Control of chaos in Hamiltonian systems

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汉密尔顿原理

汉密尔顿原理

汉密尔顿原理The Hamiltonian principle, also known as Hamilton's principle, is a fundamental principle in classical mechanics. It states that the dynamics of a physical system are determined by a single function, known as the Hamiltonian. This principle was formulated by Sir William Rowan Hamilton in 1834 and is a powerful tool for understanding the behavior of a wide range of physical systems.汉密尔顿原理,也称为汉密尔顿原则,是古典力学中的基本原理。

它表明物理系统的动力学是由一个称为汉密尔顿量的单个函数所决定的。

这一原理是由威廉·罗恩·汉密尔顿爵士于1834年提出的,是理解各种物理系统行为的有力工具。

One of the key insights of the Hamiltonian principle is that it provides a more general formulation of the laws of motion than the standard Newtonian approach. While Newton's laws are suitable for describing the motion of simple, low-energy systems, the Hamiltonian approach can be applied to more complex systems, including those involving relativistic effects and quantum mechanics.汉密尔顿原理的一个关键见解是,它提供了比标准牛顿方法更一般的运动定律公式。

DYNAMICAL SYSTEMS, STABILITY, AND CHAOS

DYNAMICAL SYSTEMS, STABILITY, AND CHAOS

In this expository and resources chapter we review selected aspects of the mathematics of dynamical systems, stability, and chaos, within a historical framework that draws together two threads of its early development: celestial mechanics and control theory, and focussing on qualitative theory. From this perspective we show how concepts of stability enable us to classify dynamical equations and their solutions and connect the key issues of nonlinearity, bifurcation, control, and uncertainty that are common to time-dependent problems in natural and engineered systems. We discuss stability and bifurcations in three simple model problems, and conclude with a survey of recent extensions of stability theory to complex networks.
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Greek word for governor is kubernetes, from which the mathematician Norbert Wiener (1894–1964) coined the term cybernetics as a name for the collective field of automated control and information theory.

对混沌自适应控制的控制强度的讨论之二

对混沌自适应控制的控制强度的讨论之二

对混沌自适应控制的控制强度的讨论之二何花;赵泓【期刊名称】《计算机工程与设计》【年(卷),期】2001(022)002【摘要】文中对文献[1]提出的混沌自适应控制方法中给出的控制强度取值范围的计算方法作出了重要修改,指出了上文忽略的与控制矩阵的复数本征值λ±对应的控制强度,对离散系统只要满足|λ±|<1亦可控制混沌,且更有效。

其次指出对连续性系统仅考虑文献[1]给出的条件是不够的,控制强度还要满足λ±值的实部小于零,即微分方程的李雅普诺夫渐近稳定条件才能有效控制混沌。

%This paper make important correction for reference [1]. We point out it is more effective that the control stiffness is correspending to complex eigenvalue of the matrix introduced by linearizing the dynamic system, it can also control chaos when |λ±|<1 for discrete system. We point out it is ont enough for control chaos of continuous system that only consider the condition proved by reference [1], the control stiffness should accord with the condition of Re (|λ±|) <0.【总页数】4页(P70-73)【作者】何花;赵泓【作者单位】首都师范大学计算机系,物理系,;首都师范大学计算机系,物理系,【正文语种】中文【中图分类】O545;TP273.2【相关文献】1.电弧喷涂控制系统研究之二——系统控制参数优化及自适应控制设计 [J], 李鹤歧;李春旭;陈爱军2.超混沌Lorenz系统与超混沌Rossler系统的自适应控制同步 [J], 蒋楠3.基于自适应控制的八个混沌系统的多级组合同步 [J], 孙军伟; 李楠; 王延峰4.对混沌自适应控制方法的控制强度的讨论 [J], 赵泓;何花;沈京玲5.耦合时空混沌的模糊混沌神经网络鲁棒自适应控制 [J], 窦春霞;李鑫滨;袁石文因版权原因,仅展示原文概要,查看原文内容请购买。

