimed to be true believers.I guess it's not all that surprising. _____68 _____He features in every Christmas TV show and movie. Each year the North American Aerospace Defence Command (NORAD)allows you to track Santa's journey on Christmas Eve. To reassure children during the pandemic in 2020,the World Health Organization issued a statement declaring that Santa was “immune”from Covid 19. And it's precisely this effort on behalf of parents,and society in general,to create such seemingly overwhelming evidence for the existence of Santa Claus that David Kyle Johnson,a professor of philosophy at King's College in Pennsylvania,describes as 'The Santa Lie' in his book The Myths That Stole Christmas. He highlights how we don't simply ask children to imagine Santa,but rather to actually believe in him. _____69 _____The 'Santa lie' can reduce trust between a parent and a child. _____70 _____It is the creation of false evidence and convincing kids that bad evidence is in fact good evidence that discourages the kind of critical thinking we should be encouraging in children in this era. “The ‘Santa lie' is part of a parenting practice that encourages people to believe what they want to believe,simply because of the psychological reward,”says Johnson. “That's really bad for society in general. ”IV. Summary WritingDirections: Read the following passage. Summarize the main idea and the main point(s)of the passage in no more than 60 words. Use your own words as far as possible.Exploring the Appeal of VintageToday,the term“vintage”applies to almost everything. Vintage is more recent than an antique (古董)which is defined as 100 years old or more. It basically means reviving something old- fashioned or filled with memories. For an object to be considered vintage,it must be unique and genuine enough to retain at least some of its original charm.We buy vintage because it creates a sense of personal connection for us:it speaks to our childhood memories and that feels good. We also buy vintage because we're rebels. Vintage is a protest against modern mainstream culture. In an age of technology,buying vintage is a refuge from our fast-paced,high-tech world. We want our children to make the most of their creativity and know how to entertain themselves without electronic gadgets. Ironically,early video games are now considered vintage.Of all the vintage objects,vintage toys are forever attractive for both adults and children. Although some toys have emotional value,others have high market value and are expensive to collect. Vintage toys that were made in small quantities often bring a higher value than those that were mass produced. That means,if you own one of the 2,000 “Peanuts”royal blue beanie baby elephants that were manufactured with a darker blue coat than originally intended,you might have something valuable on your hands. In fact,due to a manufacturer error,this is the most collectible beanie baby around —and worth about f3,000.If you're motivated and feeling lucky,you can find deals on vintage toys by browsing charity shops,secondhand stores,community centers,flea markets and garage sales. You never know what kind of treasures are hiding at the bottom of a mixed box in someone's basement,garage or attic.第Ⅱ卷(共40分)V. TranslationDirections: Translate the following sentences into English. using the words given in the brackets.72. 他在升旗仪式上的演讲得到了高声喝彩。
Iliadis Modeling
1 Exactfinite-size scaling with corrections in the two-dimensional Isingmodel with special boundary conditionsW.Janke a and R.Kenna ba Institut f¨u r Theoretische Physik,Universit¨a t Leipzig,Augustusplatz10/11,04109Leipzig,Germanyb School of Mathematics,Trinity College Dublin,IrelandThe two-dimensional Ising model with Brascamp-Kunz boundary conditions has a partition function more amenable to analysis than its counterpart on a torus.This fact is exploited to exactly determine the fullfinite-size scaling behaviour of the Fisher zeroes of the model.Moreover,exact results are also determined for the scaling of the specific heat at criticality,for the specific-heat peak and for the pseudocritical points.All corrections to scaling are found to be analytic and the shift exponentλdoes not coincide with the inverse of the correlation length exponent1/ν.1.INTRODUCTIONFinite-size scaling(FSS)is a well established technique for the extraction of critical exponents fromfinite volume analyses[1].Such exponents characterise critical phenomena at a second-order phase transition.The simplest model exhibiting such a transition is the Ising model in two dimen-sions,which,despite a long history and extensive study,still offers new results and insights.Here, we study the model under the special boundary conditions of Brascamp and Kunz[2]to extract new information and to help resolve some hith-erto puzzling features of FSS.Let C L(β)be the specific heat at inverse tem-peratureβfor a system of linear extent L.FSS of the specific heat is characterized by the location of its peak,βL,its height C L(βL)and its value at the infinite-volume critical point C L(βc).The peak position,βL,is a pseudocritical point which typically approachesβc as L→∞as|βL−βc|∼L−λ,(1) whereλis the shift exponent.In two dimensions, the Ising specific heat scales as ln L.Of further interest is the FSS of the complex Fisher zeroes of the partition function[3].The leading behaviour of the imaginary part of a Fisher zero is[4]Im z j(L)∼L−1/ν,(2)where z stands generically for an appropriate function of temperature,the subscript j labels the zeroes,andνis the correlation length critical exponent.The real part of the lowest zero may be viewed as another effective critical or pseudo-critical point,scaling as|Re z1(L)−z c|∼L−λzero,(3) where z=z c atβ=βually the shift expo-nents,λandλzero,coincide with1/ν,but this is not a consequence of FSS and is not always true. The following results have been obtained for FSS in the two-dimensional Ising model.Exact Analytical Results:For toroidal lat-tices the specific-heat FSS has been determined exactly to order L−3at the infinite-volume crit-ical point in[5–7].Only integer powers of L−1 occur,with no logarithmic modifications(except for the leading term),i.e.,C L(βc)=C00ln L+C0+∞k=1C k2Numerical Results:For spherical lattices the shift exponent of the specific heat was found to be significantly away from1/ν=1,withλranging from approximately1.75to2(with the possibility of logarithmic corrections)[8].Therefore the FSS of the specific-heat pseudocritical point does not appear to match the correlation length scaling. In another study[9],FSS of Fisher zeroes for square periodic lattices yielded a value ofνwhich appeared to approach the exact value(unity)as the thermodynamic limit is approached.Small lattices appeared to yield an effective correction-to-scaling exponentω≈1.8while closer to the thermodynamic limit,these corrections tended to be analytic withω=1.A certain formal limit of conformalfield theory suggests a correction ex-ponentω=4/3[10].However,the validity of this limit has long been unclear[11]and the ques-tion of the absence of a subleading operator corre-sponding toω=4/3in the standard Ising model in two dimensions was recently addressed in depth in[12](see also[13]).In the light of these analyses,we present ex-act results which help clarify the situation.To this end,we have selected the Ising model with Brascamp-Kunz boundary conditions[2].2.FISHER ZEROESThe Brascamp-Kunz lattice has M sites in the x direction and2N sites in the y direction.The boundary conditions are periodic in the y direc-tion and the2N spins along the left and right bor-ders arefixed to...+++...and...+−+−+−..., respectively.The partition function is[2]Z∝Ni=1M j=1 1+z2−z(cosθi+cosφj) ,(5)where z=sinh2β,θi=(2i−1)π/2N andφj= jπ/(M+1).One notes that the partition function (5)is given as a double product.Determination of the Fisher zeroes of(5)is thus straightforward, as is the calculation of thermodynamic functions. For toroidal boundary conditions,on the other hand,the partition function is a sum of four such products[14].There it is non-trivial to determine the zeroes or the thermodynamic functions.The zeroes of(5)are on the unit circle in the complex-z plane(so the critical point is z c=1) [2].These are z ij=exp(iαij),whereαij=cos−1 cosθi+cosφj4 1+122−M−2σ2(1+σ2)2π 1+1M k.(10) The coefficients c k can easily be determined ex-actly and those up to c3are explicitly given in[15].So for the critical specific heat on3 a Brascamp-Kunz lattice,apart from a trivialln M/M term(which could be removed by a re-definition of M[15]),the FSS is qualitatively thesame as(but quantitatively different to)that ofthe torus topology in(4).Specific Heat near the Critical Point:Thepseudocritical point of the specific heat,z pseudoM,2N ,can be determined as the point where the deriva-tive of C M,2N(z)vanishes.This gives[15]z pseudo M,2N =1+a2ln MM2+a3ln MM3+O (ln M)2π 1+1M+d 2(ln M)2M2 ,(12)with c 0=c0and c 1=c1.Higher order terms are of the form1/M2,(ln M)2/M3,ln M/M3and 1/M3.Notice that,up to O(1/M),(12)is quanti-tatively the same as the critical specific-heat scal-ing(10).The higher order terms of(12)differ qualitatively from those in(10)in that there are logarithmic modifications of the form(ln M)k/M l (with integer k and l).Again,the values of the coefficients are given in[15].4.CONCLUSIONSFor the two-dimensional Ising model with Brascamp-Kunz boundary conditions,we have derived exact expressions for the FSS of the Fisher zeroes to all orders.We have also deter-mined the FSS of the critical specific heat,its pseudocritical point and its peak.The advantage of Brascamp-Kunz boundary conditions(over pe-riodic ones)is that the partition function is a product and meliorates determination of higher order corrections.The following are the main features we have found:All corrections to scaling are analytic(ex-cept for logarithms).The shift exponentλdoes not coincide with1/ν.The FSS of the specific-heat pseudocritical point and peak have logarith-mic corrections.Apart from the leading term, this feature is absent in the critical specific heat. REFERENCES1.M.N.Barber,in:Phase Transitions and Crit-ical Phenomena,Vol.8,eds.C.Domb and J.L.Lebowitz(Academic Press,New York, 1983),p.145.2.H.J.Brascamp and H.Kunz,J.Math.Phys.15(1974)65.3. C.N.Yang and T.D.Lee,Phys.Rev.87(1952)404;ibid.410;M.E.Fisher,in:Lectures in Theoretical Physics,Vol.VIIC,ed.W.E.Brit-tin(Gordon and Breach,New York,1968), p.1.4. C.Itzykson,R.B.Pearson,and J.B.Zuber,Nucl.Phys.B220(1983)415.5. A.E.Ferdinand and M.E.Fisher,Phys.Rev.185(1969)832.6.N.Sh.Izmailian and C.-K.Hu,Phys.Rev.E(in print)[cond-mat/0009024].7.J.Salas,J.Phys.A34(2001)1311.8.J.Gonz´a lez and M.A.Mart´ın-Delgado,hep-th/9301057;O.Diego,J.Gonz´a lez,and J.Salas,J.Phys.A27(1994)2965;Ch.Hoel-bling and ng,Phys.Rev.B54(1996) 3434.9.N.A.Alves,J.R.Drugowich de Felicio,andU.H.E.Hansmann,Int.J.Mod.Phys.C8 (1997)1063.10.J.Zinn-Justin,Quantum Field Theory andCritical Phenomena,3rd ed.(Clarendon Press,Oxford,1996),p.636.11.G.Jug and B.N.Shalaev,J.Phys.A32(1999)7249.12.P.Calabrese,M.Caselle,A.Celi,A.Pelis-setto,and E.Vicari,J.Phys.A33(2000) 8155.13.M.Caselle,M.Hasenbusch,A.Pelissetto,andE.Vicari,cond-mat/0106372.14.B.Kaufman,Phys.Rev.76(1949)1232.15.W.Janke and R.Kenna,Phys.Rev.B(inprint)[cond-mat/0103332].。
Renormalization group and critical behaviour in gravitational collapse
Tatsuhiko Koike†
Department of Physics, Keio University, Hiyoshi, Kohoku, Yokohama 223, Japan
Satoshi Adachi‡
Department of Applied Physics, Tokyo Institute of Technology, Oh-Okayama, Meguro, Tokyo 152, Japan (July 4, 1996; revised: April 16, 1997)
A very important question here is how formation of a black hole depends on initial data, for example, which initial data evolve into black holes and which do not. It is concerned with many important problems such as cosmic censorship [1]. Christodoulou [2–5] rigorously analyzed such a problem in a relatively simple system, namely, spherically symmetric scalar field collapse. He proved that the field disperses at later times if the initial field is sufficiently weak, and also found a sufficient condition for black hole formation. However, the behaviour of the field and the space-time for initial data sets around the threshold of the black hole formation remained open, and he posed a question whether the phase transition between spacetimes with and without black holes is of the first or of the second order, i.e., whether the mass of the black hole formed is a continuous function at the threshold. Choptuik [6] numerically analyzed the system and obtained a result which strongly suggests the latter. Furthermore, he discovered a “critical behaviour” of the gravitational collapse of the system. His result can be summarized as follows: Let the initial distribution of the scalar field be parametrized smoothly by a parameter p, such that the solutions with the initial data p > pc contain a black hole while those with p < pc do not. For several one-parameter families investigated, near-critical solutions (p ≈ pc ) satisfy the following: (1) the critical solution (i.e. p = pc ) is universal in the sense that it approaches the identical space-time for all families, (2) the critical solution has a discrete self-similarity, and (3) for supercritical solutions (p > pc ) the black hole mass satisfies MBH ∝ (p − pc )βBH and the critical exponent βBH , which is about 0.37, is universal for all families. Abrahams and Evans [7] found similar phenomena in axisymmetric collapse of gravitational wave and obtained βBH = 0.38. Evans and Coleman [8] found similar phenomena with βBH ≃ 0.36 in spherically symmetric collapse of radiation fluid, in which case the self-similarity is not discrete but continuous. Employing a self-similar ansatz they also found a numerical solution which fits the inner region of the near-critical solutions very well. Since the above values of βBH were close to each other, some people considered that there is a universality over many systems.
