THE EVOLUTION OF THE PHASE SPACE DENSITY OF PARTICLE BEAMS IN EXTERNAL FIELDS
空间发展顺序的英语作文
空间发展顺序的英语作文The Progression of Space ExplorationThe exploration of space has been a captivating and awe-inspiring journey for humanity since the dawn of the Space Age. From the first successful launch of a satellite to the ambitious plans for interplanetary travel and beyond, the progression of space development has been a testament to the human spirit of curiosity and the relentless pursuit of knowledge. This essay will delve into the historical milestones, current advancements, and the future prospects of space exploration.The Space Age began in 1957 with the launch of the Soviet Union's Sputnik 1, the first artificial satellite to orbit the Earth. This groundbreaking event sparked a fierce competition between the United States and the Soviet Union, known as the Space Race, which drove rapid advancements in rocketry, satellite technology, and human spaceflight. The launch of the first human into space, Yuri Gagarin, in 1961 and the subsequent Apollo program's successful moon landings in the late 1960s and early 1970s marked the pinnacle of this era of space exploration.Following the Apollo program, the focus shifted towards the development of reusable launch vehicles and the establishment of permanent human presence in space. The launch of the Space Shuttle program in 1981 and the construction of the International Space Station (ISS) in the late 1990s and early 2000s were significant milestones in this phase of space development. The ISS has served as a crucial platform for scientific research, technological advancements, and the exploration of the effects of long-term human habitation in space.Concurrent with the advancements in human spaceflight, the exploration of our Solar System has also progressed significantly. Robotic probes and landers have been sent to study the planets, moons, and other celestial bodies, providing unprecedented insights into the formation and evolution of our cosmic neighborhood. The Voyager program, which launched two spacecraft in the 1970s, has been a remarkable success, with the Voyager 1 spacecraft now the farthest human-made object from Earth, having crossed the boundary of the heliosphere and entered interstellar space.In recent years, the private sector has also become increasingly involved in space exploration, with companies like SpaceX, Blue Origin, and Virgin Galactic leading the charge in developing reusable launch systems, space tourism, and even plans for establishing a human presence on Mars. These private-public partnerships have thepotential to significantly accelerate the pace of space exploration and make it more accessible to a wider range of individuals and organizations.Looking towards the future, the progression of space exploration is poised to reach new heights. The development of advanced propulsion systems, such as nuclear thermal rockets and ion engines, could enable faster and more efficient interplanetary travel. The establishment of permanent human settlements on the Moon and Mars is also a primary focus of many space agencies and private companies, with plans for lunar bases and Martian colonies in the coming decades.Furthermore, the search for extraterrestrial life has been a driving force behind many of the recent and planned missions to explore the Solar System and beyond. The discovery of potentially habitable exoplanets and the continued exploration of our own planetary system have heightened the anticipation for the detection of signs of life beyond Earth, which would have profound implications for our understanding of the universe and our place within it.In conclusion, the progression of space exploration has been a remarkable journey, marked by groundbreaking achievements, technological advancements, and the boundless curiosity of humanity. From the humble beginnings of the Space Age to theambitious plans for interplanetary colonization and the search for extraterrestrial life, the future of space exploration holds immense potential for scientific discovery, technological innovation, and the expansion of our understanding of the cosmos. As we continue to push the boundaries of what is possible, the progression of space exploration will undoubtedly continue to captivate and inspire generations to come.。
科学精神耀四方的英语作文
The spirit of science is a beacon that illuminates the path of human progress and development.It is a set of values and attitudes that emphasizes critical thinking, evidencebased reasoning,and an openminded approach to understanding the world around us.Here is an essay that delves into the essence of scientific spirit and its impact on various aspects of society.Title:The Radiance of the Scientific SpiritIn the vast expanse of human history,the scientific spirit has emerged as a guiding light, illuminating the path to knowledge and innovation.It is a multifaceted concept that encompasses curiosity,skepticism,and a relentless pursuit of truth.The scientific spirit is not confined to laboratories or academic institutions it is a universal principle that can be applied to every facet of life.Curiosity:The Driving ForceAt the heart of the scientific spirit lies an insatiable curiosity,a desire to explore the unknown and to question the status quo.This innate human trait has led to countless discoveries and advancements,from the laws of physics to the intricacies of the human genome.Curiosity propels us to venture beyond our comfort zones,to challenge preconceived notions,and to seek answers to the most complex questions.Skepticism:The Critical EyeSkepticism is the scientific spirits critical eye,ensuring that every claim is scrutinized and every hypothesis tested.It is the discipline that demands evidence and resists the allure of unfounded beliefs or superstitions.Skepticism is not about dismissing ideas outright rather,it is about subjecting them to rigorous examination and validation. EvidenceBased Reasoning:The FoundationThe scientific method,with its emphasis on evidencebased reasoning,is the cornerstone of the scientific spirit.It is a systematic approach to understanding the natural world, involving observation,hypothesis formulation,experimentation,and analysis.This method ensures that conclusions are not based on personal biases or subjective interpretations but on verifiable and replicable data.OpenMindedness:The Path to InnovationOpenmindedness is the willingness to consider new ideas and perspectives,even thosethat may initially seem counterintuitive or controversial.It is this quality that fosters innovation and creativity,allowing scientists to think outside the box and to develop novel solutions to pressing problems.Openmindedness is the antithesis of dogmatism and is essential for the evolution of scientific thought.Impact on SocietyThe influence of the scientific spirit extends far beyond the realm of science itself.It has shaped our understanding of ethics,politics,and social issues.For instance, evidencebased policymaking is a direct application of the scientific method to governance,ensuring that decisions are informed by data rather than by ideology or conjecture.ConclusionThe scientific spirit is a beacon that shines brightly in the darkness of ignorance,guiding humanity towards a future of enlightenment and progress.It is a testament to our collective desire to understand the world and to improve the human condition.By nurturing and promoting the scientific spirit,we can ensure that the light of knowledge continues to illuminate the path forward for generations to come.。
高考英语阅读理解态度题单选题30题
高考英语阅读理解态度题单选题30题1. The author's attitude towards the new law can be described as _____.A. supportiveB. indifferentC. criticalD. ambiguous答案:C。
本题考查作者对新法律的态度。
选项A“supportive”意为支持的,若选此选项则表明作者对新法律持积极肯定态度,但文中作者列举了新法律的诸多弊端,并非支持。
选项B“indifferent”意为漠不关心的,而文中作者有明确的观点和评价,并非漠不关心。
选项C“critical”意为批评的,符合文中作者通过列举问题对新法律进行批判的态度。
选项D“ambiguous”意为模糊不清的,文中作者态度明确,并非模糊不清。
2. What is the attitude of the writer towards the proposed solution?A. OptimisticB. PessimisticC. DoubtfulD. Confident答案:C。
此题考查作者对所提出的解决方案的态度。
选项A“Optimistic”表示乐观的,若选此选项意味着作者认为该解决方案可行且效果良好,但文中作者对其可行性提出了质疑。
选项B“Pessimistic”表示悲观的,然而文中作者并非完全否定该方案,只是存在怀疑。
选项C“Doubtful”意为怀疑的,符合文中作者对方案的态度,作者在文中指出了方案可能存在的问题和不确定性。
选项D“Confident”表示自信的,与文中作者的态度不符。
3. The tone of the passage when referring to the recent development is _____.A. excitedB. cautiousC. enthusiasticD. worried答案:B。
好奇探秘星深处的英语作文
Curiosity has always been a driving force for human exploration and discovery.As we peer into the vast expanse of the cosmos,our innate desire to understand the universe and its mysteries propels us forward.The English essay on Exploring the Depths of the Stars could delve into several aspects of this pursuit.The Wonder of the CosmosThe universe is a boundless canvas of celestial bodies,each with its own unique story. Stars,galaxies,and nebulae are just a few of the celestial wonders that capture our imagination.The essay could start by describing the aweinspiring beauty of the night sky and the allure of the unknown that it represents.The History of Space ExplorationA historical perspective on how humanity has ventured into space could be an integral part of the essay.From the first telescopes to the Apollo missions and the International Space Station,the journey has been one of both technological advancement and human courage.The Role of TechnologyThe essay could explore the role of technology in our quest to understand the cosmos. Telescopes,space probes,and satellites have allowed us to peer further into space than ever before.The development of these technologies and their impact on our understanding of the universe would be a key discussion point.The Search for Extraterrestrial LifeThe possibility of life beyond Earth is a captivating subject.The essay could discuss the various missions and projects aimed at finding signs of life,such as the search for exoplanets and the study of extremophiles on our own planet.The Future of Space ExplorationLooking ahead,the essay could speculate on the future of space exploration.This could include plans for manned missions to Mars,the potential for space tourism,and the ongoing search for answers to fundamental questions about the universe.The Impact on SocietyFinally,the essay could reflect on how the exploration of space has influenced society.It could discuss the inspiration it provides,the technological spinoffs that benefit everyday life,and the philosophical implications of our place in the universe.ConclusionThe conclusion of the essay could emphasize the importance of maintaining our curiosity and continuing to explore the depths of the stars.It could call for a collective effort to push the boundaries of our knowledge and to inspire future generations to keep reaching for the stars.By weaving these elements together,the essay would not only inform but also inspire readers to appreciate the ongoing journey of space exploration and the endless possibilities it holds.。
新东方英语四级作文翻译
新东方英语四级作文翻译英文回答:The ceaseless evolution of technology has profoundly reshaped our lives, creating unprecedented opportunities and challenges. Amidst this technological revolution, the realm of language and communication has undergone a paradigm shift, giving rise to a new era of digital discourse.From the humble beginnings of instant messaging platforms to the advent of social media and virtual reality, technology has transformed the ways in which we interact with others. The days of face-to-face conversations and handwritten letters have given way to a world dominated by digital exchanges and virtual connections.This technological metamorphosis has had a profound impact on the way we use and perceive language. The speed and immediacy of digital communication have led to theemergence of a more concise and informal style of writing. Acronyms, abbreviations, and emojis have become ubiquitous in our online interactions, reflecting the desire for efficiency and brevity.Moreover, the rise of social media has created a platform for individuals to express themselves and share their ideas with a global audience. This has led to a democratization of discourse, empowering voices that were once marginalized. However, it has also brought to the fore the challenges of misinformation and echo chambers, where individuals are increasingly exposed to opinions that reinforce their own beliefs.中文回答:科技的不断发展深刻地改变了我们的生活,带来了前所未有的机遇和挑战。
Exploring the Boundaries of Space