一类混沌系统的状态量化反馈镇定控制器设计

一类混沌系统的状态量化反馈镇定控制器设计

一类混沌系统的状态量化反馈镇定控制器设计翟因虎;王银河;范永青【摘要】This paper investigates the asymptotical stabilization via state feedback for a class of chaotic systems with a quantizer connected on the input channel.The nonlinear terms in the dynamic equation of the chaotic system are represented as the homogeneous functions with arbitrary known orders.The quan-tizer has one adjustable time-varying parameter with the updated law to be designed, and thus it can quantify adaptively online the state variables of the chaotic systems according to control scheme.With the help of the updated law and adaptive law of estimated boundary error of quantization, the nonlinear adap-tive controller is proposed in this paper to ensure the chaotic system to be stabilized asymptotically in the presence of the quantizer.Finally, some simulation examples are utilized to demonstrate the validity of the results in this paper.%用状态反馈法对含量化器的一类混沌系统的渐进镇定进行了研究。

工商管理学院牛东晓,男,日生

工商管理学院牛东晓,男,日生

工商管理学院牛东晓,男,日生Prepared on 22 November 2020乞建勋,男,1946年10月生,汉族,现为华北电力大学工商管理学院教授,博士生导师。

乞建勋教授是我国技术经济预测与决策领域的专家,长期以来一直从数学的角度研究现代管理的新方法,尤其在网络计划管理与优化理论的研究中取得了突破性重大进展。

推导出了"机动时间定理"、"路长定理"、"非特征路线定理"等优化的基本定理,并利用这些定理解决了最低成本加快方法中的最大有效压缩量和群截面的求法,解决了各阶次关键路线的求法等一系列的网络计划优化的悬而未决的问题。

尤其是在近二三十年被国际一致公认的疑难问题--工序顺序排序优化问题上取得了重大突破,解决了常见的一些应用最广的特殊情况下的顺序优化问题,创造出了一套独特方法,为彻底解决该难题奠定了基础。

在国内外权威刊物上发表网络计划论文六十多篇,并由科学出版社出版了网络计划优化领域中第一部学术专着《网络计划优化新理论与技术经济决策》,在该领域的研究中达到国际先进水平。

兼任全国系统动力学学会理事、全国项目管理委员会委员、全国价值工程协会理事、《华北电力大学学报》编委、《价值工程》编委。

先后承担及主持的纵向、横向科研课题十余项。

其中一项为国家电力公司重大科研项目,一项获部级科技进步奖。

在2001-2006年间,电力管理与优化决策研究所承担了3项纵向课题:国家自然科学基金重大项目(),国家自然科学基金项目(),国家教育部博士点基金项目(008);横向课题17项。

其中《电厂大修的网络计划优化新理论及其软件开发》获得电力科学技术三等奖。

主要研究方向:优化理论与技术经济决策、技术经济评价理论与应用、电力经济管理。

牛东晓,男,1962年10月15日生,汉族,安徽宿县人,现任华北电力大学工商管理学院院长。

牛东晓教授是技术经济预测与决策领域的专家,致力于电力与经济系统中的预测与决策问题的研究,同时也开展电力工程建设项目技术经济评价的研究,曾获得中国电力科学技术二等奖、中国电力科学技术三等奖、国家教委科技进步三等奖、国家电力公司首届青年科技创新奖和河北省第三届青年科技奖等共6项省部级科技成果奖。

混沌控制英文翻译

混沌控制英文翻译

混沌控制:方法与应用B.R.Andrievskii和A.L.Fradkov俄罗斯科学院机械科学问题研究所,俄罗斯圣彼得堡,接收于2003年11月04日。

摘要:混沌的控制是最近十年被密集研究的一项课题,对它的的研究主要集中在应用方面,也即考虑其在不同的科学领域,如力学(控制的钟摆,梁、板、摩擦),物理(等离子体控制的动荡,激光,混沌,和传播的偶极子域),化学、生物学、生态学、经济学、医学、以及其他工程学如机械系统(控制vibroformers、微悬臂起重机、船),宇宙飞船,电气和电子系统,通信系统,信息系统,化学和加工工业中(信息流处理和自由流动物质的处理)的重要应用。

关键词:混沌,控制理论,科学应用,抑制混沌,工业应用。

1.引言在确定性混沌的概念渗透到科学文献的第一年,混沌的行为就被认为是一个奇特的现象,它或许只会出现在一个在实践中永远不会遇到的复杂数学运算中。

但是,后来,混沌运动现象被发现存在于许多系统力学、通信、激光和无线电物理(10、12、16、18、19),化学和生物化学[46]、[55]生物学,经济学(124,124),和药品领域。