Universality of the Ising Model on Sphere-like Lattices
a rXiv:h e p-la t/96225v126Fe b1996UTP-26-02-96Universality of the Ising model on sphere–like lattices Ch.Hoelbling and ng Institut f¨u r Theoretische Physik,Universit¨a t Graz,A-8010Graz,AUSTRIA February 1,2008Abstract We study the 2D Ising model on three different types of lattices that are topologically equivalent to spheres.The geometrical shapes are reminiscent of the surface of a pillow,a 3D cube and a sphere,respectively.Systems of volumes ranging up to O(105)sites are simu-lated and finite size scaling is analyzed.The partition function zeros and the values of various cumulants at their respective peak positions are determined and they agree with the scaling behavior expected from universality with the Onsager solution on the torus (ν=1).For the pseudocritical values of the coupling we find significant anomalies indicating a shift exponent =1for sphere–like lattice topology.11Motivation and introductionMost of the Monte Carlo studies of spin models have been done on hypercubic lattices with periodic boundary conditions,i.e.with the topology of a torus. Recently,however,there has been a growing interest in the effect of other topologies.Some of that interest is motivated by the advance of quantum gravity models,some by problems related to the role of topological excitations of the particular system.Various investigations[1–6]have been carried out on lattices topologically equivalent to the surface of a hypersphere in D+1dimensions.On sphere–like surfaces a loop can be continuously contracted to a point:The fundamental homotopy group is trivial.This has immediate consequences for the dynamics of string–like objects like monopole loops(in4D pure gauge theory with U(1)gauge symmetry)or the boundaries of clusters in2D spin models.We therefore might expect a different approach to the thermodynamic limit and differentfinite size corrections to scaling.Atfirst order phase transitions the phase mixture obtained in the ther-modynamic limit may be influenced by local changes,likefixing one spin,or changing the boundary conditions.The critical exponents however,should not depend on such effects.At second order phase transitions one expects that the critical properties are not affected by boundary conditions or by whether one works on lattices with torus or spherical surface geometries if either becomesflat in the infinite volume limit.Such an assumption of universality should be tested in practical examples,which is one of the mo-tivations for this work.Another question is whether thefinite size scaling (FSS)ansatz is general enough to persist.The important leading terms and the corrections to them may have different size depending on the lattices and their topology as has been observed in the4D and2D studies.The Ising model is explicitly solved for torus geometry[7]even onfinite lattices[8,9].It has a well understood2nd order phase transition.FSS of the bulk quantities is dominated by the leading term and provides a good example of the power of this method to determine critical indices.Here we want to present a Monte Carlo study for the Ising model on different2D lattices with the topology of the surface of a sphere:the surface of a3D cube,a pillow–like structure and the cubic surface projected to a sphere.In all these cases we determine cumulants and partition function zeros on different lattice sizes in order to study the size dependence and FSS in detail.After the introduction of these geometries in sect.2,the simulation2and multi–histogram analysis are discussed in sect.3and the results in sect.4. We conclude that there are sizable differences to the usual results on torus–like lattices,but that universality prevails.Preliminary results of this work have been presented in[6].2Lattice geometryThe most straightforward approach to constructing a sphere–like lattice would be triangulation.We want to stay as close as possible to the original action, however.This is partly motivated by the related studies[1]and[5],where one wants to keep a4-link plaquette structure.Also,two of the lattices studied here can be viewed at as combinations of the usual square lattices glued together at the boundaries;thus in the thermodynamic limit even the non–universal critical coupling ought to agree with that for torus geometry.The torus is our reference geometry;in addition three other lattice ge-ometries were used for our simulations(cf.fig.1).Torus TO[N]:The solution for the Ising model on an N×N lattice with periodic b.c.is known[8,9]and we will use this as the standard to compare our results with.Pillow PI[N]:This is the surface of a cube with N×N×2sites,where N will be called the base length in the subsequent discussion.Basically it is made out of two N×N lattices glued together at the edges.The curvature is concentrated in the4×2corners,elsewhere the lattice is locallyflat.This lattice PI[N]has2N2sites and4(N2−1)links. (Dual)Cube SH[N]:This lattice is dual to the surface of a3D cubic lattice of base length N.Each plaquette of the cubic surface is identified witha site of SH.This has the advantage,that each site has4links tonearest neighbors,like for the torus.The lattice has6(N−1)2sites and12(N−1)2links.The curvature is concentrated on the8×3corner points.Sphere S[N]:That lattice is defined by the sites on the surface of a N3 cube,projected onto the unit sphere.The site–link connectivity struc-ture is identical to that of the cube’s surface,the only difference lies in weight factors in the action,to be discussed below.The lattice has 6(N−1)2+2sites and12(N−1)2links.3The total energy(or action,if used in the context of quantumfield theo-ries)for the model is given byE=− x,µw x,ˆµs x s x+ˆµ(1)where the sum runs over all links(at sites x in directionsˆµ).The spin variables s x have values∈Z(2).The weight factors w x,ˆµare equal to1 for the torus and the lattice types PI and SH.The partition function is determined by the sumZ= C exp(−βE(C))(2)over all spin configurations C.For lattices PI and SH the curvature is concentrated around the corners. The deficit angle denotes the deviation of the sums of angles of plaquettes (or triangles)at a given site from theflat–space value2π.For PI its value isπ/2on each of the4×2corners,for SH it isπ/6on each of the8×3 corners.It vanishes on all other sites,as it does on the torus:The lattices areflat almost everywhere.The total curvature on the sphere–like lattices therefore has the value4πor Euler number2,as compared to0for the torus. Euler’s relation for sphere–like lattices is n s+n p−n l=2(n s,n p,and n l denote the total number of sites,plaquettes and links,respectively)whereas for torus topology this sum is zero.Both lattice types PI and SH can be imagined as built out offlat N×N pieces,glued together along their boundaries.The deviation from the torus shaped lattice thus disappears at least as fast as a boundary contribution O(1/N).The contribution from the corners,where the curvature is concen-trated,is suppressed O(1/N2).We expect that,although not a universal quantity,the value of the critical couplingβc(in the thermodynamic limit) coincides with that for the torus.In order to mimic a truly spherical lattice more closely,we also took the structure of a cubic surface lattice projected to the sphere as shown infig.1. Since the link connectivity structure does not change,the difference has to be expressed by modifying the weight factors accordingly.Christ et al.[10] discuss a possible definition for triangulated(random)surfaces,which obeys certain properties,that are necessary for the consistency of the continuum field theory at a second order phase transition.4Our lattices are built out of quadrangles and therefore we have to modifythat method for the derivation of the weight factors.We start with the scalar continuumfield theory with the Euclidean invariant kinetic termd2x(∂µφ(x))2.(3) (In fact,we can define the Ising model as a discretization of a scalarfield theory in the limit of infinite quartic self coupling.)The discretization ona lattice replaces the derivative term by the nearest neighbor differences,∂µφ(x)−→(φx+ˆµ−φx)/l x,x+ˆµ,where l x,y denotes the distance between the neighboring two points.The area differential d2x has to be replaced by anarea element A x,ˆµassigned to each lattice link(or site term).The discretizedkinetic term then leads to the link term of the lattice action(1),with the weight factor w x,ˆµ=2A x,ˆµ/l2x,x+ˆµ.The total lattice volume has to be split into lattice area elements at-tributed to the link contributions.These lattice area elements are constructed with help of the dual lattice,where each site may be defined as the barycenter of the plaquettes of the original lattice1(cf.fig.2).Links of the dual lattice are drawn between sites corresponding to neighboring plaquettes.Each link on the original lattice corresponds exactly to one link of the dual lattice.For simplicity we make two approximations:•We assume that all quadrangles areflat;in reality the four corners are not co–planar.In the thermodynamic limit the lattice becomes locally flat and the error vanishes.•We neglect angular distortions and approximate each quadrangle bya rectangle;this allows us to write the area assigned to a lattice linkx as the product of the lengths of the dual link with that of the linkitself,A x,ˆµ=11In[10]the center of periphery was used;there is no such point in a general quadrangle, therefore the center of mass seems to be a reasonable alternative.5This way the total lattice volume is distributed over all links.With these approximations wefind that the weight factors for the lattice geometry S[N]are just the ratio of dual link length to the link lengthw x,ˆµ≡l′x,ˆµ/l x,ˆµ(4) equivalent to the factor suggested in[10]for triangulations.For this particular sphere–like lattice we do not expect,that the thermo-dynamic limit value of the critical coupling is identical to that of the torus. Since we have introduced a change of the action affecting all links,βc will be renormalized.Still we expect universal behavior of the critical exponents,to be checked numerically.The computer programs use index tables to deal with the lattice geometry. For the lattices S[N]the weight factors are precalculated and tabulated.In our discussions we will refer to the lattice volumeV= x,µw x,ˆµ(5) as the typical size quantity.For lattices TO,PI and SH this is just the number of links.A length scale may be defined as L≡Base Length NPI S 1610202724.832409211650.0641638048147.012865532195726.9Table 1:The volumes V as defined in the text;the equivalent linear extent L =(V/2)1V (E − E )2 ,(7)V CLB (β,L )=−1 E 22,(8)U 4(β,L )= (E − E )4For each lattice size we simulated the system at up to20different values ofβbetween0.41and0.47.The integrated autocorrelation times for the energy varied betweenτ≈3−7.For each size we produced between2 and5×106independent configurations.The errors were estimated with the jackknife algorithm,i.e.from the variation of the results for the analysis of subsamples of the raw data.Throughout the discussion of the data we use L≡2The goodness offit parameter Q is defined as Q=Γ(n−p2),where n is thenumber offit points and p is the number offit parameters.It is the integrated probability over allχ2larger than the measured one.8We denote byβc(L)our definitions for pseudocritical points:The posi-tions of the extrema in the cumulants.The so–called shift–exponentλis for many models equal to1/ν,but not necessarily so in general;this relation is not a necessary conclusion of FSS(cf.the discussion in[19]).We return to this issue in the discussion of the results.A priori we know nothing about the absolute size of the multiplicative coefficients in the scaling formulas.They depend on the details of the lattice geometry and topology and on the boundary conditions.The FSS behavior comes from the rescaling properties of the bulk quan-tities.The effect of changing the boundary properties may be responsible for further contributions.The non–homogeneous distribution of the curvature in our lattices PI and SH might also be responsible for additional(constant) terms in the total free energy.Actually,since the total curvature is an invariant,there may be another contribution,which—relative to the bulk contribution O(V)—becomes irrelevant in the thermodynamic