Exploring the Boundaries of Space Exploring the boundaries of space is an endeavor that has captivated the human imagination for centuries. The idea of venturing beyond our own planet and into the vast expanse of the universe has inspired countless scientific discoveries, technological advancements, and works of art and literature. However, the exploration of space also presents a myriad of challenges and ethical considerations that must be carefully navigated. From a scientific perspective, the exploration of space holds immense potential for expanding our understanding of the universe and our place within it. Through endeavors such as the Hubble Space Telescope and the Mars rover missions, scientists have been able to gather valuable data about distant galaxies, planetary bodies, and the conditions of outer space. This information has not only deepened our knowledge of astrophysics and cosmology but has also contributed to practical applications such as satellite technology and space travel. On the other hand, the exploration of space also raises ethical and philosophical questions about the impact of human activities beyond Earth. As we venture further into space, we must consider the potential consequences of our presence on other celestial bodies and the delicate ecosystems they may harbor. Additionally, the prospect of encountering extraterrestrial life forms raises complex ethical dilemmas about our responsibilities as stewards of the universe and the potential implications of contact with other intelligent beings. Furthermore, the exploration of space is also deeply intertwined with political and economic considerations. Space agencies and private companies around the world are engaged in a race to develop the technology and infrastructure necessary for space exploration, driven by a combination of national pride, scientific ambition, and commercial interests. This competition has led to collaborations and rivalries between nations, as well as debates about the allocation of resources and the prioritization of space exploration in relation to other pressing global issues. From a cultural and artistic perspective, the exploration of space has inspired countless works of literature, film, and visual art that reflect humanity's fascination with the unknown. Whether through the imaginative worlds of science fiction or the awe-inspiring images captured by space probes and telescopes, the exploration of space has sparked the creativeimagination and encouraged contemplation of the profound mysteries of the cosmos. On a personal level, the exploration of space evokes a sense of wonder and curiosity about the possibilities that lie beyond our own planet. The idea of venturing into the unknown and experiencing the beauty and grandeur of the universe firsthand is a source of inspiration and motivation for many individuals, driving them to pursue careers in science, engineering, and space exploration. In conclusion, the exploration of space encompasses a wide range of scientific, ethical, political, and cultural considerations that reflect the complexity of human endeavors beyond Earth. As we continue to push the boundaries of space exploration, it is essential to approach these challenges with a thoughtful and holistic perspective that takes into account the potential benefits and risks of our actions. Ultimately, the exploration of space offers a profound opportunity to expand our knowledge, inspire our imagination, and cultivate a deeper appreciation for the interconnectedness of all life within the cosmos.。
The Future of Space Exploration A New Frontier
The Future of Space Exploration A NewFrontierThe future of space exploration is a topic that has captured the imagination of humanity for decades. From the early days of the space race to the recent advancements in technology, the possibilities for exploring the cosmos seem boundless. However, as we look to the future, there are a multitude of factors to consider, including the potential benefits and challenges of space exploration, the ethical implications of venturing into the unknown, and the role of international collaboration in shaping the future of space exploration. One of the most compelling arguments in favor of continued space exploration is the potential for scientific discovery. The universe is a vast and mysterious place, and there is still so much that we have yet to learn about it. By venturing into space, we have the opportunity to expand our understanding of the cosmos, from studying distant planets and stars to gaining insights into the origins of the universe itself. These discoveries have the potential to revolutionize our understanding of the world around us and drive technological advancements that could benefit humanity as a whole. In addition to the scientific benefits, space exploration also holds the promise of economic opportunities. As technology continues to advance, the potential for commercial ventures in space is becoming increasingly feasible. From asteroid mining to space tourism, there are a multitude of ways in which the private sector could capitalize on the resources and opportunities that space has to offer. This could not only drive economic growth but also create new industries and job opportunities for people here on Earth. However, the future of space exploration is not without its challenges. One of the most pressing issues is the environmental impact of space travel. The rockets and spacecraft used to explore space produce a significant amount of pollution, and as we look to expand our presence in space, these emissions are only expected to increase. Finding sustainable and environmentally friendly ways to travel to and from space will be crucial in ensuring that our exploration of the cosmos does not come at the expense of our own planet. Another consideration is the ethical implications of space exploration. As we venture into the unknown,we may encounter new forms of life or come across resources that are of great value. It will be important for us to approach these discoveries with a sense of responsibility and respect, ensuring that we do not exploit or harm other life forms for our own gain. Additionally, we must consider the impact that our presence in space may have on other celestial bodies, such as the potential for contaminating other planets with Earth-based microorganisms. Furthermore, the future of space exploration will undoubtedly be shaped by international collaboration. The challenges and costs associated with space exploration are immense, and no single country can tackle them alone. By working together, nations can pool their resources and expertise to achieve common goals, whether it be establishing a permanent human presence on another planet or conducting large-scale scientific experiments in space. International collaboration will also be crucial in establishing guidelines and regulations for space exploration, ensuring that it is conducted in a safe and responsible manner. In conclusion, the future of space exploration holds great promise, from the potential for scientific discovery to economic opportunities and technological advancements. However, it is important for us to approach this new frontier with a sense of responsibility and mindfulness, considering the ethical implications and environmental impact of our actions. By working together on an international scale, we can ensure that the future of space exploration is one that benefits all of humanity and respects the vast and wondrous cosmos that we are so eager to explore.。
後科学时代的宇宙和生命新思维
後科學時代的宇宙和生命新思維李政道吳健雄Segre Serber WickWilhelm Conrad Roentgen (1845-1923)Discoverer of the X-rayThe hand of Mrs. Wilhelm Roentgen: the first X-ray image, 1895Murray Gell-Mann1969 Nobel Prize winner, he coined the name of "quark”後科學時代的宇宙和生命新思維科學分殊的危機認知的局限物質科學粒子物理More Unified Theories •For years, physicists have sought for and found unified theories.•1861-1865•James Maxwell, in a series of pages, described theinterrelation of electric and magnetic fields therebyunifying them into electromagnetism. This led to thenow-famous Maxwell's Equations.•1881-1884•Hertz demonstrated radio waves and established that radio waves and light are electromagnetic waves ofdifferent frequencies, as predicted by Maxwell.Heinrich Rudolf Hertz James Clerk Maxwell1967-1970Glashow, Salam, and Weinberg proposed a theory that unifieselectromagnetic and weak interactions.They predicted the mass of the W boson which mediates weak processessuch as beta decay and predicted a new type of weak interaction and itsmediating particle the Z boson. Higgs Boson.1979The Nobel Prize was awarded to Glashow, Salam, and Weinberg for their role in the development of the electroweak theory, four years before the discovery of the W and Z bosons!1983The W and Z bosons were finally discovered in 1983 by the UA-1 and UA-2 experiments at CERN.基本粒子物理電磁理論(James Maxwell)+弱作用理論電弱理論+強作用理論標準模型(Standard Model)+重力作用統一場論Grand Unified TheoryOne of the biggest goals in physics today isto unify the strong, weak, electromagnetic,and gravitational forces into one unified force,or what physicists call the "Grand Unified Theory".It has already been discovered thatat high enough energies, electromagnetismand the weak force are the same force,known as the electroweak force.It is theorized that if energies are increased even further, all the known forces will boil down into the same force. If the standard model can be simplified in this way,it may lead into areas of further study in orderto get a better grasp of the world around us.粒子物理電磁理論(James Maxwell)+弱作用理論電弱理論+強作用理論標準模型(Standard Model)+重力作用統一場論誰是Edward Witten?Many physicists consider Ed Witten tobe Einstein's true successor.什麼是弦理論?What is string theory?Witten:String theory is an attempt at a deeper description of nature by thinking of an elementary particle not as a little point but as a little loop of vibrating string.One of the basic things about a string is that it can vibrate in many different shapes or forms, which gives music its beauty. If we listen to a tuning fork, it sounds harsh to the human ear. And that's because you hear a pure tone rather than the higher overtones that you get from a piano or violin that give music its richness and beauty.•So in the case of one of these strings it can oscillate in many different forms --analogously to the overtones of a piano string. And those different forms of vibration are interpreted as different elementary particles: quarks,electrons, photons. All are different forms of vibration of the same basicstring. Unity of the different forces and particles is achieved because they all come from different kinds of vibrations of the same basic string. In the case of string theory, with our present understanding, there would be nothingmore basic than the string.EssayNature 438, 1085 (22 December 2005)|ConceptUnravelling string theoryEdward Witten1•(Last two paragraphs)•But what is string theory? It may well be the only way to reconcile gravity and quantum mechanics, but what is the core idea behind it?Einstein understood the central concepts of general relativity years before he developed the detailed equations. By contrast, stringtheory has been discovered in bits and pieces —over a period that has stretched for nearly four decades —without anyone reallyunderstanding what is behind it. As a result, every bit that isunearthed comes as a surprise. We still don't know where all these ideas are coming from —or heading to.•One day we may understand what string theory really is. But even if we do, and the theory is on the right track, will we be able to learn how it works in nature? I certainly hope so. Realistically, it alldepends on many unknowns, including the nature of the answer, how clever we will be, and the clues we can get from experiment.Superstring Theory WorldNature 440, 1132-1136 (27 April 2006) | doi:10.1038/nature04804Is our Universe natural?Sean M. Carroll11.Enrico Fermi Institute, Department of Physics and Kavli Institute for Cosmological Physics, Universityof Chicago, 5640 South Ellis Avenue, Chicago, Illinois 60637, USA.Email:carroll@AbstractIt goes without saying that we are stuck with the Universe we have. Nevertheless, we would like to go beyond simply describing our observed Universe, and try to understand why it is that way rather than some other way. When considering both the state in which we find our current Universe, and the laws of physics it obeys, we discover features that seem remarkably unnatural to us. Physicists and cosmologists have been exploring increasingly ambitious ideas in an attempt to explain how surprising aspects of our Universe can arise from simple dynamical principles.A natural state for a Universe with a positive vacuum energy is empty de Sitter space; this is the background universe in the figure, with time running vertically. In the presence of an appropriate scalar field, quantum fluctuations in such a background can lead to the nucleation of baby universes. Each baby universe is created in a proto-inflationary state, which then expands and reheats into a universe like that we observe. These universes are portrayed as evolving 'sideways', to emphasize that the local direction of time may not be related to that of thebackground space-time.Chen Ning Yang Albert Einstein Professor Emeritus Nobel Laureate in Physics Yang-Mills TheoryMy PhysicsString Theory Their MathematicsMurray Gell-Mann1969 Nobel Prize winner, he coined the name of "quark”Stephen William HawkingJohn HorganThe Author of The End of Science迎接一個後科學時代的宇宙新思維江才健科學是不是絕對客觀或合理,並不影響其成就一個強勢的創造文化,而它的巨大的致用效果,也並不截然來自它更接近了真理……•科學發展走到今天這個局面,呈現出兩種不同的面象:一方面是繁複抽象、精準嚴謹,另一方面則是深奧難喻、疏離冷僻。