在1997年和2002年之间有超过300篇发表在同行评议期刊的论文致力于研究混沌控制方法在多种情况下的应用。

在科学和技术领域如混沌流线物理过程,激光物理和光学、等离子体物理、分子和量子物理、力学、化学和电化学、生物学和生态学、经济学和财务、医学、机械工程、电气工程和化工、交通控制、通信与信息系统,混沌控制方法的问题一直都被积极探讨。

混沌控制在工程应用领域的实践证明了混沌的价值和混沌系统的控制方法在特定实际问题中的作用,也起码证明了混沌控制应用的可行性。

但是,混沌在科学领域的应用(在物理、化学或生物学),主要是朝向发现物理(化学、生物)系统行为中的新属性和规律的控制理论和方法方面发展,而不是特定的应用。

他们经常利用简单的模型描述被研究的系统。

科学应用2.1.机械系统混沌控制应用钟摆,梁和盘中的混沌控制。

哈密顿 拉格朗日 多体系统动力学

哈密顿 拉格朗日 多体系统动力学

哈密顿拉格朗日多体系统动力学(中英文实用版)Title: Hamilton and Lagrange Multibody System DynamicsHamilton"s mechanics and Lagrange"s equations are two essential frameworks in the field of multibody system dynamics.They provide a mathematical description of the motion of systems composed of multiple interacting particles or bodies.Hamilton"s mechanics, formulated by William Rowan Hamilton in the early 19th century, is based on the principle of least action.It provides a comprehensive framework for describing the dynamics of systems with a wide range of complexity, from simple mechanical systems to celestial mechanics and quantum mechanics.In Hamilton"s mechanics, the equations of motion are derived from the action principle, which states that the actual path of a system is the one that minimizes the action, a functional that depends on the configuration and time evolution of the system.In Chinese, Hamilton mechanics, formulated by William Rowan Hamilton in the early 19th century, is based on the principle of least action.It provides a comprehensive framework for describing the dynamics of systems with a wide range of complexity, from simple mechanical systems to celestial mechanics and quantum mechanics.In Hamilton"s mechanics, the equations of motion are derived from theaction principle, which states that the actual path of a system is the one that minimizes the action, a functional that depends on the configuration and time evolution of the system.Lagrange"s equations, on the other hand, were formulated by Joseph-Louis Lagrange in the mid-18th century.They provide an alternative approach to the study of dynamic systems, focusing on the conservation of grange"s equations are derived from the principle of virtual work, which states that the actual motion of a system is the one that minimizes the potential energy of the system.In Lagrange"s framework, the equations of motion are expressed in terms of generalized coordinates and their derivatives, which represent the configuration and time evolution of the system.In contrast to Hamilton"s mechanics, Lagrange"s equations focus on the conservation of energy.They were formulated by Joseph-Louis Lagrange in the mid-18th century.In Lagrange"s framework, the equations of motion are expressed in terms of generalized coordinates and their derivatives, which represent the configuration and time evolution of the system.The principle of virtual work underlies Lagrange"s equations, stating that the actual motion of a system is the one that minimizes the potential energy of the system.Both Hamilton"s and Lagrange"s frameworks are widely used in the study of multibody system dynamics.They provide powerful tools foranalyzing the motion of complex systems, such as robotic arms, vehicles, and biological organisms.By employing these frameworks, researchers and engineers can accurately predict the behavior of these systems under various conditions and design optimal control strategies for their operation.In summary, Hamilton"s and Lagrange"s mechanics are two complementary frameworks that play a crucial role in the analysis of multibody system dynamics.They provide a mathematical description of the motion of systems composed of multiple interacting particles or bodies, allowing for the study and optimization of complex dynamic systems.。

物理学专业英语

物理学专业英语

华中师范大学物理学院物理学专业英语仅供内部学习参考!2014一、课程的任务和教学目的通过学习《物理学专业英语》,学生将掌握物理学领域使用频率较高的专业词汇和表达方法,进而具备基本的阅读理解物理学专业文献的能力。

通过分析《物理学专业英语》课程教材中的范文,学生还将从英语角度理解物理学中个学科的研究内容和主要思想,提高学生的专业英语能力和了解物理学研究前沿的能力。

培养专业英语阅读能力,了解科技英语的特点,提高专业外语的阅读质量和阅读速度;掌握一定量的本专业英文词汇,基本达到能够独立完成一般性本专业外文资料的阅读;达到一定的笔译水平。