limit.It has been shown[20],that the total free energy forfinite2D systems with non–singular metric and smooth bound-aries has at criticality(in addition to boundary terms O(L))an asymptotic contribution proportional to ln L.The proportionality constant is a prod-uct of the central conformal charge and the Euler number(vanishing for the torus).Thus this contribution depends only on the topology of the system, not on the shape of the boundary.All these contributions to the free energy are suppressed O(1/L2)or O(ln L/L2)relative to the leading term.In the absence of a strict theory we therefore might expect corresponding additive corrections terms in the FSS relations(11)–(15).4.2Cumulant values and partition function zerosThe values of the cumulants at their respective pseudocritical points provide information on the critical exponents according to(11)–(13).As discussed, they may have geometry dependent corrections.However,in our data we find qualitatively excellent agreement with the scaling of the torus–results and no significant indication of geometry–corrections.Fig.3shows that the specific heat scales with ln L,as expected forα=0.A power lawfit gives a value forαcompatible with0and has a largerχ2: The logarithmic behavior is preferred.Comparing the results for the higher order cumulants V CLB and U4we9alsofind excellent agreement with the torus results,if compared at the corre-sponding scales L,and with the expected scaling behavior forα=0according to(12)–(13).In particular the results for V CLB lie on top of a common curve for all geometries.Thefinite size dependence of the positions of the partition function zeros confirms this observation.Infig.4the nearest Fisher zeros for sphere–like lattices are compared with those for toroidal lattice.The real part is substantially closer to the thermodynamic limit.Its scaling properties are discussed below together with the pseudocritical points derived from the cumulants.The imaginary part of the closest Fisher zero appears to profit from the smallness of the deviation of the real part from the thermodynamic value. The log–log plot(fig.5)demonstrates the excellent scaling signal and afit of the formIm z0(L)=aL−1/ν(16) givesν=0.9964(46)(goodness offit Q=0.39)for PI,ν=0.9975(57) (Q=0.77)for SH andν=1.0023(54)(Q=0.12)for S lattices.For all these lattices the result is in perfect agreement with the valueν=1of the toroidal lattice.We conclude,that the imaginary part of thefirst partition function zero is an optimal observable for extracting the critical exponentν.It appears to be least affected by correction to scaling due to lattice topology and boundary effects.In this light the excellent scaling behavior of the specific heat should not be too surprising,since the peak value is directly related to the vicinity of the closest Fisher zero.Since the partition function is proportional to the product of all zeros,Z∝ i(β−z i)(17) the specific heat includes for its singular part the contributioni1the specific heat itself.Infig.6we compare the torus results with those for the cubic surface lattices for equivalent lattice volumes.The approach to the infinite volume case(Onsager solution)is in a much more symmetric way than for the torus lattice.4.3Pseudocritical pointsWe discuss here the pseudocritical values derived from-the peak positions of the specific heat,-the minima positions of the other cumulants V CLB and U4,-the real part of the position of the closest zero in the complexβ–plane. For the lattice geometries PI and SH we expect(see the discussion in sect.2)that in the thermodynamic limit the critical valuesβc coincide with those of the torus,and we therefore present these results in direct comparison. For the lattice type S the asymptotic value of the critical coupling will be somewhat different and we discuss these results separately.4.3.1PI and SH latticesIt turns out,that both lattice geometries have very similar behavior and agree (except for the smallest lattice PI[16])even numerically with each other,if compared at corresponding volumes.Asfig.7clearly exhibits,there is an obvious difference in the FSS behav-ior compared to the usual torus results.The overall size of the corrections to the thermodynamic value of the critical coupling are much smaller for the sphere–like lattices.The leading FSS behavior ofβc(L)for large L should follow(15).For the Ising model on a torus the shift exponent isλ=1/ν=1 [9].This leading behavior linear in1/L is evident in thefigure.However,for PI and SH another effect seems to blur this picture:A possible(but clearly very small)linear term is dominated by contributions nonlinear in1/L.As discussed in[19]the leading linear term may vanish even for N×M torus geometry,depending on the ratio N/M.In particular it vanishes in the limit M→∞,where the leading behavior becomes O(ln L/L2)[9].There are also other specific models and cases,whereλ=1/ν[19].As mentioned below (15)also the topology may give rise to additional terms[20]in the free energy11(per unit volume)proportional to the Euler number and to O(ln L/L2);it is unclear how these affect the pseudocritical points in our particular situation.This observation,that the dominating behavior appears to be non–linear in1/L,was also made in a study of the Ising model for a honeycomb lattice on a tetrahedron surface[3].Both,series and Monte Carlo results led to a valueλ=1.745(15)[3].The value ofνobtained there from the correlation length and the specific heat agreed with the Onsager value.We thereforefit our data for the pseudocritical points toβc(L)−βc=aL−1+bL−λ,(19)βc(L)−βc=aL−1+bL−2ln L,(20) with the Onsager value forβc=12).The data for each of the4definitions of pseudocritical coupling(from c V,V CLB,U4and Re z0)appears to be consistent for both geometries PI and SH.We therefore use one set of parameters a and b different for each definition but identical for the two geometries.The value ofλis assumed to be universal for all definitions and both geometries.Wefit to data for N≥32.The results according to(19)are given in table2and are plotted infig.7:theyfit the data perfectly with aχ2/d.f.≃1.2(Q=0.26).Lattice Par.V CLB Re z0 PI,SH a0.000(13)0.009(10)b-4.29(96)-0.45(24)1.71(10)0.028(10)0.032(11)-0.62(13)-0.24(14)the samefit quality and would be indistinguishable in thefigure.Alsofixing λto a value2is still compatible with the data.We conclude that we are in a situation where a possible leading FSS term O(1/L)has an(almost or completely)vanishing coefficient and the subleading terms dominate.This resembles the Ising model on a cylinder with infinite extension in one direction.It cannot be decided,whether the corresponding term is of form(19)or(20).4.3.2Spherical surface latticesNow we turn to the approximate spherical surface topology(S).Whereas for the pillow and cubic surface lattices the curvature is concentrated in8or 24points here it is more or less uniformly distributed among all sites of the lattice.The total curvature(the Euler number)remains constant.Infig.8the peak positions of the specific heat and the other cumulants are plotted together withfitted curves according to(19).Hereβc is a free parameter,otherwise we follow the procedure discussed above,i.e.one com-mon value ofλbut different parameters a and b depending on the observable. Since we have fewer data we include the data from the smaller lattices with N=16.This is also justified by the overall smaller deviations from the asymptotic value.The resulting values are also given in table2.Wefind a behavior in agreement with the other sphere–like lattices.The contribution of the term O(1/L)is again very small and the non–linear term dominates again.The overall variation of the pseudocritical points with L is for most observables smaller than for the other lattice geometries.Thefitted critical temperature isβc=0.43883(3)with aχ2/d.f.≃0.5(Q=0.81).The value ofλ=1.71(10) is consistent.Again thefit to(20)gives results of comparable quality and corresponding curves would be indistinguishable in thefigure.5ConclusionWe have performed a high statistics Monte Carlo study of the Ising model on lattices of various size and different shapes,all with sphere–like topology. Our FSS analysis led to the following conclusions.13•We have found explicitly,that the Ising model on a spherical surface topology lies in the same universality class as the planar Ising model with periodic boundary conditions—topologically the surface of a torus.Our results demonstrate that universality holds,independent of the lattice geometry.This agrees with similar conclusions obtained for tetrahedral lattices[3]and random lattices[4]of sphere–like topology.•However,some observables are not well suited tofind the expected leading FSS behavior.Different observables vary in their sensitivity. Of the studied quantities(in the even sector of the Ising model)wefind that the imaginary part of the Fisher zero closest to the real axis has the smallest(in fact:not identifiable within our accuracy)deviations from the leading FSS behavior.Related to this quantity,also the peak value of the specific heat scales according to the FSS formulas with the Onsager values for the critical exponents without further(identifiable) corrections.The values of the other cumulant have larger statistical errors but are also in agreement with the torus results.•The change in the topology class influences the size of the FSS contri-butions.This appears to affect in particular the pseudocritical points. Wefind no significant contribution of O(1/L),which is the dominant FSS term for the torus pseudocritical points(with a shift exponent λ=1/ν=1).Instead wefind that the FSS behavior is dominated by a term O(L−λ)with a mean valueλ≃1.74(6)(averaging the results for PI,SH and S).A compatible value was obtained in an independent study for tetrahedral lattices[3].The behavior seems to be universal for all sphere–like lattices,independent of the details of the geometry. This contribution is also consistent with a term O(ln L/L2);such a term describes the FSS of the specific heat peak position for the Ising model in cylinder geometry[9].It also has been argued,that a term of that kind contributes to the free energy per unit volume for systems with non–zero Euler number[20].Unfortunately this implies that none of these observables is qualified to derive the critical exponentν.•In general wefind that the studied sphere–like lattices have smaller corrections to the infinite volume behavior than one observes for the torus(i.e.periodic boundary conditions).The approach to the ther-modynamic shapes is faster and in a more symmetric way.14•Our analysis of the Fisher zeros of the partition function is consistent with this picture.With increasing size the closest zero approaches the real axis almost perpendicular.(Note,that this behavior is afinite size behavior and is not identical to the asymptotic impact angle–defined e.g.as the angle between thefirst and second zero).The results for the spherical surface geometry appear to be closest to the thermodynamic behavior in general.For different lattice(sphere–like)geometries the FSS behavior is consistent if one chooses the size variable L=References[1]ng and T.Neuhaus,Nucl.Phys.B431,119(1994).[2]J.Jers´a k,ng,and T.Neuhaus,Nucl.Phys.B(Proc.Suppl.)42,672(1995).[3]O.Diego,J.Gonz´a lez,and J.Salas,J.Phys.A27,2965(1994).[4]C.Holm and W.Janke,FUB-HEP18/95,KOMA-95-81,hep-lat/9512002to appear in Nucl.Phys.B(Proc.Suppl.)(1996).[5]H.Gausterer and ng,Nucl.Phys.B455,785(1995).[6]C.Hoelbling,A.Jakovac,J.Jers´a k,ng and T.Neuhaus,preprintUNIGRAZ-UTP-070995,hep-lat/9509009,to appear in Nucl.Phys.B (Proc.Suppl.)(1996).[7]L.Onsager,Phys.Rev.65,117(1944).[8]B.Kaufman,Phys.Rev.76,1232(1949).[9]A.E.Ferdinand and M.Fisher,Phys.Rev.185,832(1969).[10]N.H.Christ,R.Friedberg,and T.D.Lee,Nucl.Phys.B210[FS6],337(1982).[11]R.H.Swendsen and J.-S.Wang,Phys.Rev.Lett.58,86(1987).[12]A.M.Ferrenberg and R.H.Swendsen,Phys.Rev.Lett.61,2635(1988),Err.,ibid.63,1658(1989);ibid.,Phys.Rev.Lett.63,1195(1989). [13]M.S.S.Challa,ndau,and K.Binder,Phys.Rev.B34,1841(1986).[14]K.Binder,in Computational Methods in Field Theory,Lecture Notes inPhysics409,edited by H.Gausterer and ng(Springer-Verlag, Berlin,Heidelberg,1992),p.59.[15]C.N.Yang and T.D.Lee,Phys.Rev.87,404(1952).