想要了解的事物英语作文
想要了解的事物英语作文Things I Yearn to Understand The world is an intricate tapestry woven with threads of knowledge, both known and unknown. While I find myself fascinated by the vast amount of information we’ve accumulated as a species, I am acutely aware of the vast, uncharted territories of understanding that lie before me. There are several key areas that spark a deep curiosity within me, areas I yearn to explore and grasp with greater clarity. Firstly, I am captivated by the complex workings of the human mind. The brain, a three-pound universe contained within our skulls, is a marvel of intricate networks and electrochemical signals that give rise to consciousness, emotion, and behavior. How do neurons fire in symphony to create our perceptions of the world? What are the mechanisms behind memory formation and retrieval? How does our unique blend of genetics and environment shape our personalities and predispositions? Unraveling the mysteries of the mind holds the key to understanding the very essence of what makes us human. The vast universe, with its swirling galaxies, enigmatic black holes, and the tantalizing possibility of life beyond Earth, also ignites my imagination. I long to understand the fundamental laws that govern the cosmos, from the delicate dance of subatomic particles to the majestic movements of celestial bodies. What is the true natureof dark matter and dark energy, the unseen forces shaping the universe's evolution? Are we alone in this vast cosmic expanse, or does life, in all its wondrous forms, exist elsewhere? The pursuit of answers to these questions is a quest to understand our place in the grand scheme of existence. Closer to home, the interconnected web of life on our planet fascinates me. The intricate ecosystems teeming with biodiversity, the delicate balance of predator and prey, theintricate cycles of energy and nutrients - these are all testament to the awe-inspiring power of evolution and adaptation. I yearn to understand the complex interactions within these ecosystems, the delicate balance that sustains them, and the impact of human activities on this delicate web. Understanding these complexities is crucial for our responsible stewardship of the planet and the preservation of its irreplaceable biodiversity. Furthermore, I am drawn to the intricacies of human history and its impact on our present reality. From the rise and fall of civilizations to the struggles for freedom and equality, historyoffers a lens through which we can examine the triumphs and failures of humankind.I crave a deeper understanding of the forces that have shaped our social,political, and economic systems, the ideologies that have fueled conflicts and cooperation, and the enduring legacies of past events. By studying history, wecan learn from our ancestors' mistakes and successes, equipping ourselves to navigate the challenges of the present and build a better future. The ever-evolving world of technology, with its rapid advancements in artificial intelligence, biotechnology, and space exploration, also holds a powerful allure.I am driven to understand the principles behind these innovations, their potential to address global challenges, and the ethical implications that accompany them. How can we harness the power of artificial intelligence for the betterment of society while mitigating potential risks? What are the ethical considerations surrounding genetic engineering and its impact on future generations? How can space exploration contribute to scientific advancements and inspire future generations? Exploring these frontiers of technology is essential for shaping a future where innovation serves humanity and the planet. Finally, I yearn to understand the very essence of creativity and its power to inspire, challenge, and transform. From the evocative brushstrokes of a painter to the soaring melodiesof a composer, creativity speaks a universal language that transcends cultural boundaries. What are the cognitive processes that underpin artistic expression? How does creativity foster innovation and problem-solving across disciplines? How can we nurture and cultivate our own creative potential to contribute to the world in meaningful ways? Understanding the nature of creativity is key to unlockingour own potential and enriching the human experience. In conclusion, the pursuit of knowledge is a lifelong journey, an insatiable thirst for understanding that fuels my curiosity and motivates my exploration. From the inner workings of the human mind to the vast expanses of the cosmos, from the intricate web of life on Earth to the enduring legacies of human history, from the frontiers of technology to the power of creative expression - these are the areas I yearn to understand with greater depth and clarity. This quest for knowledge is not merely an academic pursuit but a fundamental aspect of what makes us human - the desire to learn, grow, and contribute to the betterment of ourselves and the world around us.。
探索太空的发展史英语作文
探索太空的发展史英语作文The exploration of space has always been a fascinating and thrilling endeavor for humanity. From the early days of space travel to the modern era of space tourism, the development of space exploration has been a remarkable journey.The first successful human spaceflight was achieved by the Soviet Union in 1961, when Yuri Gagarin orbited the Earth aboard the Vostok 1 spacecraft. This historic event marked the beginning of human space exploration andinspired a new era of innovation and discovery.Over the years, space agencies such as NASA and Roscosmos have made significant advancements in space technology, leading to the development of space stations, satellites, and robotic spacecraft. These achievements have expanded our understanding of the universe and paved the way for future space missions.In recent years, the rise of commercial space companies like SpaceX and Blue Origin has revolutionized the space industry. These companies have made significant strides in developing reusable rocket technology and have set ambitious goals for space tourism and colonization.The future of space exploration holds great promise, with plans for manned missions to Mars and beyond. The ongoing development of advanced propulsion systems, life support technologies, and habitat designs will play a crucial role in making these missions a reality.As we look ahead to the next chapter of space exploration, it's clear that the possibilities are endless. With continued innovation and collaboration, humanity will undoubtedly achieve new milestones in the exploration of space, unlocking the mysteries of the cosmos and expanding our presence beyond Earth.。
Microstructure and mechanical properties of
Microstructure and mechanical properties ofZrB 2–SiC–ZrO 2f ceramicLin Jia,a ZhangXinghong,a ,⇑Wang Zhi ,b ,⇑and Han Wenbo aaNational Key Laboratory of Science and Technology on Advanced Composites in Special Environments,Harbin Institute of Technology,Harbin 150001,PR ChinabSchool of Aeronautics and Astronautics,Faculty of Vehicle Engineering and Mechanics,State Key Laboratory of Structural Analysis for Industrial Equipment,Dalian University of Technology,Dalian 116024,PR ChinaReceived 10January 2011;accepted 12January 2011Available online 15January 2011ZrB 2–SiC–ZrO 2f ceramic was fabricated by hot-pressing at 1850°C for 1h under a uniaxial load of 30MPa in vacuum.The ZrB 2–SiC–ZrO 2f ceramic thus produced showed excellent fracture toughness due to the addition of ZrO 2fiber.The increase in toughness was attributed mainly to the addition of the ZrO 2fiber,which could enhance fiber pull-out,crack bridging and crack branching.In addition,the stress-induced transformation toughening was also considered to be main reason for the improvement in toughness.Ó2011Acta Materialia Inc.Published by Elsevier Ltd.All rights reserved.Keywords:Ceramics;Microstructure;Mechanical properties;CompositesZirconium diboride (ZrB 2)is one of the families ofmaterials known as ultra-high-temperature ceramics [1].Because of strong covalent bonding and low self-diffu-sion,high temperatures and external pressures are re-quired to densify monolithic ZrB 2[2].In previous studies,nominally stoichiometric ZrB 2without additives has only been densified by hot-pressing at 2000°C or higher with pressures of 20–30MPa,or at reduced tem-peratures (1790–1840°C)with much higher pressures (800–1500MPa)[3].Recent studies have shown that the addition of SiC particles improves the densification of ZrB 2by maintaining a fine grain size and a uniform distri-bution of the reinforcing phase,and enhances oxidation resistance by promoting the formation of silicate-based glasses that inhibit oxidation at temperatures between 800and 1700°C [4].Unfortunately,unsatisfactory frac-ture toughness is still the obstacle preventing ZrB 2–SiC ceramic from being widely used,especially for applica-tions in thermal shock conditions with high heat transfer and/or rapid environmental temperature changes,such as furnace elements,plasma arc electrodes,hypersonic air-craft,reusable launch vehicles,or rocket engines and ther-mal protection structures for leading edge parts onhypersonic reentry space vehicles [1–3,5].One method for improving thermal shock resistance is to tailor the structure on multiple length scales to produce architec-tures that are engineered to enhance thermal shock resis-tance while maintaining load-bearing capability—zirconia (ZrO 2)particles [6],graphite flakes [7],carbon fi-bers [8]or SiC whiskers [9]have been used as toughening materials.In addition,among these materials ZrO 2is of particular interest as it undergoes at least three crystallo-graphic transformations (monoclinic,tetragonal and cu-bic)when it cools from high temperature to room temperature,shown as the following transformation [10]:222C 2370C 2370C950C1170ZrO c ZrO t ZrO m −°⎯⎯←⎯→⎯°−°⎯⎯←⎯→⎯°−It has been shown that yttria-stabilized tetragonal zir-conia polycrystals (Y-TZP)possess superior fracture toughness.The high toughness of the Y-TZP monoliths arises from the volume expansion (4–5%)because of the stress-induced martensitic phase transformation of tetragonal to monoclinic symmetry in the stress field of propagating cracks,known as transformation tough-ening [11,12].Furthermore,fiber is found to be effective in strengthening and toughening ceramic materials,and1359-6462/$-see front matter Ó2011Acta Materialia Inc.Published by Elsevier Ltd.All rights reserved.doi:10.1016/j.scriptamat.2011.01.019⇑Correspondingauthor.Tel./fax:+8645186402382;e-mail:jiajia10182003@Scripta Materialia 64(2011)872–875/locate/scriptamatthe toughening is mainly the result of three mechanisms:fiber bridging,fiber pullout and crack deflection [13,14].It was expected that the toughness can further be improved when both fiber-toughening and phase transformation are incorporated into the ceramic ma-trix.Nevertheless,there are few reports in the open liter-ature on the cooperative toughening of fibers and transformation toughening of ZrO 2fiber-toughened ZrB 2–SiC ceramics.In this study,in order to improve further the fracture toughness of ZrB 2–SiC ceramic so that this material can be used more widely in severe environments,ZrB 2–SiC ceramic toughened with ZrO 2fiber was fabricated by hot pressing.The microstructure and the mechanical properties of the ZrB 2–SiC–ZrO 2f ceramic were investi-gated and are discussed in detail.The purpose of this paper is to take the lead in reporting ZrB 2–SiC ceramic toughened by ZrO 2fiber,and this study clearly showed that the addition of ZrO 2fiber into ZrB 2–SiC ceramic is a promising way to improve the fracture mercially available ZrB 2powder (2l m,>99.5%,Northwest Institute for Non-ferrous Metal Research,PR China),SiC (1l m,>99.5%,Weifang Kaihua Mi-cro-powder Co.Ltd.,PR China)and ZrO 2fiber (mean diameter 5–8l m,mean length 200l m,>99%,Shan-dong Huolong Ceramic Fiber Co.Ltd.,PR China)were used as raw material.The powder mixtures of ZrB 2plus 20vol.