要求译文通顺、准确和专业化。

要求译文通顺、准确和专业化。

二、课程内容课程内容包括以下章节:物理学、经典力学、热力学、电磁学、光学、原子物理、统计力学、量子力学和狭义相对论三、基本要求1.充分利用课内时间保证充足的阅读量(约1200~1500词/学时),要求正确理解原文。

2.泛读适量课外相关英文读物,要求基本理解原文主要内容。

3.掌握基本专业词汇(不少于200词)。

4.应具有流利阅读、翻译及赏析专业英语文献,并能简单地进行写作的能力。

四、参考书目录1 Physics 物理学 (1)Introduction to physics (1)Classical and modern physics (2)Research fields (4)V ocabulary (7)2 Classical mechanics 经典力学 (10)Introduction (10)Description of classical mechanics (10)Momentum and collisions (14)Angular momentum (15)V ocabulary (16)3 Thermodynamics 热力学 (18)Introduction (18)Laws of thermodynamics (21)System models (22)Thermodynamic processes (27)Scope of thermodynamics (29)V ocabulary (30)4 Electromagnetism 电磁学 (33)Introduction (33)Electrostatics (33)Magnetostatics (35)Electromagnetic induction (40)V ocabulary (43)5 Optics 光学 (45)Introduction (45)Geometrical optics (45)Physical optics (47)Polarization (50)V ocabulary (51)6 Atomic physics 原子物理 (52)Introduction (52)Electronic configuration (52)Excitation and ionization (56)V ocabulary (59)7 Statistical mechanics 统计力学 (60)Overview (60)Fundamentals (60)Statistical ensembles (63)V ocabulary (65)8 Quantum mechanics 量子力学 (67)Introduction (67)Mathematical formulations (68)Quantization (71)Wave-particle duality (72)Quantum entanglement (75)V ocabulary (77)9 Special relativity 狭义相对论 (79)Introduction (79)Relativity of simultaneity (80)Lorentz transformations (80)Time dilation and length contraction (81)Mass-energy equivalence (82)Relativistic energy-momentum relation (86)V ocabulary (89)正文标记说明:蓝色Arial字体(例如energy):已知的专业词汇蓝色Arial字体加下划线(例如electromagnetism):新学的专业词汇黑色Times New Roman字体加下划线(例如postulate):新学的普通词汇1 Physics 物理学1 Physics 物理学Introduction to physicsPhysics is a part of natural philosophy and a natural science that involves the study of matter and its motion through space and time, along with related concepts such as energy and force. More broadly, it is the general analysis of nature, conducted in order to understand how the universe behaves.Physics is one of the oldest academic disciplines, perhaps the oldest through its inclusion of astronomy. Over the last two millennia, physics was a part of natural philosophy along with chemistry, certain branches of mathematics, and biology, but during the Scientific Revolution in the 17th century, the natural sciences emerged as unique research programs in their own right. Physics intersects with many interdisciplinary areas of research, such as biophysics and quantum chemistry,and the boundaries of physics are not rigidly defined. New ideas in physics often explain the fundamental mechanisms of other sciences, while opening new avenues of research in areas such as mathematics and philosophy.Physics also makes significant contributions through advances in new technologies that arise from theoretical breakthroughs. For example, advances in the understanding of electromagnetism or nuclear physics led directly to the development of new products which have dramatically transformed modern-day society, such as television, computers, domestic appliances, and nuclear weapons; advances in thermodynamics led to the development of industrialization; and advances in mechanics inspired the development of calculus.Core theoriesThough physics deals with a wide variety of systems, certain theories are used by all physicists. Each of these theories were experimentally tested numerous times and found correct as an approximation of nature (within a certain domain of validity).For instance, the theory of classical mechanics accurately describes the motion of objects, provided they are much larger than atoms and moving at much less than the speed of light. These theories continue to be areas of active research, and a remarkable aspect of classical mechanics known as chaos was discovered in the 20th century, three centuries after the original formulation of classical mechanics by Isaac Newton (1642–1727) 【艾萨克·牛顿】.University PhysicsThese central theories are important tools for research into more specialized topics, and any physicist, regardless of his or her specialization, is expected to be literate in them. These include classical mechanics, quantum mechanics, thermodynamics and statistical mechanics, electromagnetism, and special relativity.Classical and modern physicsClassical mechanicsClassical physics includes the traditional branches and topics that were recognized and well-developed before the beginning of the 20th century—classical mechanics, acoustics, optics, thermodynamics, and electromagnetism.Classical mechanics is concerned with bodies acted on by forces and bodies in motion and may be divided into statics (study of the forces on a body or bodies at rest), kinematics (study of motion without regard to its causes), and dynamics (study of motion and the forces that affect it); mechanics may also be divided into solid mechanics and fluid