[16]M.E.Fisher,in Lectures in Theoretical Physics,edited by W.E.Brittin(Gordon and Breach,New York,1968),Vol.VIIC,p.1.16[17]R.Kenna and ng,Nucl.Phys.B393,461(1993),Err.ibid.B411,340(1994);Phys.Rev.E49,5012(1994).[18]M.E.Fisher,in Critical Phenomena,Proc.of the51th Enrico FermiSummer School,Varena,edited by M.S.Green(Academic Press,New York,1972).M.E.Fisher and M.N.Barber,Phys.Rev.Lett.28,1516 (1972).E.Br´e zin,J.Physique43,15(1982).J.L.Cardy,in Finite–Size Scaling,edited by J.L.Cardy(North-Holland,Amsterdam,1988),p.1.[19]M.N.Barber,in Phase Transitions and Critical Phenomena,Vol.8,edited by C.Domb and J.Lebowitz(Academic Press,New York,1983), Vol.VIII,Chap.2,p.104.[20]J.L.Cardy and I.Peschel,Nucl.Phys.B300[FS22],377(1988).17Figure1:Lattices PI[6],SH[6]and S[6].2050100200500L45678V c Figure 3:Specific heat peak values vs.ln L for lattices PI ,SH ,TO and S .Here and in all the other figures the error bars are smaller than the symbols.19Im(z 0)00.020.04Re(z 0)Figure 4:(a)Position of the partition function zero closest to the real axis in the complex βplane for different lattices.The numbers indicate the base length N .The real part of the zeros are closer to their thermodynamic value for the sphere–like lattices than for the torus.In (b)we plot the results for the spherical surface lattices S .2030100300L0.010.030.003Im(z 0)Figure 5:Plot of ln(Im z 0)vs.ln L ;the fit represents the leading FSS behavior.210.410.430.450.47β2.003.004.005.00c VTO SHthermodyn. limit Figure 6:Specific heat per unit volume vs.βfor TO [37]and SH [16];these lattices of similar volume are compared to the Onsager solution.One finds that the curve for the SH lattice is more symmetric around βc than for the TO .220.010.020.031/L0.4380.4390.44β0.4340.4350.4360.4370.4380.4390.44β0.010.020.031/L0.4380.4390.44β0.4380.4390.44βFigure 7:Results for the pseudocritical coupling vs.L for (a)the specific heat c V and V CLB ,(b)the real part of the closest partition function zero and U 4,for pillow,dual cube and torus type lattices.The curves are fits according to (19)for the pillow and cubic surface lattices as described in the text.2300.010.020.031/L0.4320.4340.4360.4380.440βFigure 8:Peak positions of the cumulants on spherical surface lattices S .One can clearly see,that βc differs from the critical temperature on the torus βc,T O ≈0.44068.The curves are from fits to (19.)The error bars are smaller than the symbols.24。
2023-2024学年辽宁省部分学校高二下学期6月份阶段考英语试卷
2023-2024学年辽宁省部分学校高二下学期6月份阶段考英语试卷Art Contest-Technology &You!Technology is everywhere these days. Automation has pioneered innovation. Your phone is probably in your pocket or your hands at all times, and now it’s easier than ever to communicate with anyone in the world. What are your thoughts on technology, social media or your phone? Do you feel excitement every time you get a notification message, or do you feel tied down by these digital “chains”?However you feel, we want you to put that into artwork-paintings, digital art or photography. One winner and several honorable mentions will be featured in the December 2024 magazine, and the winner will receive a $25 gift card! You may even see your art work in future issues of Teen Ink magazine.Deadline: Nov. 1, 2024Details and requirements:Entrants must have a Teen Ink account and be aged 13~19.Inappropriate content will not be accepted.Submissions must relate to the topic(technology).Entries must be a piece of artwork created by the entrants themselves.Entrants can submit as many pieces of art as they wish.How to submit:Entries can be submitted through the Teen Ink website. All entries submitted will be reviewed and considered for the contest. See our submission guidelines for more information.Make sure to submit your art work to the appropriate art category(technology) on Teen Ink. You can do this by using the “additional tags(标签)” field in your submission form.1. What is the main theme of the art contest?A.The development of technology. B.The application of technology.C.Innovations of technology. D.Viewpoints on technology.2. What is one of the requirements for submitting artwork to the contest?A.Submit original artwork. B.Submit artwork with a unique tag.C.Submit different types of artwork. D.Submit only one piece of artwork.3. What is Teen Ink?A.A library. B.A magazine. C.An art school. D.An art museum.The public footpath laid barely 20 meters from where I stood, promising a walk along the river, passing fields and through woodland, well away from any road. Yet there was something in my way—the River Thames.I checked my map to see how to reach the path, but there was no other footpath that would lead me to the island on which it sat. It was only accessible by boat—kid’s dream. Similar to a talent show, some performances are educational but mostly, they just make you laugh. Talent is irrelevant, and audience engagement through call and response is essential.Away from phones and peers back home, social norms fade and space for self-exploration forms. Shy kids come out of their shells, and cool kids let their guard down. They get to open up this door to a part of themselves that they wouldn’t have felt safe to reveal at school or at home.It’s been a decade since my last performance as a camp counselor, and I never thought of skits from a skill-building perspective. But I now realize this rich camp tradition left a great impression on me. Through camp skits, I developed my sense of humor, built confidence in front of a crowd, and learned how to accept others for their quirks(怪癖).Maybe we can make our schools or communities more like summer camps by bringing the silliness of skits into our families and classrooms to reconnect with ourselves and each other. The next time you’re sitting around a campfire with friends and family, give it a try. Embrace the discomfort and invite your loved ones to join in on the improvising(即兴创作). And remember: the more funny noises and childlike humor, the better.4. What is the main purpose of skit performances at summer camps?A.To entertain and engage the audience. B.To showcase talent and skills.C.To educate the audience. D.To compete with fellow campers.5. What does the un derlined phrase “let their guard down” in Paragraph 3 mean?A.Defend. B.Relax. C.Mature. D.Respond.6. How did the author benefit from camp skits?A.She developed a competitive spirit. B.She understood social norms better.C.She became more tolerant. D.She became more creative.7. What does the author advise us to do?A.Take up challenges in life. B.Accept our imperfections.C.Participate in more community activities. D.Break out of our comfort zone.When it comes to architectural accomplishments, humans like to think they stand at the top. That is to underestimate the astonishing achievement s of social insects; for example, white ants raise skyscraping nests. The true master builders of the insect world, however, are the hundreds of species of stingless bees.In a new study, Ms. Di Pietro and her colleagues observed over 400 colonies of the stingless bee species in a large bee house in Brazil in 2022 and 2023. Around 95% of the colonies exhibitedhoneycombs(a structure made by bees) built up in horizontal layers(水平分层), like tiered wedding cakes, while the rest adopted a spiral(螺旋的) structure.Since the stingless bee shows a strong preference for a horizontal-layer honeycomb structure, it’s surprising that spiral honeycombs occur. The team confirmed that there was no difference in the average cell-building rate between the two styles, and therefore no efficiency advantage.In order to rule out a genetic explanation for the different styles, the researchers transplanted workers from colonies that built in one tradition to colonies that built in the other, having first emptied the host structures of their native adults. The imported workers soon switched to the local style, which was then continued by the colony’s young insects as they eventually matured into workers.Dr. Tom Wenseleers guessed that the bees may switch styles as a way of coping with the build-up of small construction errors made by their fore-runners. Such a process, in which multiple organisms indirectly affect each other’s behavior thro ugh the traces they leave in their environment, is known as stigmergy(共识主动性). The researchers later introduced a sign of spirals to the otherwise perfect horizontal-layer honeycombs, and found that it did indeed cause the bees to switch to building spirals.These results suggest that stingless bees can pass on different building traditions across generations and individuals needn’t be instructed by their peers. “The findings are the clearest demonstration of cultural differences naturally appearing in insects. Insect culture would once have been thought impossible,” says behavioral biologist Andrew Whiten, who wasn’t involved in the research. “Less than a century ago, culture was thought to be uniquely human.”8. How does the author introduce the topic of the text?A.By posing a contrast. B.By reporting an event.C.By supposing a situation. D.By justifying an assumption.9. What can be inferred about the stingless bees’ honeycomb-building behavior?A.It is a result driven by genetic factors.B.It involves cost and efficiency considerations.C.It is switched constantly between several styles.D.It shows flexibility in the changing environments.10. What is Paragraph 5 mainly about?A.The impact of fore-runners’ behavior on other stingless bees.B.The und erlying logic behind stingless bees’ building styles.C.The advantages of maintaining stigmergy among stingless bees.D.The significance of correcting small errors during construction.11. What is Andrew Whiten’s attitude towards the findings of the stu dy?A.Doubtful. B.Conservative.C.Favorable. D.Critical.The American Psychological Association(APA) has issued its first advisory on social media use in adolescence(青春期). What’s most striking in its data based on recommendations is how little we really know about how these apps affect our kids.The relative newness of platforms like Snapchat and Tik Tok means little research is available about their long-term effects on teen and tween brains. Getting better data will require significant funding—and much more openness from tech companies.“What little evidence we do have unsurprisingly suggests that social media trades on motivators that aren’t great for young brains. Many kids’ first exposure to social media occurs at the worst possible time when it come s to brain development,” says Mitch Prinstein, a psychologist and neuroscientist at the University of North Carolina(UNC).“Things like ‘button and artificial intelligence(in general)’ are going to affect young people’s brains in a way that’s very differen t from adult brains when it comes to the desire to stay online and to say or do almost anything to get followers.” When it comes to social interactions, he compares kids’ brains to a car with a huge gas pedal and weak brakes(刹车).Earlier this year, Prinstein and his UNC colleagues published the results of one of the first studies of how the adolescent brain reacts to social media. The team surveyed a group of middle schoolers to understand their social media habits, and then stuck them in an MRI machine to watch their brains as they reacted to social rewards or punishments. They found that 12-year-olds who habitually checked social media had distinct neural patterns, with more activities over time in parts of the brain associated with motivation, salience(or where attention is focused) and cognitive control.The team didn’t weigh in on whether those differences were good or bad, or whether the relationship was causal or correlational. But their work points to the need for more research. It should also remind parents of the need to be keenly aware of social media’s hidden influence on still-developing brains.12. What issue regarding social media apps does the APA report highlight?A.Their addictive nature. B.The lack of data on their influence.C.The dishonesty of their developers. D.The ineffectiveness of their incentives. 