%SiC plus 15vol.%ZrO 2fiber (ZrB 2–SiC–ZrO 2f )were ball-mixed for 20h in a polytetrafluoroethylene bottle using ZrO 2balls and ethanol as the grinding med-ia.After mixing,the slurry was dried in a rotary evapo-rator.The resulting powder mixtures were hot-pressed at 1850°C for 1h under a uniaxial load of 30MPa in vacuum.The microstructural features of the hot-press-ing composite were observed by scanning electron microscopy (SEM;FEI Sirion,Holland)with simulta-neous chemical analysis by energy-dispersive spectros-copy (EDS;EDAX Inc.).The phase composition was determined by X-ray diffraction (XRD;Rigaku,Dmax-rb,Cu K a =1.5418A˚).The bulkspecimens was measured by the Archimedes Flexural strength (r )was tested by three-point on 3mm Â4mm Â36mm bars,using a 30and a crosshead speed of 0.5mm min À1.Each was ground and polished with diamond slurries a 1l m finish.The edges of all the specimens fered to minimize the effect of stress to machining flaws.Hardness (Hv 0.5)was by Vickers’indentation with a 4.9N load 10s on polished sections.Fracture was evaluated by a single-edge notched beam a 16mm span and a crosshead speed of 0.05using 2mm Â4mm Â22mm test bars,on the used for the flexural strength measurements.All and fracture bars were cut with the tensile pendicular to the hot-pressing direction.A number of six specimens were tested for each tal condition.The hot-pressed ZrB 2–SiC–ZrO 2f ceramic to produce bars for mechanical property test sured bulk densities of 5.44g cm Àing a ture calculation,and assuming that the true were 6.09g cm À3for ZrB 2, 3.21g cm À3for 6.11g cm À3for ZrO 2[1,9],the theoretical density of the ZrB 2–SiC–ZrO 2f ceramic was calculated to be 5.52g cm À3.Based on this true density,the relative den-sity of the ZrB 2–SiC–ZrO 2f ceramic was as high as 98.6%.An XRD spectrum obtained from the fractured and polished surface of the ZrB 2–SiC–ZrO 2f ceramic is shown in Figure 1.Phase analysis indicates that the pre-dominant phases of this hot-pressed ZrB 2–SiC–ZrO 2f ceramic are ZrB 2,SiC and t-ZrO 2as well as a trace of ZrC on the polished surface of the ZrB 2–SiC–ZrO 2f ceramic.The formation of ZrC was attributed to the reaction of SiC with ZrO 2:2ZrO 2ðs Þþ3SiC ðs Þ¼2ZrC ðs Þþ3SiO ðg ÞþCO ðg Þð1ÞThe gaseous products,i.e.CO and SiO,were readily removed by the high vacuum (pressure 5Pa),which is thermodynamically favorable to reaction (1).Further-more,the very fine ZrC particles formed in situ on the surface of the ZrO 2and SiC particles were highly sinter-able,which could also provide a higher driving force for sintering as densification is driven by minimization of surface free energy,which was also thought to be main reason responsible for the high densification [3].In addi-tion,the effect of the ZrC phase on the relative density was not considered because the exact content of this phase was not calculated,and moreover the density of the ZrC phase is close to the densities of the ZrB 2and ZrO 2phases [1,3].As seen in Figure 1,the diffraction peak of m-ZrO 2phase was observed on the fracture sur-face of the ZrB 2–SiC–ZrO 2f ceramic.It is known that when subjected to external load,stress concentration in the hot-pressed ZrB 2–SiC–ZrO 2f ceramic will result in the phase transformation from t-ZrO 2to m-ZrO 2with volume change [10].According to the formula of Toraya et al.[15],the volume fraction of the m-ZrO 2(Vm )was calculated by measuring the intensities of the (111)and (11 1)reflec-tions of the monoclinic phase and the (111)peak of the tetragonal phase:L.Jia et al./Scripta Materialia 64(2011)872–875873where Xm is the integrated intensity ratio,and Im and It are the peak intensities of the m-ZrO 2and t-ZrO 2,respectively.Furthermore,the obtained Vm was individ-ually normalized to the volume fraction of ZrO 2(V ZrO 2)in each composite as follows:Vmtot ¼Vm ÂV ZrO 2100ð4ÞTherefore,the result of V mtot on the fracture surface minus that on the polished surface equals the fraction transformed from t-ZrO 2to m-ZrO 2during fracture (i.e.t-ZrO 2transformability).The obvious volume expansion upon phase transformation from t-ZrO 2to m-ZrO 2was calculated,and found to favor an increase in the fracture toughness of the ZrB 2–SiC–ZrO 2f ceramic.SEM images of the polished surface of the ZrB 2–SiC–ZrO 2f ceramic are presented in Figure 2.It was con-firmed by EDS analysis (not shown here)that the small dark phase was SiC which as dispersed uniformly in the lighter ZrB 2matrix;the rod-like phase was ZrO 2fiber.A uniform distribution of short ZrO 2fibers in ZrB 2matrix can be seen in Figure 2B.It was expected that the slight reaction of SiC grain with ZrO 2fiber occurred due to the lower hot pressing temperature and the lower content of SiC grains.Mechanical scratches on ZrO 2fibers andsize was estimated by measuring at least 120grains,and found to be 4.5and 3.4l m for ZrB 2and SiC,pared with raw particles,the growth of ZrB 2grains was inhibited by SiC grain because of the reaction of SiC grains with trace oxide impurities on the ZrB 2particle surfaces [4].It can be seen from the insert in Figure 3A that a perfect interface between ZrO 2fiber and other phases was observed,which also indicated that there was no obvious reaction between SiC grains and ZrO 2fibers.The perfect interface of ZrO 2fiber,SiC and other phases enhanced the mechan-ical properties of the ZrB 2–SiC–ZrO 2f ceramic [3].Sig-nificant pits and fiber roots occurred in the fracture surface of the ZrB 2–SiC–ZrO 2f ceramic,which indicated that the ZrO 2fibers were pulled out during the fracture process,as shown in Figure 3B.In order to further investigate the effect of ZrO 2fibers on the crack propagation models,typical crack propa-gation paths were derived using Vickers’indentation method as shown in Figure 4.The radial crack at the edge of Vickers’indentation clearly revealed that the crack propagation models caused by addition of ZrO 2fiber mainly included crack branching and crack bridg-ing.It is believed that such reaction depletes the energy of crack propagation during fracture and leads to the improvement of the fracture toughness [17].874L.Jia et al./Scripta Materialia 64(2011)872–87524±0.9GPa for ZrB2–SiC ceramics but statistically equivalent to19.3±0.4GPa of the similar ZrB2–SiC–ZrO2p ceramic[4,6].It has been recognized that the hardness of a material is generally decreased by the addition of weak second phases,such as carbon/graph-ite,h-BN and pores[18].Compared with the ZrB2–SiC ceramics[4],the reduction in the hardness of the ZrB2–SiC–ZrO2f ceramic was ascribed to its lower rela-tive density.The measured fracture toughness of the ZrB2–SiC–ZrO2f ceramic ranged from 6.3to7.6 MPaÁm1/2(average 6.8±0.6MPaÁm1/2),which was obviously higher than reported results for monolithic ZrB2(2.3–3.5MPaÁm1/2)and ZrB2–SiC composites (4.0–5.3MPaÁm1/2)[3,4].Furthermore,the fracture toughness of the ZrB2–SiC–ZrO2f ceramic was obvi-ously higher than6.0±0.2MPaÁm1/2of similar ZrB2–SiC–ZrO2p ceramic reported in the literature[6].Com-bined with XRD and SEM analysis,the improvement in strength and toughness was attributed mainly to the phase transformation toughening,fiber pull-out,crack bridging and branching,because these interaction effects absorb fracture energy.In conclusion,the ZrB2–SiC–ZrO2f ceramic was hot-pressed at1850°C for1h under a uniaxial load of 30MPa in vacuum.The relative density of the ZrB2–SiC–ZrO2f ceramic was calculated to be98.6%and the XRD spectra indicated ZrO2phase transformation from tetragonal to monoclinic symmetry.Theflexural strength of the ZrB2–SiC–ZrO2f ceramic was1085±118MPa, which is higher than788±78MPa of the similar ZrB2–SiC–ZrO2p ceramic.The hardness of the ZrB2–SiC–ZrO2f ceramic was found to be as high as18.4±1.3GPa,which is slightly lower than the value of about24±0.9GPa found for ZrB2–SiC ceramics but statistically equivalent to19.3±0.4GPa of the similar ZrB2–SiC–ZrO2p cera-mic.It was recognized that the hardness of a material was in general decreased by the addition of weak second phases,such as carbon/graphite,h-BN and -pared with the ZrB2–SiC ceramics,the reduction in the hardness of the ZrB2–SiC–ZrO2f ceramic was mainly as-cribed to its lower relative density.The measured fracture toughness of the ZrB2–SiC–ZrO2f ceramic ranged from 6.3to7.6MPaÁm1/2(average6.8±0.6MPaÁm1/2),which increased by approximately134%compared to the re-ported results of monolithic ZrB2(2.3–3.5MPaÁm1/2), 46%for ZrB2–SiC composites(4.0–5.3MPaÁm1/2), and13%for the similar ZrB2–SiC–ZrO2p ceramic (6.0±0.2MPaÁm1/2).The observed toughening mecha-nisms were attributed tofiber pull-out,crack bridging, crack branching and phase transformation toughening. This study clearly showed that the addition of ZrO2fiber to ZrB2–SiC ceramic is a promising way to improve the fracture toughness of this material.This work was supported by the NSFC (51072042,10725207),the Science Fund for Outstanding Youths of Heilongjiang Province and China Postdoc-toral Science Foundation Funded Project(2010048 1220).[1]X.H.Zhang,Q.Qu,J.C.Han,W.B.Han,C.Q.Hong,Scripta Mater.59(2008)753.[2]X.H.Zhang,W.J.Li,C.Q.Hong,W.B.Han,J.C.Han,Scripta Mater.59(2008)1214.[3]W.G.Fahrenholtz,G.E.Hilmas,I.G.Talmy,J.A.Zayko-ski,J.Am.Ceram.Soc.90(5)(2007)1347.[4]A.L.Chamberlain,W.G.Fahrenholtz,G.E.Hilmas,D.T.Ellerby,J.Am.Ceram.Soc.87(6)(2004)1170.[5]D.W.Ni,G.J.Zhang,Y.M.Kan,Y.Sakka,ScriptaMater.60(2009)615.[6]X.H.Zhang,W.J.Li,C.Q.Hong,W.B.Han,J.C.Han,Mater.Lett.62(2008)2404.[7]X.H.Zhang,Z.Wang,X.Sun,W.B.Han,C.Q.Hong,Mater.Lett.62(2008)4360.[8]F.Y.Yang,X.H.Zhang,J.C.Han,S.Y.Du,J.AlloysCompd.472(2009)395.[9]X.H.Zhang,L.Xu,S.Y.Du,W.B.Han,J.C.Han,C.Y.Liu,Scripta Mater.59(2008)55.[10]R.C.Garvie,R.H.J.Hannink,R.T.Pascoe,CeramicSteel,Nature,London,1975.[11]C.L.Yang,H.I.Hsiang,C.C.Chen,Ceram.Int.31(2005)297.[12]G.A.Gogotsi,V.I.Galenko,S.P.Mudrik,B.I.Ozersky,Ceram.Int.36(2010)345.[13]B.Budiansky,Y.Q.L.Cui,Mech.Mater.21(1995)139.[14]J.P.Singh,D.Singh,M.Sutaria,Composites:Part A30(1999)445.[15]H.Toraya,M.Yoshimura,S.Somiya,J.Am.Ceram.Soc.67(1984)119.[16]M.Singh,R.Asthana,Mater.Sci.Eng.A460–461(2007)153.[17]K.T.Fabert,A.G.Evans,Acta Metall.31(1983)565.[18]X.J.Zhou,G.J.Zhang,Y.G.Li,Y.M.Kan,P.L.Wang,Mater.Lett.61(2007)960.。
去博物馆英语作文
Visiting a museum is an enriching experience that can broaden ones perspective and deepen ones understanding of history,culture,and art.Heres how you might write an essay in English about a visit to a museum,using a Frenchstyle English approach which might include a more formal and sophisticated tone.Title:An Enchanting Journey Through Time:My Visit to the MuseumIntroduction:From the moment I set foot in the grand hall of the museum,I was transported to a realm where time stood still,and the whispers of history echoed through the corridors.The museum,a sanctuary of knowledge and beauty,beckoned me with its promise of a journey through the ages.Body Paragraph1:The Historical WingThe first wing I explored was dedicated to history.As I meandered through the exhibits,I was greeted by the artifacts of civilizations long past.The intricate designs on ancient pottery,the stern gaze of a medieval knights armor,and the delicate craftsmanship of a Renaissance tapestry all spoke to me of the ingenuity and artistry of our ancestors.Each piece was a testament to the human spirits relentless pursuit of progress and perfection.Body Paragraph2:The Art GalleryMoving on to the art gallery,I was struck by the vivid colors and bold strokes that adorned the canvases.The works of the masters,from the serene landscapes of Monet to the abstract expressions of Picasso,stirred a sense of awe within me.The gallery was a testament to the power of art to evoke emotion and provoke thought.It was here that I found myself lost in contemplation,pondering the meaning behind each masterpiece. Body Paragraph3:The Science and Technology SectionThe science and technology section was a stark contrast to the artistic endeavors I had just admired.Here,the focus was on innovation and discovery.The exhibits showcased the evolution of human understanding,from the rudimentary tools of early man to the sophisticated machinery of the modern age.The section was a celebration of human ingenuity and a reminder of our ceaseless quest for knowledge.Body Paragraph4:The Cultural ExhibitsCultural exhibits were a tapestry of diversity,weaving together the threads of various traditions and customs.Each exhibit was a window into a different world,offering a glimpse into the lives and beliefs of people from all corners of the globe.The richness ofthe cultural displays was a testament to the beauty of our shared humanity and the importance of preserving our collective heritage.Conclusion:As I left the museum,I felt a profound sense of gratitude for the opportunity to have walked through its halls.The museum was more than just a building filled with objects it was a living,breathing testament to the human experience.It was a place where the past, present,and future intersected,offering a glimpse into the vast tapestry of human existence.My visit to the museum was not just an educational experience it was a journey of discovery,a chance to connect with the stories of those who came before us and to ponder our place in the grand narrative of time.Closing Thoughts:In the hallowed halls of the museum,one can find not only the relics of the past but also the seeds of the future.It is a place where learning is a journey without end,and where each visit leaves one with a renewed sense of wonder and appreciation for the world we inhabit.As I reflect on my visit,I am reminded that the museum is not just a destination but a gateway to the infinite possibilities of human achievement and understanding.。