mechanics (known together as continuum mechanics), the latter including such branches as hydrostatics, hydrodynamics, aerodynamics, and pneumatics.Acoustics is the study of how sound is produced, controlled, transmitted and received. Important modern branches of acoustics include ultrasonics, the study of sound waves of very high frequency beyond the range of human hearing; bioacoustics the physics of animal calls and hearing, and electroacoustics, the manipulation of audible sound waves using electronics.Optics, the study of light, is concerned not only with visible light but also with infrared and ultraviolet radiation, which exhibit all of the phenomena of visible light except visibility, e.g., reflection, refraction, interference, diffraction, dispersion, and polarization of light.Heat is a form of energy, the internal energy possessed by the particles of which a substance is composed; thermodynamics deals with the relationships between heat and other forms of energy.Electricity and magnetism have been studied as a single branch of physics since the intimate connection between them was discovered in the early 19th century; an electric current gives rise to a magnetic field and a changing magnetic field induces an electric current. Electrostatics deals with electric charges at rest, electrodynamics with moving charges, and magnetostatics with magnetic poles at rest.Modern PhysicsClassical physics is generally concerned with matter and energy on the normal scale of1 Physics 物理学observation, while much of modern physics is concerned with the behavior of matter and energy under extreme conditions or on the very large or very small scale.For example, atomic and nuclear physics studies matter on the smallest scale at which chemical elements can be identified.The physics of elementary particles is on an even smaller scale, as it is concerned with the most basic units of matter; this branch of physics is also known as high-energy physics because of the extremely high energies necessary to produce many types of particles in large particle accelerators. On this scale, ordinary, commonsense notions of space, time, matter, and energy are no longer valid.The two chief theories of modern physics present a different picture of the concepts of space, time, and matter from that presented by classical physics.Quantum theory is concerned with the discrete, rather than continuous, nature of many phenomena at the atomic and subatomic level, and with the complementary aspects of particles and waves in the description of such phenomena.The theory of relativity is concerned with the description of phenomena that take place in a frame of reference that is in motion with respect to an observer; the special theory of relativity is concerned with relative uniform motion in a straight line and the general theory of relativity with accelerated motion and its connection with gravitation.Both quantum theory and the theory of relativity find applications in all areas of modern physics.Difference between classical and modern physicsWhile physics aims to discover universal laws, its theories lie in explicit domains of applicability. Loosely speaking, the laws of classical physics accurately describe systems whose important length scales are greater than the atomic scale and whose motions are much slower than the speed of light. Outside of this domain, observations do not match their predictions.Albert Einstein【阿尔伯特·爱因斯坦】contributed the framework of special relativity, which replaced notions of absolute time and space with space-time and allowed an accurate description of systems whose components have speeds approaching the speed of light.Max Planck【普朗克】, Erwin Schrödinger【薛定谔】, and others introduced quantum mechanics, a probabilistic notion of particles and interactions that allowed an accurate description of atomic and subatomic scales.Later, quantum field theory unified quantum mechanics and special relativity.General relativity allowed for a dynamical, curved space-time, with which highly massiveUniversity Physicssystems and the large-scale structure of the universe can be well-described. General relativity has not yet been unified with the other fundamental descriptions; several candidate theories of quantum gravity are being developed.Research fieldsContemporary research in physics can be broadly divided into condensed matter physics; atomic, molecular, and optical physics; particle physics; astrophysics; geophysics and biophysics. Some physics departments also support research in Physics education.Since the 20th century, the individual fields of physics have become increasingly specialized, and today most physicists work in a single field for their entire careers. "Universalists" such as Albert Einstein (1879–1955) and Lev Landau (1908–1968)【列夫·朗道】, who worked in multiple fields of physics, are now very