13. Which word can best describe young brains in relation to social interactions?A.Uncontrolled. B.Sensitive. C.Unpredictable. D.Productive.14. What did Prinstein’s team discover about adolescents who regularly use social media?A.They are usually highly motivated. B.They find it difficult to concentrate.C.They have greater cognitive control. D.Their brains show unique features.15. What might be the best title for the text?A.Empowering Teens in the Digital AgeB.How to Guide Teens’ Social Media EngagementC.The Hidden Influence of Social Media on Young MindsD.The Importance of Healthy Social Media HabitsMaking the decision to invest in healthy lifestyle changes is more than just flipping a switch. 16 . Psychologists have found that it takes an average of 66 days for a new habit to become automatic, but the truth is that building and maintaining lifestyle changes is highly dependent on each individual. However, there are some easy strategies that can help you develop a lifestyle change plan that works for you.Focus on the whole picture. Lifestyle changes are like a puzzle. There are many pieces that must add up to the whole picture. Building habits in only one area of the puzzle will leave your overall picture lacking dimension. 17 , so it is important to understand how they all interact when setting up your lifestyle change plan.Set realistic and achievable goals. 18 , focus on setting goals that are realistic. Instead of expecting to run a marathon in six months, shoot for running a 5-kilometer race then work up to the marathon. Setting realistic goals that you can achieve and then building on them will help you maintain momentum (动力)and stay motivated.19 Building habits takes time. Be patient with yourself and understand that the fastest way forward isn’t always the smartest way forward. The goal in creating lifestyle changes isn’t to get to the finish line as quickly as possible. The goal is to build habits that are sustainable in your everyday life. 20 .Looking back, the memory of doctors, nurses and the conclusion of appendicitis(阑尾炎) was still clear. ______, nothing hurt more than three days with appendicitis. After a series of emergencies, I could merely lie ______ and beg my body to stop hurting.All the ______ acquired from years of swimming was eaten away. Previously, I could swim miles daily. Now it was a(n)______ to sit up and I couldn’t swim for almost three months.When I finally returned to the pool, I struggled with my ______ ability. Race after race, I ______ my goals. Every time I ______ to enter the national competitions, I failed by a tiny amount.Finally, I came to the last event that could ______ me for nationals. This was my last ______ : now or never. After so many failures, I couldn’t help being furious about recent events.The race started, and I dived in, throwing the pain, ______ and anger I had experienced recently into the pool. My mind focused, self-limitation was ______ and I devoted all my attention and strength to my moves.When I saw my time, a wave of ______ swept over me. I eventually ______ self-doubt and won what almost ______ from me. Nationals were waiting for me, and by no means would I let anything ______ my advancement.21.A.Normally B.Frankly C.Fortunately D.Hopefully22.A.motionless B.disappointed C.unconscious D.senseless23.A.experience B.knowledge C.muscle D.honor24.A.option B.effort C.fantasy D.embarrassment25.A.regained B.fundamental C.reliable D.limited26.A.took notice of B.fell short of C.was aware of D.ran away from27.A.attempted B.applied C.declared D.determined28.A.train B.sponsor C.qualify D.instruct29.A.enemy B.performance C.failure D.shot30.A.strength B.uncertainty C.depression D.criticism31.A.taken over B.knocked down C.given away D.cut off32.A.sorrow B.gratitude C.confusion D.relief33.A.overcame B.understood C.ignored D.recognised34.A.benefited B.resulted C.originated D.escaped35.A.see through B.look over C.hold back D.account for阅读下面短文,在空白处填入1个适当的单词或括号内单词的正确形式。
2006年考研英语答案解析和参考译文(二)
2006年考研英语答案解析和参考译文(二)SectionⅠUse of English篇章导读本文是一篇论说文。
文章的主题是"英才通才教育"。
作者在文章开头就提出了一个具有选择性的问题:"如果我们只是需要决定是把基本的科学传授给每个人,还是找一些有才华的人,引领他们变得更出色,那么我们的工作将会相当容易。
"随后作者从"the education in public school,the balance among the branches of knowledge and the balance between current and classical knowledge"三个方面来论述在教育中保持知识平衡的重要性。
解读文章时注意作者的客观态度。
思路解析1「答案」[C]「解析」"选择"。
根据文章一致性原则,"choice"与文章第一句中的"decide决定"形成呼应,根据原文"decide whether......or......"所以下文就应该是对其有所"选择choice"或没有"选择choice"。
而选项[A]"(与属性区别的)本质:the entity of justice 正义的本质",[B]"拍卖;(某些纸牌戏中的)叫牌;叫牌阶段",[D]"结合体,联合;(政党、个人、国家等)临时结成的联盟"是本题的干扰,均不形成呼应,不符合题意。
「解析」"因为"。
"for"与文章第一段第三句中的"Because we depend......"构成搭配,均表示解释原因。
而选项[A][B][C]均不用于解释原因,不符合原文意思。
Regularly alternating spin-12 anisotropic XY chains The ground-state and thermodynamic prop
arXiv:cond-mat/0408033v1 [cond-mat.stat-mech] 2 Aug 2004
I.
INTRspin– 2 Ising chain in a transverse field (transverse Ising chain) is known as the simplest model in the quantum theory of magnetism. It can be viewed 1 anisotropic XY model in a transverse as the 1D spin– 2 (z ) field with extremely anisotropic exchange interaction. By means of the Jordan–Wigner transformation it can be reduced to a 1D model of noninteracting spinless fermions1,2,3,4 . As a result the transverse Ising chain appeared to be an easy case5 and a lot of studies on that model have emerged up till now. After the properties of the basic skeleton model were understood various modifications were introduced into the model and the effects of the introduced changes were examined. For example, an analysis of the critical behavior of the chain with an
北京卷D篇WhyCollegeIsNotHome专业知识
controlled by their elders. If acceptable social behavior is
too strictly defined and controlled, the insensitive or
aggressive behavior (that administrators are seeking to
important. Because a college community(群体) differs from the family, many students will struggle to find a sense of belonging. If students rely on administrators to regulate their social behavior and thinking pattern, they are not facing the challenge of finding an identity within a larger and complex community.
minimize) may actually be encouraged.
再者,大学对学生行为旳监管和塑造和年轻人旳个性特
征背道而驰,那就是受长辈控制旳反应。假如可接受旳
社会行为被过于严格地要求,实际上可能会激发麻木不
Chandra Observations of Extended X-ray Emission in Arp 220
a r X i v :a s t r o -p h /0303316v 1 13 M a r 2003Chandra Observations of Extended X-ray Emission in Arp 220J.C.McDowellHarvard-Smithsonian Centre for Astrophysics,60Garden Street,Cambridge,MA 02138,USA jcm@ D.L.Clements Physics Dept.,Imperial College,Prince Consort Road,London SW72BW,UK d.clements@ mb Center for Theoretical Astrophysics,Departments of Physics and Astronomy,Loomis Laboratory,University of Illinois,1110W.Green Street,Urbana,IL 61801,USA S.Shaked University of Arizona,Dept.Astronomy,933North Cherry Avenue,Tucson,AZ 85721-0065,USA N.C.HearnCenter for Theoretical Astrophysics,Department of Physics,Loomis Laboratory,University of Illinois,1110W.Green Street,Urbana,IL 61801,USAL.Colinalnstituto de Estructura de la Materia (CSIC),Serrano 121,28006Madrid,SpainC.MundellARI,Liverpool John Moores University,Twelve Quays House,Egerton Warf,Birkenhead,Wirral,Cheshire,CH411LD,UKK.BorneRaytheon Information Technology and Sciences Services,NASA Goddard Space FlightCentre,Greenbelt,MD20771,USAA.C.BakerDept.Physics and Astronomy,CardiffUniversity,PO Box913,Cardiff,CF243YB,UKS.ArribasSpace Telescope Science Institute,ESA Space Telescope Division,3700San Martin Drive,Baltimore,MD21218ReceivedABSTRACTWe resolve the extended X-ray emission from the prototypical ultraluminous infrared galaxy Arp220.Extended,faint edge-brightened,soft X-ray lobes out-side the optical galaxy are observed to a distance of10to15kpc on each side ofthe nuclear region.Bright plumes inside the optical isophotes coincide with theoptical line emission and extend11kpc from end to end across the nucleus.Thedata for the plumes cannot befit by a single temperature plasma,and display arange of temperatures from0.2to1keV.The plumes emerge from bright,diffusecircumnuclear emission in the inner3kpc centered on the Hαpeak,which isdisplaced from the radio nuclei.There is a close morphological correspondencebetween the Hαand soft X-ray emission on all spatial scales.We interpret theplumes as a starburst-driven superwind,and discuss two interpretations of theemission from the lobes in the context of simulations of the merger dynamics ofArp220.Subject headings:galaxies:starburst—galaxies:individual(Arp220)—X-Rays:galaxies1.IntroductionThe evolutionary importance of energetic events on galactic scales has become central to our present understanding of cosmological evolution.The realization in the IRAS era (e.g.Soifer et al.1984)that super-starburst ultraluminous infrared galaxies rivalled quasars in their energy output made it clear that for at least a subset of galaxies a large fraction of their stellar content and gas mass is drastically rearranged during interactions which lastfrom108to109years(Clements et al.1996)The observation of superwinds(Chevalier& Clegg1985)emphasizes the role of energetic events in galaxies in redistributing material both within a galaxy and into the intergalactic medium.The energy and momentum involved in the biggest train wrecks in the universe are released in a number of different channels:stellar velocity dispersions,tidal disruption,gas heating,mechanical energy deposited in the gas and stars,shock-triggered star formation and subsequent infrared emission.Truman H.Safford(1836-1901)discovered the nebula Safford7(IC1127)at Chicago on1866May4(Safford1887),but recorded its position with an RA offby one minute of time.Javelle1(1905)rediscovered it as Javelle1368at Nice on1903Jul25.It was recorded by Dreyer in IC2(Dreyer1910)as IC4553,but the object remained obscure until A.G Wilson identified it on Palomar Sky Survey prints as unusual and Arp(1966)included it in his catalog of peculiar galaxies as Arp220,the designation by which it is most commonly known today.The discovery of strong OH maser emission(Baan,Wood&Haschick1982) and ultra-luminous far infrared output(Soifer et al.1984)established Arp220as the prototypical infrared superluminous merger.ISO observations(e.g.Genzel et al.1998, Lutz et al.1998)support a starburst interpretation for the bulk of the luminosity and Scoville et al.(1998)locate a number of massive star clusters in the nuclear region using NICMOS.At a distance of76Mpc(z=0.018;Kim&Sanders1998),it is one of the most luminous objects in the local universe.The galaxy,with an apparent B magnitude of13.9 and a total infrared luminosity(10-100microns)of1.5×1012L⊙,is believed to have been formed by the almost face-on collision of two spiral disks.In the optical,Arp220appears irregular and dusty,but other wavebands have been used to probe into the center of the object and reveal the presence of activity within a few parsecs of the nucleus.VLBI observations of Arp220suggest that the peak of the OH emission originates in a structure 1pc across(Lonsdale et al.1994)and Rieke et al. (1985)claimed that as much as half of the luminosity in Arp220may be due to an active nucleus.Armus et al.(1995)used near-infrared spectra to suggest that as much as80-90% of the total luminosity is powered by an obscured AGN.Dudley and Wynn-Williams(1997) use the depth of the silicate absorption feature to estimate a size for the emission region at 10microns of only a few parsecs.Eales&Arnaud(1988)reported thefirst detection of X-rays from Arp220,using the Einstein IPC.However,their observation was confused by emission from a neighbouring group of galaxiesfirst noted by Heckman et al.