Gravity on Conformal Superspace
a r X i v :g r -q c /0311034v 1 11 N o v 2003Gravity on Conformal SuperspaceBryan KelleherThesis submitted in fulfillment of the requirements of the degree of Doctor of Philosophy from the Department of PhysicsUniversity College CorkNational University of Ireland,CorkSupervisor :Prof.Niall ´OMurchadha June 2003To my familyAcknowledgementsThere are many people I wish to thank.Firstly,Niall,go raibh m´ıle,m´ıle maith agat.It has been both a pleasure and a privilege.Thanks to the entire physics department for everything over the years-great times,a superb atmosphere and lifelong st -but most definitely not least-thanks to my parents,my brothers and sister,my wife to be Gill and my extended family and friends.I could not(and more than likely would not)have done it without you.AbstractThe configuration space of general relativity is superspace-the space of all Riemannian 3-metrics modulo diffeomorphisms.However,it has been argued that the configuration space for gravity should be conformal superspace-the space of all Riemannian3-metrics modulo diffeomorphisms and conformal transformations.Taking this conformal nature seriously leads to a new theory of gravity which although very similar to general relativity has some very different features particularly in cosmology and quantisation.It should reproduce the standard tests of general relativity.The cosmology is studied in some detail.The theory is incredibly restrictive and as a result admits an extremely limited number of possible solutions.The problems of the standard cosmology are addressed and most remarkably the cosmological constant problem is resolved in a natural way. The theory also has several attractive features with regard to quantisation particularly regarding the problem of time.Contents1Introduction11.1Introduction (1)1.2General Relativity (2)1.3(3+1)-Decomposition (2)1.4York’s Approach (5)1.4.1Gauge Fixing in GR (6)1.5Lagrangian and Hamiltonian Formulations (7)1.5.1The Lagrangian (7)1.5.2Constraints and Evolution Equations (9)1.5.3The Hamiltonian (11)1.6Jacobi Action (11)1.7Conformally Related Solutions (12)1.8Topological Considerations (14)1.8.1Integral Inconsistencies (14)1.9Other Results (18)1.10Problem (18)2A New Hope202.1The Need For A Change (20)2.1.1Resolving The problem(s) (20)2.2The Hamiltonian Formulation (24)2.3Jacobi Action (26)2.4Conformally Related Solutions (27)2.4.1What ofξc? (28)2.5Topological Considerations (30)2.5.1Integral Inconsistencies(Slight Return) (30)2.5.2New Constraints (31)2.6The Hamiltonian Formulation (32)2.7The Volume (34)2.8Jacobi Action (34)2.9Comparison with GR (35)2.10Time (36)2.11Light Cones (37)2.12Matter in General Relativity (38)2.12.1Cosmological Constant (38)2.12.2Electromagnetism (39)2.12.3Dust (40)2.13Matter and Conformal Gravity (40)2.13.1Cosmological Constant (41)2.13.2Electromagnetism (41)2.13.3Dust (42)3Four Dimensions!443.1Introduction (44)3.2BOM Conformal Gravity (44)3.2.1The Action (45)3.2.2Dimensional Properties of Conformal Transformations (45)3.2.3Varying with respect to gαβ (46)3.2.4Varying with respect toφ (47)3.2.5A note on the action (47)3.2.6(3+1)-Decomposition (47)3.3Conformally Related Solutions (51)3.3.1Topological Considerations (51)3.4New Conformal Gravity (54)3.4.1Non-Compact (55)3.4.2Compact Manifold (56)3.5Special Case (61)3.6The Solar System (61)3.7Comment (62)4Cosmology634.1Introduction (63)4.2Cosmology In General Relativity (63)4.2.1Open Universe (63)4.2.2Flat Universe (64)4.2.3Closed Universe (64)4.3Cosmology in the Conformal Theory (66)4.3.1Open Universe (66)4.3.2Flat Universe (67)4.3.3The Closed Universe (68)4.4Cosmological Parameters (71)4.4.1Hubble Parameter (72)4.4.2Deceleration Parameter (72)4.5Problems of the Standard Cosmology (72)4.5.1The Cosmological Constant Problem (73)4.5.2The Flatness Problem (73)4.5.3The Horizon Problem (74)4.6Some Numbers (76)4.7A Non-Standard Cosmology:Anisotropy (78)4.7.1The Kasner Universe (78)4.7.2Effective Anisotropic Energy Density (79)4.8Discussion (80)5Discussion81Chapter1Introduction1.1IntroductionAs formulated by Einstein,the natural arena for gravity as represented by general rela-tivity(GR)is spacetime.We have a purely4-dimensional structure and the4-geometry reigns.(The invention of GR was a truly monumental achievement and no offence is intended by any attempt here to suggest an alternative theory.)Dirac[1]and Arnowitt, Deser and Misner(ADM)[2]reformulated the theory in canonical form which is more in-keeping with other areas of modern physics.This formulation led to Wheeler’s identi-fication of the configuration space as superspace and GR as the theory of the evolution of the3-geometry which led to the coining(again by Wheeler)of geometrodynamics.To get superspace onefirst considers Riem the space of all Riemannian3-geometries.Super-space is then Riem modulo diffeomorphisms,that is,we identify all3-geometries related by diffeomorphisms.York[3]went further and identified the conformal3-geometry with the dynamical degrees of freedom of the gravitationalfield.The correct configuration space for gravity should not be superspace but rather conformal superspace-superspace modulo conformal trans-formations.Barbour and´O Murchadha(BOM)[4]went further again and formulated a theory with conformal superspace at the very core.We’ll begin with a brief review of GR as found from the Einstein-Hilbert action and the ADM formulation.We’ll then discuss the York approach and the original BOM the-ory.All of this will serve as a warm up(albeit,a necessary warm up)to the real focus ofthis work.1.2General RelativityAlthough Einstein developed GR using beautiful physical reasoning and principles it is the Hilbert derivation from an action principle which is more instructive to us.(We will however refer to the action as the Einstein-Hilbert action as it was Einstein’s work which inspired Hilbert tofind the action to begin with.)The Einstein-Hilbert action of general relativity is well known.It has the formS=1−(4)g(4)R d4x(1.1)where gαβis the4-metric and(4)R is the four dimensional Ricci scalar.The action is varied with respect to gαβand the resulting equations are the(vacuum)Einstein equationsGαβ= Rαβ−1δgαβ(1.4) 1.3(3+1)-DecompositionBefore we consider the new theory it will be instructive to recall the ADM treatment of general relativity as much of this will carry straight over to the new theory.The idea in the ADM treatment is that a thin-sandwich4-geometry is constructed from two3-geometries separated by the proper time dτ.The4-metric found from the ADM construction is(4)g00(4)g0k(4)g i0(4)g ik=(N s N s−N2)N kN i g ik(1.5)N=N(t,x,y,z)is the lapse function given bydτ=N(t,x,y,z)dt(1.6) and N i=N i(t,x,y,z)are the shift functions given byx i2(x m)=x i1−N i(t,x,y,z)dt(1.7) where x i2is the position on the“later”hypersurface corresponding to the position x i1on the“earlier”hypersurface.The indices in the shift are raised and lowered by the3-metric g ij.The reciprocal4-metric is(4)g00(4)g0k(4)g i0(4)g ik=−1/N2N k/N2N i/N2g ik−N i N k/N2(1.8)The volume element has the formg dt d3x(1.9)This construction of the four metric also automatically determines the components of the unit timelike normal vector n−(4)g(4)R d4x(1.12) Using the Gauss-Codazzi relations we get(4)R=R−(trK)2+K ab Kab−2Aα;α(1.13) where Aαis given by(as earlier)Aα= nαtrK+aα (1.14)nαis the unit timelike normal andaα=nα;βnβ(1.15) is the four-acceleration of an observer travelling along nN.Substituting into the action givesS= N√2£n.In the coordinates we are using here the extrinsic curvature takes the formK ab=−1∂t−N a:b−N b;a(1.18)The action is varied with respect to∂g abg g ab trK−K ab (1.19) and varied with respect to N and N a to give the initial value equationsH=0and H a=0(1.20) respectively,whereH=√2(trπ)2 −√∂t =δH∂t =−δH1.4York’s ApproachThe Hamiltonian and momentum constraints correspond to the00and0a components of Einstein’s equations(1.3).They are equivalently initial-value constraints.We need to be able tofind initial data which satisfy these.One method was proposed by Baerlein, Sharp and Wheeler(BSW)[5].This is known as the thin-sandwich conjecture.First the pair{g ab,∂g ab√g ab trπ(1.31)3Now,if the CMC condition holds then the momentum constraint reduces to▽bσab=0(1.32)Now the tracefree part is transverse-traceless(TT).This property is invariant under the conformal transformationg ab−→ω4g ab(1.33)σab−→ω−4σab(1.34) It is important here that trπnow transforms in a different way to the tracefree partσab. For the momentum constraint to be conformally invariant we need to definetrp=trπg−→trp(1.35)That is,trp transforms as a conformal scalar.Since there is a well known method tofind a TT tensor we canfind the pair{g ab,σab}easily.The Hamiltonian constraint transforms to becomeσabσabφ−7−13trp(1.37) is often interpreted as a notion of time,the York time,due to the properties of trp noted above.1.4.1Gauge Fixing in GRIt is important to notice the difference between a single use of the CMC condition tofind initial data and subsequent use of the condition when the data is propagated.This is byno means guaranteed.As noted earlier,once the initial data has been specified the lapse and shift are freely specifiable.To maintain the CMC slicing during the evolution it is necessary to choose the lapse in a particular ing the evolution equations we get∂trp4+▽c trπg N c(1.38) To ensure CMC slicing we need to set▽c trπ=0and∂trp∂t =2NR−2▽2N+N(trp)2∂t=0.Thus∂trpg(R−(trK)2+K ab K ab)dtd3x(1.42)To find the conformal action we simply transform the Lagrangian under the transforma-tiong ab −→ψ4g ab(1.43)We need to define how the lapse and shift are transformed under such a transformation.In a later chapter we will see that this theory can be found using a 4-dimensional action whereg αβ−→ψ4g αβ(1.44)and under this we would haveN −→ψ2N(1.45)andN i −→ψ4N i(1.46)Let’s adopt these as our transformation rules.Under such a transformationR −→ψ−4R −8▽2ψ2N∂g ab∂t−→ψ4∂g ab∂t(KN )ab −→ψ4(KN )ab +4ψ3g ab N c ▽c ψ(1.50)ThusK ab −→ψ2B ab =−ψ2∂t−(KN )ab −θg ab(1.51)whereθ=−4∂t −N c ▽c ψ(1.52)The Lagrangian is thusL =N√ψ+B ab B ab −(trB )2(1.53)Noteψ ˙ψ−ψ,i N i .We can alsofind a coordinateindependent form for B.This isB=−1(ψ4g)(1.54)This is analogous to the expressionK=−1(g)(1.55)for the extrinsic curvature K in general relativity.1.5.2Constraints and Evolution EquationsWe can perform the usual variations tofind the constraints of the theory.Let’s vary with respect to Nfirst.This gives us,R−8▽2ψψ −▽2 Nψ3 =0(1.60)where we have used the other constraints to simplify.The constraints may appear more familiar if we write them in terms of the canonical momentum rather than B ab.Wefind the canonical momentum,πab by varying the action with respect to∂g abgψ4 g ab trB−B ab (1.61) Then using equation(1.58)we getπab=−√The constraints are then,πabπab−gψ8 R−8▽2ψψ −▽2 Nψ3 =0(1.66)Equation(1.63)corresponds to the Hamiltonian constraint of General Relativity.Equa-tion(1.64)is the usual momentum constraint of general relativity which represents diffeo-morphism invariance.Equation(1.65)is