rare.Condensed matter physicsCondensed matter physics is the field of physics that deals with the macroscopic physical properties of matter. In particular, it is concerned with the "condensed" phases that appear whenever the number of particles in a system is extremely large and the interactions between them are strong.The most familiar examples of condensed phases are solids and liquids, which arise from the bonding by way of the electromagnetic force between atoms. More exotic condensed phases include the super-fluid and the Bose–Einstein condensate found in certain atomic systems at very low temperature, the superconducting phase exhibited by conduction electrons in certain materials,and the ferromagnetic and antiferromagnetic phases of spins on atomic lattices.Condensed matter physics is by far the largest field of contemporary physics.Historically, condensed matter physics grew out of solid-state physics, which is now considered one of its main subfields. The term condensed matter physics was apparently coined by Philip Anderson when he renamed his research group—previously solid-state theory—in 1967. In 1978, the Division of Solid State Physics of the American Physical Society was renamed as the Division of Condensed Matter Physics.Condensed matter physics has a large overlap with chemistry, materials science, nanotechnology and engineering.Atomic, molecular and optical physicsAtomic, molecular, and optical physics (AMO) is the study of matter–matter and light–matter interactions on the scale of single atoms and molecules.1 Physics 物理学The three areas are grouped together because of their interrelationships, the similarity of methods used, and the commonality of the energy scales that are relevant. All three areas include both classical, semi-classical and quantum treatments; they can treat their subject from a microscopic view (in contrast to a macroscopic view).Atomic physics studies the electron shells of atoms. Current research focuses on activities in quantum control, cooling and trapping of atoms and ions, low-temperature collision dynamics and the effects of electron correlation on structure and dynamics. Atomic physics is influenced by the nucleus (see, e.g., hyperfine splitting), but intra-nuclear phenomena such as fission and fusion are considered part of high-energy physics.Molecular physics focuses on multi-atomic structures and their internal and external interactions with matter and light.Optical physics is distinct from optics in that it tends to focus not on the control of classical light fields by macroscopic objects, but on the fundamental properties of optical fields and their interactions with matter in the microscopic realm.High-energy physics (particle physics) and nuclear physicsParticle physics is the study of the elementary constituents of matter and energy, and the interactions between them.In addition, particle physicists design and develop the high energy accelerators,detectors, and computer programs necessary for this research. The field is also called "high-energy physics" because many elementary particles do not occur naturally, but are created only during high-energy collisions of other particles.Currently, the interactions of elementary particles and fields are described by the Standard Model.●The model accounts for the 12 known particles of matter (quarks and leptons) thatinteract via the strong, weak, and electromagnetic fundamental forces.●Dynamics are described in terms of matter particles exchanging gauge bosons (gluons,W and Z bosons, and photons, respectively).●The Standard Model also predicts a particle known as the Higgs boson. In July 2012CERN, the European laboratory for particle physics, announced the detection of a particle consistent with the Higgs boson.Nuclear Physics is the field of physics that studies the constituents and interactions of atomic nuclei. The most commonly known applications of nuclear physics are nuclear power generation and nuclear weapons technology, but the research has provided application in many fields, including those in nuclear medicine and magnetic resonance imaging, ion implantation in materials engineering, and radiocarbon dating in geology and archaeology.University PhysicsAstrophysics and Physical CosmologyAstrophysics and astronomy are the application of the theories and methods of physics to the study of stellar structure, stellar evolution, the origin of the solar system, and related problems of cosmology. Because astrophysics is a broad subject, astrophysicists typically apply many disciplines of physics, including mechanics, electromagnetism, statistical mechanics, thermodynamics, quantum mechanics, relativity, nuclear and particle physics, and atomic and molecular physics.The discovery by Karl Jansky in 1931 that radio signals were emitted by celestial bodies initiated the science