(1996)who carried out thefirst detailed study of the X-ray properties of the galaxy with the ROSAT PSPC.Their data show that the X-ray emission in the0.1-2.4keV band has a size of∼30×11kpc and a luminosity of between4.3×1040and2.3×1041ergs s−1and set an upper limit of∼20%of the observed X-ray emission associated with any single point source.They noted that the spatial extent of the X-ray emission was around22kpc,much larger than the IR-emitting region,and that the X-ray luminosity was an order of magnitude larger than that of normal spiral galaxies. The”double-bubble”morphology seen in optical emission-line images(Heckman,Armus& Miley1987)coincided with the X-ray nebula seen with ROSAT,but the spatial resolution of those data was insufficient for a detailed comparison.Heckman et al.suggested that both the X-ray and line emission is due to a bipolar”superwind”driven out from the nucleus by a starburst or a dust-shrouded QSO.Gallagher et al(2002)report similar extendedX-ray emission in the ultraluminous galaxy Markarian231,although at z=0.042the spatial resolution of their Chandra image reveals less detail than the observations presented here.2.Observations and Data AnalysisWe observed Arp220on2000Jun24for56ks with the ACIS camera on the Chandra X-ray Observatory as part of the Cycle1guest observer program.Arp220was placed on the S3back illuminated chip near the node0/node1boundary.Here we report on the extended emission from Arp220;Clements et al(2002,Paper I)discuss the point sources in the nuclear region.Data reduction was carried out with CIAO version2.1and 2.2.The data were taken with the chip at a temperature of-120C and were gain-corrected using the revisedfile acisD2000-01-29gainN0003.fits from the July2001recalibration, which improves the calibration at low energies.The observation was relatively unaffected by backgroundflares and only a small amount of exposure was removed,leaving aneffective exposure time of55756s.Astrometry was corrected using a revised geometryfile (telD1999-07-23geomN0004.fits)which is believed to provide positions across the full ACIS field accurate to about1arcsecond.The extended emission from Arp220is clearly visible in the raw data.The west lobe is dithered partly across the node0boundary,but the remainder of the emission is all on node1.We generated spectral responses making use of the recently recalibrated (acisD2000-01-29fefthe morphology of the region and allow regions of different spectral properties to be distinguished.The smoothed images were used in further analysis only to define extraction regions,not to determine any numerical quantities.For spectral studies we extracted PI count histograms for various regions in the emission(Fig.5).We made two background spectra,one using the Markevitch background files and one using a local background extracted from two50-arcsecond-radius circles at either end of node1in our dataset and containing10650counts.The two spectra were similar,and the results presented here use the local background.The galactic extinction in the direction of Arp220has a column of4.1×1020cm−2(Stark et al.1992)and this has been used as a lower limit in our spectralfits.3.X-ray emission from Arp2203.1.Overall morphologyThe Chandra view of Arp220reveals structure on scales from one arcsecond to several arcminutes.We can distinguish four scales of interest:the nuclear region,the galaxy with two regions of extended emission(‘plumes’),the extended20-kpc scale emission(‘lobes’), and the unrelated group of galaxies to the south reported by Heckman et al.(1996).The position angles of the plumes and lobes are in agreement with the PSPC and HRI structures described by Heckman et al.Here we describe the observations,leaving most physical interpretation to later sections.The integrated spectrum from Arp220can befit by the sum of several thermal contributions and a power law,and gives good agreement on the totalflux with the individualfits to components,with1694net counts and a luminosity of1.2×1041erg s−1, in good agreement with the estimates of Heckman et al(1996).The data on individualcomponents are summarized in Table1and discussed below.3.2.The circumnuclear regionIn the nuclear region we see hard emission on a scale of two to three arcseconds,and indications of bright point sources,denoted X-1and X-4in Paper I(Clements et al.2002) close to the nucleus.A soft emission peak,denoted X-3in Paper I,is also present andis extended over a diameter of2.5kpc.Its centroid is displaced1.5arcseconds to the northwest of the hard emission.The hard emission coincides with a dust lane in the galaxy (Joy et al.1986),and indeed the soft emission is suppressed there.However,the absence of hard emission away from the nucleus shows that the spectral change is due to a different type of source,and not merely an absorption effect.In Paper I we presented reconstructed images and spectralfits to the nuclear sources X-1to X-4.3.3.The plumesOn a scale of a few kiloparsecs,we see two regions of bright extended X-ray emission, one on either side of the nucleus,along a position angle of135-150degrees.This emission was seen in the HRI observations reported by Heckman et al.(1996);we will refer to these regions as the NW and SE‘plumes’.We cannot rule out that the emission comes from unresolved point sources,but if the plumes are two unrelated starburst regions we would expect binaries to contribute a hard component to the spectrum.Fig.6shows a contour plot of the reconstructed image of the plume region.The bright region of the NW plume is about3kpc in extent and the SE plume is larger and brighter,3x5kpc in extent;the projected tip-to-tip length of the emission is10 kpc.Each of the plumes appears to be roughly round,but with an elongation in the radialdirection for the SE plume.The emission is not sharp-edged,and the dimensions given here correspond to a contour of10percent of the peak surface brightness.The east plume spectrum is inconsistent with that from a single temperature plasma.It includes a soft thermal contribution with a temperature of less than0.25keV,together with hotter thermal plasma or bremsstrahlung ranging from1to5keV.There are fewer counts in the west plume,but the spectrum definitely containsflux out to2keV.Formally,the data provides only an upper limit to the absorption column in the plumes of1.5×1022cm−2. The difference in inferred intrinsic luminosity(source side of absorption)between assuming only foreground absorption and using this upper limit renders estimates of the unabsorbed luminosity for this soft emission uncertain by a factor of a thousand;the values in Table1 should therefore be considered illustrative.The overall morphology of the plumes could also be affected by patchy absorption in the galaxy,but the visible dust lanes do not correlate with the plume boundaries except in the inner edge of the east plume.Radio observations (Hibbard,Vacca and Yun2000)show the presence of an elongated HI emission feature to the NE and SW of the galaxy on20kpc scales;notably,the HI emission avoids the regions of X-ray emission-there is a gap in the HI which corresponds to the area with the plumes and is aligned with them.However,the measured column of the HI,less than5×1019cm−2 in the region of the plumes,would provide too little absorption to affect the observed soft X-ray morphology.We will assume in the later discussion that the observed morphology corresponds to the actual distribution of soft X-ray emitting gas.3.4.The lobesBeyond the plumes we observe large,lower surface brightness extended oval regions (which we will refer to as the E and W‘lobes’)which lie along a position angle of100-110 degrees.This larger scale emission extends across25kpc from the end of one lobe to thatof the other,and each oval lobe is8kpc along its major axis.The east lobe has a major axis diameter of23arcseconds(8kpc)along PA90degrees,and a minor axis diameter of15arcseconds(5kpc).The west lobe is elongated NE to SW and may consist of two separate components;it is10x22arcseconds in size.We have estimated nominal centers of the east and west lobes at11and8kpc from the nucleus.The smoothed image makes it appear that the lobes are edge brightened,although this is only marginally evident in the raw data and one might worry that it is an artifact of the smoothing process.Extracting counts from raw data in the lobe centers and the lobe rims shows a difference of4sigma,with6total counts in the0.2-2keV range for a pair of5arcsecond diameter circles in the E and W holes(lobe centers)respectively,compared to26total counts in a bright rim region of equal size.We conclude that the lobes are indeed edge-brightened,although an exposure three times as deep would provide afirm confirmation.The lobes show marginal evidence for some very soft photons below0.25keV,but the spectral calibration of ACIS is still unreliable in that energy band.The spectrum is consistent with no absorption in excess of the foreground value from Stark et al.;formally, the bestfits of the east lobe data to a two temperature Raymond-Smith model are with a lower temperature of0.3±0.1keV and a higher temperature of1.0±0.2keV,while the west lobe is slightly softer with values of0.2and0.7keV.There are364total net counts in the lobes.Their total luminosity is1.3×1040erg s−1,a result which is insensitive to the assumed spectralfit parameters(but see below). Wefixed the absorption at the galactic value of4×1020cm−2;we were not able to obtain an acceptablefit with a single Raymond-Smith plasma for either lobe,but the sum of two temperatures was adequate(although of no physical significance with this small number of counts).We note that ACIS-S is not very sensitive to diffuse hard emission.The hard background in our data gives a weak upper limit of about1×1040erg s−1for the2-10keV luminosity in the lobes,comparable to the observed soft luminosity.Therefore,although we have demonstrated the presence of low temperature X-ray gas in the lobes,we cannot rule out the presence of hotter temperature gas.Nevertheless,we see no evidence for the 1×1041erg s−1of emission reported by Iwasawa et al(2001)from BeppoSAX data.This emission was detected in a3arcminute circle and is not inconsistent with our upper limit on this scale,but we can rule out its association with the inner regions of Arp220;possibly they underestimated the contribution from Heckman’s group(see below).The spectra of the lobes and the plumes are compared in Fig.7.3.5.The background clusterFig.8shows a larger scale X-ray image which includes the region of Heckman et al.’s (1996)z=0.09group1RXH J153456.1+232822.The X-ray observations of this object and others in thefield will be discussed in detail in Paper III(McDowell et al.,in preparation). We briefly note here that we confirm the X-ray source as a diffuse object associated with the optical group and detect several embedded point sources.Galaxies Ohyama A and C (Ohyama et al.1999,Grogin&Geller2000),which are are also2MASS sources(2MASS, 1999),are both bright X-ray sources,with Ohyama A showing a soft extended plume,while the third cataloged galaxy,Ohyama B,is not detected.Two further bright point sources CXOU153452.9+232833and CXOU153451.9+232828are present within the cluster but have no counterparts on the POSS2images.4.Correspondence with other wavebands4.1.Optical line emissionWe obtained new integralfield spectroscopy of the Arp220system in Hαand NII as part of a program to study ionized gas in ULIRGs.Arribas,Colina&Clements(2001) presented observations of the nuclear region of the galaxy.The present observations were taken on2000May8and9on the4.2m William Herschel Telescope using INTEGRAL (Arribas et al.1998)and WYFFOS(Bingham et al.1994)and consist of a mosaic of three pointings with a30arcsecondfield-of-viewfiber bundle.As in other star forming galaxies studied by Chandra(e.g.Strickland et al2000),there is a strong correlation of X-ray morphology with optical line emission.Heckman,Armus& Miley(1987)discovered the20kpc‘double-bubble’Hαstructure around Arp220,as well as the inner HαSE plume.The Hαand soft X-ray morphology agree well in overall form and location-faint lobes, stronger plumes and the bright nuclear region-but there are differences in detail.Fig.9 shows contours of Hαemission superimposed on the soft X-ray image.The peak of the Hαemission coincides to within the1”registration error with the soft X-ray peak(X-3).The holes in the lobes agree to within a couple of arcseconds,and the eastern plume is brighter than its western counterparts in both Hαand X-rays.However, the brightest part of the line emission in the western lobe is shifted about8arcseconds south of the western X-ray lobe,and the eastern lobe is much more prominent in X-rays than it is in Hα.The peak of the SE plume is2arcseconds north of the plume’s soft X-ray peak.For a typical electron density of100cm−3and temperature of104K we derive the mass of Hα-emitting gas to be2×106M⊙.The velocity in the plumes derived from theHαobservations(Colina et al2003,in prep.)is about200km/s on average(with gradients up to600km/s in the lobes).Interpreting this as an outflow leads to a kinetic energy of 8×1053erg s−1.4.2.Overall picture of Arp220Arp220is a complex system with tidal tails,dust lanes,and multiple nuclei.About 150clusters and nine satellite galaxies can be seen on a recent HST I-band image(Paper III),reinforcing the impression that the Arp220system is massive compared to the Milky Way.The hard source X-1is clearly associated with the galaxy’s central regions,and is probably coincident with the western nucleus Arp220B(Paper I),although uncertainties in registration mean we cannot rule out an identification with the eastern nucleus.The soft emission and the X-3peak(which also has a soft spectrum)coincide with the emission line peak rather than with the optical continuum peak.As other authors have discussed, the location of the optical peak is likely determined by gaps in the absorption and may not correspond to a physical object.None of the known optical and infrared clusters in this system(Shaya et al.1994,Scoville et al.1998)are detected in X-rays.X-2is in a star cloud just to the south of the western end of the central dust lane;there is a probable cluster at 1.2arcsecond from its estimated location,not close enough to propose as an identification.The optical dust lane coincides with the separation between the nuclear emission and the SE plume,indicating that this separation is probably due to absorption.Interestingly, the plumes’outer boundaries,while not sharp,coincide with a drop in the optical isophotes and plausibly represent the escape of the gas into a less dense halo interstellar medium.The axis of the plumes is perpendicular to the dust lane of Joy et al.