new and represents conformal invariance.Our initial data consists of a pair(g ab,πab)which must satisfy equations(1.64)and(1.65). These are the initial value equations.Equation(1.63)is used tofind the“conformal field”ψonce we have specified the initial data.Equation(1.66)is a lapse-fixing equation which is used to determine N throughout.We must check if these constraints are propa-gated under evolution.The evolution equations are found in the usual way.They are∂g ab2ψ−4πab+(KN)ab−θg ab(1.67) and∂πabgNψ4 R ab−g ab R−8▽2ψ2ψ−4πacπb c+√gψ3 ▽a▽bψ+3g ab▽2ψ+4√g▽(a(Nψ3)▽b)ψ+▽c N cπab −πbc▽c N a−πac▽c N b−θπab (1.68)It can be verified that these equations do indeed preserve the constraints.We can see how similar the results are to those in York’s approach.The Hamiltonian constraint has become the Lichnerowicz equation.The momentum is TT.Also,the lapsefixing equation is the gauge requirement of GR to preserve the trπ=0constraint.Of course,those equations are all secondary in GR whereas here they have arisen directly through a variational procedure!1.5.3The HamiltonianNow that we have found the momentum it is straightforward to find the Hamiltonian.As usual we haveH =πab∂g abgψ4R −8▽2ψ2(trπ)2√2(trπ)2−√ψ−2N a ▽b πab +θtrπd 3x(1.71)Recalling the constraints we see that yet again,as found by Dirac and ADM,the Hamil-tonian is a sum of the constraints with Lagrange multipliers.1.6Jacobi ActionBaerlein,Sharp and Wheeler [5]constructed a Jacobi Action for general relativity.Their action was,S =+g√T GR d 3x(1.72)whereT GR =g ac g bd −g ab g cd∂g ab∂t−(KN )cd(1.73)Variation with respect to∂g abgR∂t−(KN )cd(1.74)This expression is squared to give the Hamiltonian constraint.The variation with respect to N a gives the momentum constraint.The evolution equations are found in the usual way.The equations found with the Jacobi action are those of general relativity if we identify 2N and R .We want to construct the analogous case in conformal gravity.Letus return to our (3+1)Lagrangian,L =N√ψ−(trB )2+B ab B ab(1.75)We can write this asL =√ψ+1∂t−(KN )ab −θg ab.We now extremise with respect to N .This gives us,N =+2βab βab −(trβ)21ψ −1dλ √R −8▽2ψT d 3x(1.78)where T =βab βab −(trβ)2 .This is the conformal gravity version of the BSW action (1.72).We can do all the usual variations here:N a ,˙ψand ψ.These give the momentum constraint,the conformal constraint and the lapse-fixing equation respectively.Becauseof the independent variations of ˙ψand ψ,it turns out that we may vary with respect to θand ψto get the conformal constraint and the lapse-fixing equation respectively.When we find the canonical momentum πab we can “square”it to give the “Hamiltonian constraint.”Actually,this is precisely the BOM action found by starting with the BSW action and conformalising it under conformal transformations of the 3-metricg ab −→ψ4g ab(1.79)The Jacobi action is manifestly 3-dimensional and its configuration space is naturally conformal superspace -the space of all 3-D Riemannian metrics modulo diffeomorphisms and conformal rescalings.1.7Conformally Related SolutionsIn conformal superspace conformally related metrics are equivalent.Thus conformally related solutions of the theory must be physically equivalent and so it is crucial that we have a natural way to relate such solutions.Suppose we have one set of initial data (g ab ,πab ).These must satisfy the constraints (1.64)and (1.65).We solve the Hamiltonian constraint (1.63)for our “conformal field”ψ.Suppose now we start with a different pair (h ab ,p ab )where h ab =α4g ab and ρab =α−4πab .Our new initial data is conformallyrelated to the original set of initial data.This is allowed as“transverse-traceless”-ness is conformally invariant and so our initial data constraints are satisfied.All we must do is solve the new Hamiltonian constraint for our new conformalfieldχsay.This constraint is nowρabρab=hχ8 R h−8▽2hχ.That is,ψis automati-αcally transformed when our initial data is transformed.Now,ψ4χ4h ab==Ng−1∂t=−√gN∂t−√2πacπb c−▽c N aπbc−▽c N bπac+▽c N cπab (1.88)These are exactly those of general relativity on a maximal slice.Thus,solutions of general relativity in maximal slicing gauge are also solutions here.There are of course solutions of general relativity which do not have a maximal slicing and these are not solutions of the conformal theory.1.8Topological ConsiderationsSo far we have not considered any implications which the topology of the manifold may have.In an asymptoticallyflat case we have no problems with the theory as it stands. This is not the case however in a topology which is compact without boundary.1.8.1Integral InconsistenciesRecall the lapse-fixing equation of the theory in the physical representation(removing the “hats”for simplicity),NR−▽2N=0(1.89) Let’s integrate this equation:√g▽2N d3x=0(1.90)The second term integrates to zero and so we just have√gNR d3x− √gNR d3x(1.93) is positive definite.The second integral is− √gN▽c N dΣc(1.95)whereΣc is the boundary on which N=0.Since N is decreasing on the boundary we have that this term is positive definite.This means however that we have a vanishing sum of two positive definite quantities.This is a contradiction.Thus we must have N≡0. We get frozen dynamics.(This is not the case with a manifold which is asymptotically flat so the earlier analysis works in that case.)Frozen dynamics also arises in general relativity if one imposes afixed trπ=0gauge condition.However,this is a problem of the gauge rather than a problem of the theory as with conformal gravity.(See[6]for a treatment of this problem.)The easiest way to resolve this problem involves a slight change to the action.We intro-duce a volume term.The inspiration for this term comes from the Yamabe theorem.The action isS= N√V2/3 R−8▽2ψgψ6d3x(1.97) The power of2gψ4V4/3 R−8▽2ψψ −▽2 Nψ3 =Cψ5(1.102)The term C is given byC= N√V R−8▽2ψV(ψ)4/3(1.104)▽bπab=0(1.105) trπ=0(1.106) NR−▽2N=C(1.107)where C is nowC=1g√T: A is the average of A given by the usual notion of averageA = √ √gNR d3x− ▽2N d3x− √gNR d3x− √:Although we have only used the physical representation in our integral tests it can be verified easily that everything also works out in the general representation.Of course,in EVERY situation,this must be true.We are losing nothing by working in the physical representation.We should consider the evolution equations again now that we have changed the action. The evolution equations become∂g ab2V(ψ)2∂t =−N√V2/3 R ab−g abR−8▽2ψ√gψgψ3gg ab g3√V2/3(1.114)where C is as in(1.103).As usual we can write these in the physical representation.In this form the evolution equations are∂g ab2V2∂t =−N√V2/3 R ab−g ab R−2NV4/3gπacπb c +√V2/3 ▽a▽b N−g ab▽2N+▽c N cπab −πbc▽c N a−πac▽c N b−2gg ab CThe lapse-fixing equation isNR−▽2N=C(1.121) These are precisely the constraints and gaugefixing conditions for propagated maximal slicing in GR.The evolution equations are∂g ab2 πab+(KN)ab(1.122) and∂ πab g R ab−g ab R −2N g πac πb c+√3√V2/3(1.123)which are identical to those in GR apart from the global C term in the equation forπab. We can easilyfind the Hamiltonian and the Jacobi action for the new form.They are H= N V2/3gψ4 πabπab−1gψ4ψ d3x(1.124) andS= dλ √R−8▽2ψT3d3x(1.125) Note again the homogeneity throughout inψ.1.9Other ResultsThere has been work on other aspects of this theory not described here.It is unnecessary from the point of view of this work while,of course,being valuable in itself with a number of worthwhile results most notably on the constraint algebra and the Hamilton-Jacobi theory.The interested reader canfind this in[7].1.10ProblemAlthough the theory has emerged beautifully and easily form very natural principles we canfind at least one major problem immediately.Consider the volume of a hypersurface VV= √Taking the time derivative of this we get∂V2√∂td3x(1.127)This becomes∂V∂t=0(1.129) and the volume of the universe is static.This rules out expansion and thus the stan-dard cosmological solution is lost.In particular,the red-shift,an experimental fact,is unexplained.This is a serious shortcoming.All is not lost however...Chapter2A New Hope2.1The Need For A ChangeDespite all the promising features of the theory there is at least one major drawback.We canfind the time derivative of the volume quite easily and get that it is proportional to trπand thus is zero.That is,the volume does not change and so the theory predicts a static universe and we cannot have expansion.This is quite a serious problem as the pre-diction of expansion in GR is considered to be one of the theory’s greatest achievements. We are left with the following options:(a)Abandon the theory;(b)Find a new explanation of the red-shift(among other things);(c)Amend the theory to recover expansion.Thefirst option seems quite drastic and the second,while certainly the most dramatic, also seems to be the most difficult.Thus,let’s check what we canfind behind door(c).2.1.1Resolving The problem(s)Any change to the theory needs to be made at the level of the Lagrangian and so we’ll return to our earlier expression for LL=N√ψ+B ab B ab−(trB)2 (2.1)but naively change the form of B ab toB ab=−1∂t−(KN)ab−▽cξc g ab(2.2)Let’s vary the action with respect toξc.We getδL=N√gψ4 B ab−2trBg ab −1gψ4trB▽cδξc(2.3)Integrating by parts givesδL=2√3g ab trB(2.8) We shall retain the new form of B ab as defined above in(2.2)all the same.The Lagrangian now readsL=N√ψ+S ab S ab−2gψ4 R−8▽2ψ3ψn(trB)2 (2.10)Before we continue,one interesting point about S ab is the following.We haveS ab =B ab −12N∂g ab3g abg cd ∂g cd2N∂g ab2Ng ab ▽c ξc −1∂t−g cd (KN )cd−32N∂g ab3g abg cd∂g cd3g ab trK (2.15)That is,S abis the tracefree part of the extrinsic curvature and is independent of anyconformal fields.Let us find πab .This is done as usual by varying with respect to∂g abgψ42S ab δS ab −4gψ4S ab δB ab −13ψn trBg ab δB ab=2N√3ψn trBg abδB ab=−√3ψn S ab trBδ∂g abgψ4S ab +2gψn +4g ab trB(2.17)Splitting πab into its trace and tracefree parts will further clear things up.We’ll label the split asπab =σab +1gψ4S ab (2.19)and the trace is given bytrπ=2ψn+4trB(2.20) Note that our value of n is undefined as yet.The constraints are found by varying with respect toξc,ψ,N and N a.The confor-mal constraint and the lapse-fixing equation are given by varying with respect toξc and ψrespectively.These give▽c trπ=0(2.21) andNψ3 R−7▽2ψ4=0(2.22) respectively.From the variation with respect to N we getS ab S ab−2ψ =0(2.23) which in terms of the momentum isσabσab−1ψ =0(2.24) andfinally,from the variation with respect to N a we get▽bπab=0(2.25) We require conformal invariance in our constraints.Under what conditions is the momen-tum constraint(2.25)invariant?The tracefree part of the momentum,σab,has a natural weight of−4(from the original theory).That isσab−→ω−4σab(2.26) If trπ=0then we have conformal invariance.If not however,we require various further conditions.We need▽bσab=0(2.27)▽c trπ=0(2.28)and thattrp=trπg−→trp(2.29)under a conformal transformation.In our theory we have thefirst two conditions emerg-ing directly and naturally from the variation.Thus we simply define trp to transform as a conformal scalar as required.With this done our momentum constraint is conformally invariant.23Transforming the constraint(2.24)givesσabσab−1ψ =0(2.30) and so we must have n=−12for conformal invariance.The constraint then becomesσabσab−1ψ =0(2.31)(Note:This is exactly the Lichnerowicz equation from GR.However,we have found it directly from a variational procedure.)Thus we have determined the unique value of n and our constraints areσabσab−1ψ =0(2.32)▽bπab=0(2.33)▽c trπ=0(2.34) Nψ3 R−7▽2ψ4=0(2.35) Let’s proceed to the Hamiltonian formulation.2.2The Hamiltonian FormulationThe earlier expression forπab can be inverted to get∂g ab∂t =2Ngψ4 σab−1√6(trπ)2ψ12−gψ8 R−8▽2ψAs a consistency check let’sfind∂g ab∂t =2Ngψ4 σab−1∂t=−N√ψ−2N gψ4 πacπb c−16πab trπψ12+√gψ3 ▽a▽bψ+3g ab▽2ψ+4g ab√g▽(a(Nψ3)▽b)ψ+▽c πab N c −πbc▽c N a−πac▽c N b− πab−1∂tquite easily.