(1986)and the CO disk, implying that they may be collimated in the inner region.One might expect the faintness of the NW plume to reflect its orientation deeper into the galaxy,but the X-ray spectrumdoes not allow us to constrain the possibility of larger absorption in the NW.However,a second dust lane visible in the HST data bounds the brightest part of the NW plume on its northern side,implying that there may be more X-ray emission hidden behind it.5.Discussion5.1.The Superwind and the PlumesHeckman et al.(1996)proposed that the extended H-alpha and soft X-ray emission in Arp220originates in a‘superwind’driven by starbursts which have been triggered by the merger.An alternate possibility,to be discussed in more detail by Hearn&Lamb(2003), is that the galaxy collision and merger dynamics are directly responsible for the extended structural morphology and hot gas.We consider each of these possibilities and conclude that both processes may play important roles in the Arp220system.If Arp220is the product of the merger of two gas-rich disk galaxies,as is commonly thought to be the case because of the apparent presence of two,very close galactic nuclei and the overall disturbed morphology,then the physical processes that take place in this collision lead not only to conditions ripe for a central starburst,but also large-scale shocking of the interstellar gas over significant parts of the galactic disks.That is,in such a system,it is expected that a starburst-generated superwind will have to punch through a complicated region that lacks three dimensional symmetry,and consists of sectors of rapidly outflowing and inflowing shock-heated gas,coupled to sectors offlowing neutral gas that did not experience a direct impact.Thus the dominantflow direction of the superwind is likely to be constrained by the evolving geometry of the colliding system.The plumes will not expand into the regions of high pressure and high density,that comprise the hot expanding shocked gas and the cool expanding gas,respectively.The three dimensional morphologyof the overall system is very dependent on the collision parameters,and the time sincefirst impact.Thus the environment of a superwind in a merging system is possibly different to that in a system like M82,that appears to be experiencing a central massive starburst in a previously relatively undisturbed disk galaxy.Strickland and Stevens(2000)have used a combined Eulerian/Lagrangian hydrody-namics code to perform2-D modeling of the superwind in M82,assuming cylindrical and reflection symmetry.As discussed by them,construction of a model to match the observed wind proved to be elusive,and will possibly require the inclusion of processes such asinflow of cold material or magneticfields,to produce the observed confinement at the base of the wind in the starburst region.They conclude from their modeling that the bulk of the outflowing gas is at high temperatures of around107.5K and low density,and would, therefore,be difficult to observe because of low emissivity.Interesting new information on the nature of starburst-driven winds and the interpretation of their observed X-rayfluxes is provided in Strickland et al.(2000).This tends to support the supposition that the temperature of the outflowing gas is not easily determined from X-ray data.Theyfind that high-resolution Chandra observations of the kiloparsec-scale wind in NGC253demonstrate a strong correspondence between the X-ray and H-alpha observations of the outflow cone, with approximately equal amounts of energy being emitted from the hot gas in optical lines and in X-rays,and a total energy in both of the order of1041erg s−1.This is about one percent of the mechanical energy estimated to be injected by the starburst.Strickland et al.(2000)also determined that the bulk of the X-rayflux originates in a limb-brightened structure,with at most20%of theflux coming from the body of thefluid.This provides the first direct evidence that this radiation is generated at the interface between the outflowing gas and the ambient denser medium,rather than in the bulk of theflowing gas,whose temperature is,therefore,not well established.Comparing our Chandra observations of Arp220with those of NGC253,we see some similarities,despite the large difference in scale.As noted previously,the extended X-ray lobes in Arp220extend a distance of10-15kpc from the nucleus on the plane of the sky, and these also appear to be limb-brightened.The observed“edges”show reasonable overlap with the arcs of H-alpha emission in these regions,one each on the east and west sides(see Fig.9).The lobes also display apparent central”holes”in the emission.In fact,the counts in the lobe regions are sufficiently low that our results are consistent with all of this soft X-rayflux originating within edge-brightened structures.However,although both sets of structures(plumes and lobes)appear to be produced by outflowing gas colliding with an external,denser medium,this may be an incorrect model for the lobes of Arp220,because simulations of colliding galaxies indicate that the collision itself may haveflung a dense ring-like structure of gas out on each side of the nucleus.For this system,we suggest that at these vast distances from the nucleus,it is the tidal interaction itself that is propelling the gas outwards;that there is shock heating within,and along the edges of the locally overdense structures,as demonstrated in previous studies of colliding galaxies(see Gerber et al,1996,Lamb et al,1998,and Hearn&Lamb,2001);and that whether the source of the outflow energy is overpressure from a central starburst or tidally channeled galactic gravitational energy,the net effect is a strong correlation between the X-ray emission and H-alpha emission from gas that attains a temperature of around106K in shocks at an interface.The inner two plumes of hot gas observed in Arp220are likely to be due to a superwind that is driven by a central massive starburst,because such a wind would be a natural outcome(although similar features can be produced byflowing shocked regions of gas in slightly off-center galaxy collisions).In thisfirst picture,the central regions have become sufficiently dense that a large fraction of the gas has cooled to form molecular gas and a super starburst has occurred.This latter has then produced a superwind which hasinteracted with,and been somewhat chanelled by the structures formed by the collision itself.The extent of these plumes is large,spanning11kpc across the nuclear region. However,in contrast to the outflow cone in NGC253,the Arp220plumes are very bright in soft X-rays,and no limb-brightening is noticable in our data.The ambient medium into which these plumes are driving may be considerably different to that in NGC253, consisting of entangled regions of shock-heatedflowing gas and cooler,non-shocked gas,as discussed above.The energyflux coming from the central starburst in Arp220is larger than that from NGC253by a factor of70,and this may also play a role in producing the different X-ray properties of the two objects.As noted in Section3.3,the Chandra X-ray data for the Arp220plumes is consistent with a thermal plasma with temperatures ranging from0.25to1keV.This temperature range may result from the interaction of gas ejected in hot stellar winds and SN with regions of collisionally shock-heated gas,and with cooler flowing gas.That is,the entrained material may be of very varied initial temperature.5.2.Merger SimulationsThe overall context within which we wish to discuss our Chandra X-ray data for Arp 220is that of a colliding pair of co-rotating,comparable mass,gas-rich galaxies which have not yet fully merged,but whose nuclei are now very close,and lie within a central disk of material that has been formed from remnants of the original two gaseous disks.Other disk remnants have beenflung to large distances from the joint nuclear region.Relevant numerical modeling(Lamb et al2003)indicates that the collision was likely almost face-on, and had an impact parameter of roughly70%of the optical disk radius.Such a collision will leave some parts of the gas disks,those furthest from the impact point,unshocked by the direct collision,and this material is likely to retain its original temperature,whereas that。
critical observations的意思
critical observations的意思【释义】critical observations关键的观察【短语】Ability to make critical observations做出批判性观察的能力【例句】1In each area I have summarized my view of the critical observations of a few authors who have shaped the theory.在每一个方面,我都将概述一些在我看来对该理论有重大影响的作者所提出的重要观点。
2You are also in a position to make some critical observations as to what you could do to improve your living conditions at home.你也可以审视一下看看有什么可以做的来改善你的生活环境。
3MEREDITH GRIFFITHS:He says long term funding for sustained ocean observations is absolutely critical.梅勒迪斯格里菲斯:他说对持续海洋观测的长期资金支持绝对是至关重要的。
4These critical theoretic observations have many interesting consequences.这些关键的理论观点会带来很多有趣的结果。
5It may include your own empirical and theoretical observations and your own critical thoughts about papers we will discuss in class.它也可包含你自己经验上或理论上的观察、以及你自己对于课堂上所讨论文章的评论思维。
临界反应 英语
临界反应英语全文共6篇示例,供读者参考篇1Title: Critical ReactionHey guys! Today I want to talk to you about something super cool – critical reactions! Have you ever heard of them? Basically, a critical reaction is when something happens that sets off a chain reaction of events. It's like a chain of dominoes falling down, one after the other.Let me give you an example. Imagine you have a piece of uranium. When a neutron hits the uranium, it can split the uranium atom in two, releasing more neutrons. These new neutrons can then hit other uranium atoms, causing them to split as well. This creates a chain reaction, with more and more atoms splitting and releasing energy.This process is called nuclear fission, and it's what powers things like nuclear reactors and atomic bombs. But here's the thing – fission reactions need to be controlled. If too many atoms split at once, it can create a huge explosion, like in a nuclear bomb. This is called a critical reaction.Scientists have to carefully control fission reactions in nuclear reactors to make sure they don't get out of hand. They use things like control rods to absorb excess neutrons and stop the chain reaction from speeding up too much.So, next time you hear about critical reactions, remember that it's all about controlling the energy released by splitting atoms. It's like a super cool science experiment, but withreal-world implications. Pretty awesome, right? Let me know if you have any questions about critical reactions – I'd love to chat more about it with you!篇2Title: The Critical ReactionHey guys! Today I'm gonna tell you all about this really cool thing called critical reaction. It's like when things get super intense and reach a tipping point, you know? Let's dive right in!So, imagine you have a bunch of chemicals in a test tube. They're just chilling there, minding their own business. But then, you add a little extra something-something, like heat or a catalyst, and bam! Those chemicals start reacting like crazy. This is what we call a critical reaction.It's like the chemicals are having a party in that test tube, dancing and bouncing around. And when they reach a certain point, the reaction goes into overdrive. It's like they can't stop themselves!But here's the thing - critical reactions can be a bit dangerous. If you're not careful, things can get out of control real quick. That's why scientists always wear safety goggles and gloves when they're working with chemicals. Safety first, guys!But critical reactions aren't just for scientists. They can happen in all sorts of situations. Like when you and your friends are having a heated debate about which is better, pizza or ice cream. Things can escalate pretty quickly, right?So next time you see a critical reaction happening, remember to stay safe and keep a cool head. And who knows, maybe you'll discover something amazing in the process! Stay curious, my friends.篇3Once upon a time, there was a super important scientific thing called nuclear fission. It's like when a big atom breaks into smaller atoms and releases a bunch of energy. This is what happens in a nuclear power plant to make electricity.But sometimes, things can get a little crazy. If the atoms are breaking too fast and releasing too much energy, it's called a critical reaction. It's like when you're playing with a toy and it's going so fast that it starts to overheat and smoke. That's not good!In a nuclear reactor, if there's a critical reaction, it can be dangerous. The heat and energy can get out of control, and that's called a meltdown. Just like when your ice cream cone melts in the sun, except way scarier!That's why scientists and engineers have to be super careful when they're working with nuclear reactors. They have to make sure everything is just right so that there's no critical reaction. They use special controls and safety measures to keep everything under control.So remember, nuclear fission is cool and all, but we have to be really careful with it. We don't want anything to go boom!篇4Title: The Critical ReactionHey guys, today I want to talk to you about something super cool and important called the critical reaction. Have you everheard of it before? Well, don't worry if you haven't because I'm here to explain it to you!So, the critical reaction is basically a super important process in science where things change really quickly and can even create a big explosion! It happens when a certain amount of stuff, like chemicals or atoms, come together and react in a big way. It's kind of like when you mix vinegar and baking soda and it fizzes up everywhere!But the thing about the critical reaction is that it can be really dangerous if it's not controlled properly. That's why scientists have to be really careful when they're working with things that could cause a critical reaction. They have to follow all the rules and wear special gear to keep themselves safe.One famous example of a critical reaction is when atomic bombs were dropped on Japan during World War II. The reaction was so powerful that it caused immense destruction and loss of life. That's why it's super important for us to understand the critical reaction and be careful with it.So, remember guys, the critical reaction is a really cool but also really serious thing. Make sure to always be safe and follow the rules when you're doing any experiments or science projects. Stay curious and keep learning! Bye for now!篇5Title: The Exciting Adventure of Critical Reaction!Once upon a time, I learned about something super cool called a critical reaction in science class. It's like when a bunch of atoms get super excited and start bouncing around like crazy. It's kind of like when my little brother has too much sugar and can't sit still!So, the other day in class, my teacher showed us this experiment where she mixed two liquids together and BAM! they started fizzing and bubbling like a volcano! It was so awesome!She explained that in a critical reaction, the atoms in the liquids get so hyped up that they start smashing into each other and creating new substances. It's like a big party inside the beaker!I asked my teacher why critical reactions happen, and she said it's because the atoms in the liquids don't like being alone. They want to be with their friends, so they get all jittery and jump around until they find a buddy to hang out with. It's like a big game of tag, but with atoms!I also learned that critical reactions can be dangerous if you're not careful. My teacher told us to always wear safety goggles and follow the instructions carefully. Safety first, always!I can't wait to do more experiments with critical reactions. It's like being a scientist in a super cool lab, mixing things together and watching the magic happen. Who knew science could be so fun?篇6Title: The Critical ReactionHey guys, today I want to talk about something super cool and important - it's called a critical reaction! It's like when you mix two things together and they make a big BOOM! But don't worry, it's all safe and controlled in science labs.So, a critical reaction is when you have just the right amount of stuff mixed together to make a big reaction happen. If you have too little or too much of something, then nothing cool will happen. It's all about finding that perfect balance.One example of a critical reaction is in nuclear power plants. They use uranium to make energy, but if you have too much uranium in one place, it can be really dangerous. So scientistsmake sure to keep everything in just the right amounts to keep things safe and working properly.Another example is in chemistry labs when you mix chemicals together. If you have just the right amount of each chemical, then they can react and make new substances. It's like magic happening right before your eyes!So, remember, a critical reaction is all about finding that perfect balance. Too little or too much of something won't work, but just the right amount can create some amazing reactions. Keep exploring and experimenting, and who knows what cool things you might discover!。
反常评价法作文
反常评价法作文Hello there! Let's embark on a journey of exploration through the lens of the Unusual Evaluation Method in our essay. This unconventional approach to writing will guide us in delving into topics in a fresh and exciting manner.你好!让我们通过反常评价法作文的镜头,踏上一段探索之旅吧。
这种非传统的写作方式将引导我们以新颖和激动人心的方式深入探究各种话题。
Firstly, let's consider the topic of technology. In a world where smartphones and social media have become integral parts of our lives, it's easy to fall into the trap of praising their benefits. But let's flip the script. Instead of focusing on the positives, let's highlight the downsides.首先,我们考虑技术这个话题。
在一个智能手机和社交媒体已成为我们生活不可或缺部分的世界里,很容易陷入赞美其好处的陷阱。
但让我们反其道而行之。
与其专注于积极方面,不如强调其缺点。
For instance, the excessive use of smartphones has led to a rise in neck pain and eye strain. Social media, while connecting us with friends and family, has also given rise to issues like cyberbullying and the constant need for validation. By adopting an unusual evaluation method, we can bring these often-ignored aspects to the forefront.例如,智能手机的过度使用导致颈部疼痛和眼睛疲劳的问题日益严重。
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3 Depaade Federal de Alagoas, 57072-970 Macei´o–AL, Brazil (February 1, 2008)
arXiv:cond-mat/0007094v3 [cond-mat.stat-mech] 10 Aug 2000
Universidade Federal do Rio Grande do Norte, 59078-970 Natal–RN, Brazil 2Departamento de Matem´atica, Universidade Federal do Rio Grande do Norte, 59078-970 Natal–RN, Brazil
due to termination of polymerization at all active growth sites. Along the critical line b = bc(c), the polymer is fractal (Fig. 1(a)) and has a diverging correlation length.
We investigate this problem by using simulations of the BPGM [10]. BPGM is a generalization of KGW [11] which is able to capture the essential dynamics of branched polymerization. We briefly describe the model here (Fig. 1(b)). The BP is generated from an initiating seed at time t = 0 located at the center of a d-dimensional lattice. At time step t = 1, one of the vacant nearestneighbor sites of the seed is chosen randomly and occupied to become the next active growth tip, and the seed ceases to be an active growth tip. At each step t of the growth process, a branching also can occur at every such growth tip, by occupation of an additional (second) site with probability b. A fraction c of randomly chosen sites is not available for growth. Hence, at time t+1, the poly-
We find that 2-dimensional (2-D) critical branched polymers with no impurities conclusively belong to the same universality class as 2-D random percolation clusters, although pure critical 3-D branched polymers do not belong to the 3-D percolation universality class. We find, moreover, that the fractal dimension df of critical branched polymers is independent of the presence of a random environment in 2D, but not in 3-D. We also report that when there are no impurities the critical branching probability in 3-D is bc = 3.34 × 10−4 ± 0.16 × 10−4.
The commonly held belief that BP belong to the lattice animals [14] universality class was based on the assumption that there is no random environment (c = 0) and that there are only repulsive forces between chains [15]. It was thus a remarkable finding when Bunde et al. [1] showed, using the branched polymer growth model (BPGM), that critical BP in random environments in 2-D belong to the same universality class as 2-D random percolation clusters. One conceivable explanation for this interesting result is that in 2-D such behavior is induced by the random impurity obstacles that, indeed, form real percolation clusters with site occupation probability p = c. Hence, it can be argued that the polymer grows as if constrained by the random obstacles, and this effect can generate an effective attraction between chains (Fig. 1(b)). For the special case c = 0, however, there are no such impurities, hence this physical argument becomes irrelevant. The study by Bunde et al. [1] is conclusive all along the critical line b = bc(c) for c = 0, but the important special case of pure BP (c = 0) still remains unconfirmed [1], and both the percolation as well as the lattice animals universality classes remain plausible. An additional controversy surrounding the special case c = 0 arises because in many systems [15] the introduction of disorder is sufficient to modify the universality class (and sometimes even to destroy the ordered phase). The Harris criterion [15] predicts that the critical BP in 2-D is a candidate for experiencing a change of universality class when going from c = 0 to c = 0.
The Strange Behavior of Critical Branched Polymers
H. H. Arag˜ao-Rˆego1, J. E. de Freitas1,2, Liacir S. Lucena1, G. M. Viswanathan1,3 1 International Center for Complex Systems and Departamento de F´ısica Te´orica e Experimental,
Polymerization has been an important topic of recent interest in the physics community [1–4]. Polymers are extensively studied [5–7] complex systems, and can be either linear or branched [1,8–10]. In spite of being simpler, linear polymers (LP) present physical features such as non-Markovian growth and nontrivial scaling. For several decades it has been known that linear polymers in diluted solutions can be successfully modeled using selfavoiding walks (SAW). More recently it was found that large SAW chains can be more easily constructed by kinetic growth walks (KGW) [11] that belong to the same universality class as SAW chains [12]. Branched polymers (BP) have a larger degree of complexity and exhibit an astonishingly rich phenomenology [1,2,4,6,7,10,13–15]. In the 1990’s, the KGW approach was generalized to describe the growth of BP in disordered media [1,10,16]. Such BP are typically grown when polymerization occurs in a solution with two types of units: (i) monomers with two chemically active molecular sites (“tips”) that lead to linear polymerization and (ii) three-tipped mononers that lead to branchings (i.e., bifurcations). Many important physical properties of the resulting BP depend on the probability b for branching to occur and the concentration c of impurities [13] that can block or slow the polymerization.