(Of course,we need the evolution equations to propagate all of the constraints.We will deal with the others later.)Wefind that∂trp∂t =∂πab3∂g ab trπWorking through the details gives us∂σabgψ4 R ab−1ψ −2N gψ4σacσb c+√3g ab▽2(Nψ3)+N√3g ab▽2ψ(2.42)+4g ab√g▽(a(Nψ3)▽b)ψ+▽c σab N c −σbc▽c N a−σac▽c N b−σab▽cξc+Nψ8gσab trπ2.3Jacobi ActionWe can alsofind the Jacobi action of this theory.Recall the(3+1)Lagrangian,L=N√ψ+S ab S ab−2gψ4 N R−8▽2ψ4N ΣabΣab−21ψ−12(trβ)2 1ψ −13dλ √R−8▽2ψT d3x(2.46) where T= ΣabΣab−22.4Conformally Related SolutionsWe can do almost exactly the same thing here as we did in the section with the same name in Chapter1.Suppose we start with initial data{g ab,σab,trp}obeying the initial data conditions(2.33)and(2.34).We then solve(2.32)forψSuppose instead that we start with the conformally related initial data{h ab,ρab,trp}= {α4g ab,α−4σab,trp}.These automatically satisfy the initial data conditions by the con-formal invariance.We now solve the Hamiltonian constraint for the conformal“field”χ, say.Just like before it can be shown thatχ=ψ6(trπ)2− g R=0(2.49)▽b πab=0(2.50)▽c trπ=0(2.51)N R− ▽2 N+( trp)26(trπ)2−gR=0(2.53)▽bπab=0(2.54)▽c trπ=0(2.55) Evolution of the CMC condition givesNR−▽2N+(trp)22.4.1What ofξc?Precious little has been revealed about whatξc may be or even how it transforms.This needs to be addressed.First let’s recall that we demanded thattrB−→ω−8trB(2.57)under a conformal transformation.This will be enough to reveal the transformation properties ofξc.Taking the trace gives ustrB=−1∂t−g ab(KN)ab−3▽cξc(2.58)Under a conformal transformation we getω−8trB=−1∂t+12˙ω2ω2N g ab∂g ab2ω2N▽cξc+3ω3N ˙ω−ω,c N c=ω−2trB+3ω ˙ω−ω,c N c(2.59)Thus,3ω ˙ω−ω,c N c=−1ω ˙ω−ω,c N c−2N∂t =2 N g σab−1and∂ σab g R ab−1g ▽a ▽b N−13ω(˙ψ−ψ,c N c)−2Nψ(˙ψ−ψ,c N c)+2N3trB(1−ψ−6)(2.66)whereθis as in the original theory.Thus,the exact form ofξc is determined.We needed ▽cξc to be zero in the physical representation for constraint propagation and so we should check that this is the case with our newly found expression for▽cξc.We can check this easily.In the physical representationθ=0andψ=1.Thus,we do have that ▽c ξc is zero.It is vital to note that this is strictly a POST-VARIATION identification.If we use this form forξc in the action we will run into problems,not least an infinite sequence in the variation of trB with respect toξc.(This is because we would have trB defined in terms of trB itself.)We see thatξc is intimately related with howψchanges from slice to slice.Our constraints in the physical representation areσabσab−1。
火星基地的构想作文英语
火星基地的构想作文英语Title: Concept of a Mars Base。
In the grand scope of human exploration, Mars stands as the next frontier. The prospect of establishing a sustainable human presence on the Red Planet has captivated the imagination of scientists, engineers, and dreamers alike. This essay delves into the conceptualization of a Mars base, outlining its key components and the challenges that must be overcome.1. Location Selection:The first critical step in establishing a Mars base is selecting an appropriate location. Factors such as accessibility, resource availability, and scientific interest must be taken into account. Regions near the equator offer moderate temperatures and access to sunlight for solar power generation, while areas with subsurface water ice deposits could provide essential resources forlife support and fuel production.2. Habitat Modules:Habitats are essential for providing a safe and comfortable living environment for the crew. These modules must be radiation-shielded, airtight, and equipped with life support systems capable of recycling air and water. Advanced 3D printing technologies could be utilized to construct habitats using locally available materials, reducing the need for transporting bulky structures from Earth.3. Life Support Systems:Mars lacks a breathable atmosphere and abundant liquid water, necessitating the development of robust life support systems. Closed-loop systems capable of recycling water, generating oxygen, and removing carbon dioxide are essential for sustaining human life on Mars. Additionally, innovative agricultural techniques such as hydroponics and aeroponics could be employed to grow food in the harshMartian environment.4. Power Generation:Solar power is the primary source of energy for a Mars base due to the planet's abundant sunlight. However, dust storms and the planet's distance from the sun pose challenges to solar power generation. To mitigate these challenges, redundant solar arrays and energy storage systems must be employed. Furthermore, nuclear power systems could serve as a reliable backup source of energy, providing power during prolonged periods of darkness.5. Resource Utilization:In-situ resource utilization (ISRU) is key to the long-term sustainability of a Mars base. Water extracted from the Martian regolith can be electrolyzed to produce oxygen for breathing and hydrogen for fuel. Additionally, carbon dioxide in the atmosphere can be chemically processed to produce methane, which serves as a propellant for return missions to Earth and for powering surfacevehicles.6. Communication and Navigation:Reliable communication and navigation systems are essential for maintaining contact with Earth and forguiding exploration missions on Mars. Orbital relaysatellites can facilitate communication between the Mars base and Earth, while surface-based navigation systems such as GPS-like networks can assist in locating and mapping key landmarks on the Martian surface.7. Health and Well-being:The psychological and physiological well-being ofthe crew is paramount to the success of a Mars mission.Long-duration spaceflight can have detrimental effects on the human body, including muscle atrophy, bone density loss, and psychological stress. To address these challenges, comprehensive medical facilities, exercise equipment, and psychological support systems must be incorporated into the Mars base design.8. Exploration and Science:Beyond its role as a habitat for human settlers, a Mars base serves as a hub for scientific exploration and discovery. Robotic rovers, drones, and sample return missions can uncover the secrets of Mars' geology, climate history, and potential for past or present life. Furthermore, scientific research conducted on Mars can provide valuable insights into planetary formation and the potential for life beyond Earth.In conclusion, the conceptualization of a Mars base represents a monumental undertaking that requires interdisciplinary collaboration, technological innovation, and unwavering determination. While numerous challenges lie ahead, the prospect of establishing a sustainable human presence on Mars holds the promise of expanding our understanding of the universe and securing the future of humanity as a multi-planetary species.。
40人类如何通过自然科学理解宇宙
40人类如何通过自然科学理解宇宙Understanding the universe through the lens of natural science is a profound and awe-inspiring journey that has captivated human minds for centuries. It is a quest that transcends the boundaries of time and space, delving into the very fabric of existence. As we embark on this intellectual odyssey, we must approach it with a sense of humility and wonder, recognizing the vastness of the cosmos and our place within it.The first perspective we must consider is the historical evolution of our understanding of the universe. From the ancient Greeks, who believed in a geocentric model with Earth at the center, to the revolutionary ideas of Copernicus, who proposed a heliocentric model with the Sun at the center, our comprehension of the cosmos has undergone a radical transformation. This evolution is a testament to the power of human curiosity and the relentless pursuit of knowledge. It is a reminder that our understanding of the universe is not static but is constantly evolving as new evidence and theories emerge.The second perspective is the role of mathematics and physics in unraveling the mysteries of the universe. The laws of physics, such as Newton's laws of motion and Einstein's theory of relativity, have provided us with a framework to understand the behavior of celestial bodies and the forces that govern them. Mathematics, with its precision and elegance, has been instrumental in formulating these laws and predicting the outcomes of various phenomena. The interplay between mathematics and physics has not only deepened our understanding of the universe but has also inspired a sense of awe at the underlying order and harmony that pervades the cosmos.The third perspective is the exploration of the cosmos through observation and experimentation. The advent of the telescope and other observational tools has allowed us to peer into the depths of space, revealing the existence of distant galaxies, stars, and planets. The development of space probes and telescopes, such as the Hubble Space Telescope and the James Webb Space Telescope, has furtherexpanded our horizons, enabling us to study the universe in greater detail andwith greater accuracy. These technological advancements have not only broadenedour knowledge of the universe but have also instilled a sense of excitement and anticipation for the discoveries that lie ahead.The fourth perspective is the study of the origins and evolution of the universe. The Big Bang theory, which posits that the universe began as asingularity and has been expanding ever since, has become the prevailing explanation for the birth of the cosmos. This theory, along with the discovery of cosmic microwave background radiation, has provided compelling evidence for the origins of the universe. Furthermore, the study of the life cycles of stars, the formation of galaxies, and the distribution of matter in the universe has shedlight on the processes that have shaped the cosmos over time. This exploration of the universe's history has not only deepened our understanding of its evolutionbut has also sparked philosophical and existential questions about our place inthe grand scheme of things.The fifth perspective is the search for extraterrestrial life and the implications it holds for our understanding of the universe. The discovery of exoplanets and the ongoing search for signs of life beyond Earth have fueled our imagination and expanded our horizons. The possibility of life on other planets raises profound questions about the uniqueness of life on Earth and the potential diversity of life forms in the universe. This quest for extraterrestrial life is not only a scientific endeavor but also a reflection of our innate desire to connect with the cosmos and to seek out our place within it.The final perspective is the philosophical and emotional impact of our understanding of the universe. As we delve deeper into the mysteries of the cosmos, we are confronted with a sense of awe and wonder at the vastness and complexity of the universe. This exploration of the universe can evoke a range of emotions, from humility in the face of the cosmos's immensity to a sense of unity and interconnectedness with the universe. It can also inspire a sense ofresponsibility to protect and preserve our planet and the delicate balance of life within it.In conclusion, understanding the universe through natural science is a multifaceted and deeply enriching experience. It involves a historical perspective, the application of mathematics and physics, observational and experimental exploration, the study of the universe's origins and evolution, the search for extraterrestrial life, and the philosophical and emotional implications of our cosmic journey. As we continue to unravel the mysteries of the universe, we mustdo so with a sense of curiosity, humility, and wonder, recognizing the profound impact that our understanding of the cosmos has on our lives and our place within the grand tapestry of existence.。
2022年考研考博-考博英语-四川农业大学考试预测题精选专练VII(附带答案)卷4
2022年考研考博-考博英语-四川农业大学考试预测题精选专练VII(附带答案)第1套一.综合题(共25题)1.单选题According to new research of Prof. Randolf Menzel from the Free University in Berlin, the popular image of bees as the ultimate hard workers was inaccurate. “Although we see bees buzzing around tirelessly in spring and summer, the common belief in a bee’s busy nature is based on a misconception,” he said. People only really see bees when they’re out flying, or they look at a colony of bees and see thousands of them buzzing around. They don’t get to pick them out as individuals. The professor, who this month won a German Zoological Society award for his work on bees, added that bees compensated for their apparent laziness with high intelligence, advanced memory skills and an ability to learn quickly.The suggestion that bees were not pulling their weight met with skepticism from British beekeepers. Glyn Davies, the President of the British Beekeepers Association, said that bees were not lazy but efficient, “At any particular stage in its ener gy by doing nothing. Each bee has a unit of life energy and the faster it works, the faster it dies. They are being very wise and perhaps humans should try to follow their example instead of running about like headless chickens.”The idea of the busy bee is several thousand years old. One current author who has nothing but admiration for the bee is Paul Theroux, the novelist and part-time beekeeper.” I have never seen a bee sleeping. My bees never stop working,” he said. Mr. Theroux added that Prof. Menzel’s research could have been affected by his national origins. “Perhaps in comparison to the German rate of work, the bee does look lazy,” he said.Few people think that the busy bee idea will go away, despite the efforts of Prof. Menzel. It seems absurd to apply the word “lazy” to a colony of creatures capable of producing something so extraordinary as honeycomb. The truth is that bees give us an inferiority complexthat is not entirely unjustified. In fact, the worship of bees seems to be undergoing a renai ssance. IBM recently ran a series of ads drawing on the “waggle dance” of bees, telling businessmen to “make your business waggle.”1. Prof. Randolf Menzel’s latest research ______.2. Prof. Randolf Menzel would disagree that ______.3. According to Glyn Davies, what should we learn from bees?4. It could be inferred from Paragraph 3 that the Germans ______.5. The IBM ads in the passage are used to ______.问题1选项A.challenges our knowledge of the relations among beesB.confirms our knowledge of the relations among beesC.challenges our perception of the nature of beesD.confirms our perception of the nature of bees问题2选项A.bees are hardworkingB.bees are quick learnersC.bees have intelligenceD.bees have good memory问题3选项A.How to work faster.B.How to live longer.C.How to cooperate with each other.D.How to improve work efficiency.问题4选项A.are easily affected by their national charactersB.are extremely busy and hard workingC.have many things in common with beesD.tend to look down upon lazy people问题5选项A.show the popularity of the idea of busy beesB.emphasize the negative image of busy beesC.initiate public discussions on the busy bee imageD.question the comparison of busy bees to humans【答案】第1题:C第2题:A第3题:D第4题:B第5题:A【解析】1.推理判断题。
火箭对科技的影响英语作文
The advent and development of rocket technology have had a profound impact on the field of science and technology.Rockets,as a means of space exploration,have opened up new frontiers for humanity to understand and utilize space resources.Firstly,rocket technology has driven the advancement of aerospace engineering.The design and manufacturing of rockets require the integration of multiple disciplines, including aerodynamics,materials science,propulsion,and control systems.The development of rocket technology has promoted the progress of these fields and provided technical support for the aerospace industry.Secondly,rocket technology has facilitated the exploration of the universe.Rockets can carry satellites,probes,and manned spacecraft into space,enabling us to observe celestial bodies,study the origins of the universe,and search for extraterrestrial life.For instance, the Mars rovers sent by NASA have provided us with a wealth of information about the Martian environment and geological structure.Additionally,rocket technology has supported the development of communication technology.Geostationary satellites launched by rockets can provide global communication services,including television,telephone,and internet.This has made the world more closely connected and facilitated the dissemination and exchange of information.Furthermore,rocket technology has also contributed to the field of meteorology. Meteorological satellites can monitor weather changes and predict natural disasters, helping humans to respond to climate change and reduce the losses caused by natural disasters.In summary,rocket technology has had a significant impact on the field of science and technology.It not only promotes the development of aerospace engineering but also provides technical support for the exploration of the universe,the development of communication technology,and the advancement of meteorology.As rocket technology continues to evolve,it will bring more possibilities and opportunities to the field of science and technology.。
外刊话题-(大脑里有个定位系统)精校版
1.话题导读大脑里有个定位系统尤瓦尔·赫拉利在畅销书《未来简史》中写道:进入21世纪后,曾长期威胁人类生存和发展的瘟疫、饥荒和战争三大难题已被攻克,智人面临着新的待办议题:长生不老、幸福快乐和成为具有“神性”的人类。
其实,中国人追求长生不老由来已久,想想多少皇帝醉心于炼丹不可自拔,结果却因此而暴毙。
现代的人们在科学指导之下,知道了人的器官功能会不断老化,就像汽车零件一样不断磨损,最终无法使用。
然而,现在科学家却重新研究起长生不老,并且有越来越多的学术机构和私人公司加入进来。
这已不是个未来的产业了!本篇课程选自LeapsMag, an editorially independent online magazine2.外刊话题提要(选自The Economists Espresso)Navigating thoughts: spatial maps① Humans navigate the world by creating mental maps.① "Place" cells in the hippocampus pinpoint where we are; symmetrically-firing "grid" cells in the neighbouring entorhinal cortex give us spatial context.① In this week's Science, researchers hypothesise that the same system guides us through the process of thinking, too.① The brain organises information into cognitive spaces: large cats by their ferocity and size, say.① Studies show the system of place and grid cells is also active when it encodes new information.① Perhaps, then, this is how we navigate the knowledge stored in our minds.① Place cells mark how and where information is placed, grid cells code how close ideas are to one another.① In our cognitive space for animals, for example, jaguars will be closer to panthers than to elephants.① As the researchers used their own mental maps to conclude this, you're now thinking about thinking about thinking.① A little meta-cognition to start the weekend.①4句话总结文章内容1. Creating mental maps includes the action of place cells and grid cells.2. Place cells pinpoint where we are.3. Grid cells give us spatial context.4. Maybe we are using the same mental map system to guide our thoughts.3.生词好句①navigate /ˈnævɪɡeɪt/: vt. 引导;导航①spatial /ˈspeɪʃəl/: adj. 空间的①place cell: 位置细胞①hippocampus /ˌhɪpəˈkæmpəs/: n. 海马体①pinpoint /ˈpɪnpɔɪnt/: vt. 准确指出/确定(位置或时间)①grid cell: 网格细胞①entorhinal cortex /ˌentəˈraɪnəl/ /ˈkɔːteks, ˈkɔːrteks/: 内嗅皮层/皮质①context /ˈkɒntekst, ˈkɑːntekst/: n. 环境;背景①hypothesise /haɪˈpɒθəsaɪz, haɪˈpɑːθəsaɪz/: vt. 假设;假定①cognitive /ˈkɒɡnətɪv, ˈkɑːɡnətɪv/: adj. 认知的;感知的①ferocity /fəˈrɒsəti, fəˈrɑːsəti/: n. 凶残;猛烈。
科学思维发展史
科学思维发展史The evolution of scientific thinking is a fascinating journey that spans centuries and diverse cultures. It began with ancient philosophers, who pondered the nature of the universe and the origins of life. Over time, these inquiries gave way to more systematic approaches, leading to the emergence of the scientific method.科学思维的发展史是一段跨越世纪和多元文化的迷人旅程。
它始于古代的哲学家们,他们深思宇宙的本质和生命的起源。
随着时间的推移,这些探索逐渐转变为更为系统的方法,最终催生了科学方法的出现。
The Renaissance period marked a significant shift, as scholars began to embrace empirical observation and experimentation. This led to groundbreaking discoveries in areas such as astronomy, physics, and biology. The Scientific Revolution, spearheaded by figures like Isaac Newton and Galileo Galilei, further established the principles of rational inquiry and experimentation as the foundation of scientific knowledge.文艺复兴时期标志着一次重大的转变,学者们开始接受经验观察和实验。
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spatial coordinates ( ri , pi are independent variables). The p p F F is the force acting value v p p H Fr H Fr upon the particle. The conservative force FH eE ( r, t ) ( e / c )[v H ( r , t )] is determined by external fields and the fields of the particle beam ( div p FH 0 ), while FFr is the frictional force. That is why div p v p div p FFr , and the equation (1) can be presented in the integral form 0 exp[ div p FFrdt ] . The frictional force can be written in the form FFr Fr ( r, p, t ) n , where p | p | , n p / p , Fr (r , p, t ) is the frictional coefficient. In this case div p FFr Fr div p n n grad p Fr 2 Fr / p Fr / p . We took into account, that div p n 2 / p and n grad p Fr ( r , p, t ) = ( Fr / p ) vr ( Fr / ) , where p 2c 2 m 2 c 4 is the energy of the particle. The frictional power PFr F Fr v r Fr ( r, p, t ) n v r c Fr (r , p, t ) , where vr / c . It follows that Fr PFr (r , p, t ) / c , and the equation (1) become 0 exp[ 6 D (r , p, t ) dt ] , (2) where 6 D ( r, p, t ) div p FFr = 2 Fr / p + Fr / p or: 1 PFr (r , , t ) PFr (r , , t ) . 6 D (r , , t ) (1 2 )
d div v 0 . (1) dt Here components of the 6D velocity v (v r , v p ) are
x, y, z , px , p y , pz , where ri dri / dt , pi dpi / dt . The equation (1) or equivalent equation / t div ( v) 0 expresses the number of particles conservation law. In our case the form of the equation (1) is preferable as it presents the total derivation of the density in the coordinate system moving with the beam. It can be presented in the integral form 0 exp[ div(v)dt ] ,
THE EVOLUTION OF THE PHASE SPACE DENSITY OF PARTICLE BEAMS IN EXTERNAL FIELDS*
E.G.Bessonov, Lebedev Physical Institute of the Russian Academy of Sciences, Moscow, Russia Abstract
In this paper the evolution of the phase space density of particle beams in external fields is presented proceeding from the continuity equation in the six-dimensional (6D) phase space ( -space). Such a way the Robinson theorem, which includes the Liouville theorem as a special case, was proved in a more simple and consistent alternative way valid for arbitrary external fields, averaged fields of the beam (self-generated electromagnetic fields except intrabeam scattering) and arbitrary frictional forces (linear, nonlinear). It includes particle accelerators as a special case. The limits of the applicability of the Robinson theorem in case of cooling of excited ions having a finite living time are presented.
EVOLUTION OF PARTICLE BEAM DENSITY IN THE EXTERNAL ELECTROMAGNETIC FIELDS
Let us proceed from the continuity (Liouville’s) equation in the 6D phase space coordinate-momentum (r , p ) :
where 0 is the initial phase space density. The divergence div v divr v r div p v p , divr v r 0 as the velocity v r cp / p 2 m 2 c 2 does not depend on
The integral (2) along a trajectory of a particle is the solution of the equation (1). According to (2), the 6D rate of the beam density change is determined by the frictional power and its derivative with respect to the particle energy. The integral (2) is valid for the arbitrary systems (linear, nonlinear, coupled). We did not use a curvilinear coordinate system, the Jacobee’s formula for the system of linear differential equations, matrices; any additional conditions (see [3]). In our case the expression (2) is valid for the nonrelativistic case as well. In general case ( 6 D const ) the solution is not exponential function. The equation (2) is valid for infinitesimal parts of the beam. The damping of different parts of the beam in some methods of cooling should be distinguished. If PFr ( p ) 0 , then 6 D (r , p, t ) 0, d / d t 0 and, according to (2), we come to the Liouville’s theorem [4]– [7]. It states that for conservative systems the particle density in the 6D phase space, the number of particles in the phase space volume occupied by the beam and hence the volume stay constant. In this case the volume is named the 6D normalized emittance. The volume divided by the factor ( )3 is named the unnormalized emittance accordingly. The normalized emittance is invariant for conservative systems. 2D and 4D phase space volumes can be exchanged by conservative external fields. It follows from private examples (see e.g. [1]). Robinson and Liouville theorems are valid for identical particles (electrons, protons, muons and so on). The Robinson theorem is valid if frictional forces exist only at the moment of their interaction with media or external fields and there is no time delay between the interaction time and the frictional force. Excited ions have higher rest mass then unexcited ones and have finite lifetime. It means that in general case the above theorems are not valid for ion cooling (excited ions are not identical to unexcited ones and have finite lifetime). The theorems works well if the lifetime of excited ions is less then some characteristic time for the processes of the beam evolution determined by concrete conditions. E.g., in the case of particle accelerators the delay time between the moment of the ion excitation by a laser beam and following photon reemission must be less then the period of betatron oscillations. Otherwise, the additional cooling or heating of the ion beam is possible. It is supposed above that the particle beam is a continuous media (there is no free space between particles). On practice it means that the distance between particles is much less then dimensions of any instrument, which is used to move a particle from a peripheral region of the 6D volume of the beam to the central one and that the instrument do not disturb another particles of the beam (otherwise, the stochastic cooling is possible).