of radio astronomy. Most recently, the frontiers of astronomy have been expanded by space exploration. Perturbations and interference from the earth's atmosphere make space-based observations necessary for infrared, ultraviolet, gamma-ray, and X-ray astronomy.Physical cosmology is the study of the formation and evolution of the universe on its largest scales. Albert Einstein's theory of relativity plays a central role in all modern cosmological theories. In the early 20th century, Hubble's discovery that the universe was expanding, as shown by the Hubble diagram, prompted rival explanations known as the steady state universe and the Big Bang.The Big Bang was confirmed by the success of Big Bang nucleo-synthesis and the discovery of the cosmic microwave background in 1964. The Big Bang model rests on two theoretical pillars: Albert Einstein's general relativity and the cosmological principle (On a sufficiently large scale, the properties of the Universe are the same for all observers). Cosmologists have recently established the ΛCDM model (the standard model of Big Bang cosmology) of the evolution of the universe, which includes cosmic inflation, dark energy and dark matter.Current research frontiersIn condensed matter physics, an important unsolved theoretical problem is that of high-temperature superconductivity. Many condensed matter experiments are aiming to fabricate workable spintronics and quantum computers.In particle physics, the first pieces of experimental evidence for physics beyond the Standard Model have begun to appear. Foremost among these are indications that neutrinos have non-zero mass. These experimental results appear to have solved the long-standing solar neutrino problem, and the physics of massive neutrinos remains an area of active theoretical and experimental research. Particle accelerators have begun probing energy scales in the TeV range, in which experimentalists are hoping to find evidence for the super-symmetric particles, after discovery of the Higgs boson.Theoretical attempts to unify quantum mechanics and general relativity into a single theory1 Physics 物理学of quantum gravity, a program ongoing for over half a century, have not yet been decisively resolved. The current leading candidates are M-theory, superstring theory and loop quantum gravity.Many astronomical and cosmological phenomena have yet to be satisfactorily explained, including the existence of ultra-high energy cosmic rays, the baryon asymmetry, the acceleration of the universe and the anomalous rotation rates of galaxies.Although much progress has been made in high-energy, quantum, and astronomical physics, many everyday phenomena involving complexity, chaos, or turbulence are still poorly understood. Complex problems that seem like they could be solved by a clever application of dynamics and mechanics remain unsolved; examples include the formation of sand-piles, nodes in trickling water, the shape of water droplets, mechanisms of surface tension catastrophes, and self-sorting in shaken heterogeneous collections.These complex phenomena have received growing attention since the 1970s for several reasons, including the availability of modern mathematical methods and computers, which enabled complex systems to be modeled in new ways. Complex physics has become part of increasingly interdisciplinary research, as exemplified by the study of turbulence in aerodynamics and the observation of pattern formation in biological systems.Vocabulary★natural science 自然科学academic disciplines 学科astronomy 天文学in their own right 凭他们本身的实力intersects相交,交叉interdisciplinary交叉学科的,跨学科的★quantum 量子的theoretical breakthroughs 理论突破★electromagnetism 电磁学dramatically显著地★thermodynamics热力学★calculus微积分validity★classical mechanics 经典力学chaos 混沌literate 学者★quantum mechanics量子力学★thermodynamics and statistical mechanics热力学与统计物理★special relativity狭义相对论is concerned with 关注,讨论,考虑acoustics 声学★optics 光学statics静力学at rest 静息kinematics运动学★dynamics动力学ultrasonics超声学manipulation 操作,处理,使用University Physicsinfrared红外ultraviolet紫外radiation辐射reflection 反射refraction 折射★interference 干涉★diffraction 衍射dispersion散射★polarization 极化,偏振internal energy 内能Electricity电性Magnetism 磁性intimate 亲密的induces 诱导,感应scale尺度★elementary particles基本粒子★high-energy physics 高能物理particle accelerators 粒子加速器valid 有效的,正当的★discrete离散的continuous 连续的complementary 互补的★frame of reference 参照系★the special theory of relativity 狭义相对论★general theory of relativity 广义相对论gravitation 重力,万有引力explicit 详细的,清楚的★quantum field theory 量子场论★condensed matter physics凝聚态物理astrophysics天体物理geophysics地球物理Universalist博学多才者★Macroscopic宏观Exotic奇异的★Superconducting 超导Ferromagnetic铁磁质Antiferromagnetic 反铁磁质★Spin自旋Lattice 晶格,点阵,网格★Society社会,学会★microscopic微观的hyperfine splitting超精细分裂fission分裂,裂变fusion熔合,聚变constituents成分,组分accelerators加速器detectors 检测器★quarks夸克lepton 轻子gauge bosons规范玻色子gluons胶子★Higgs boson希格斯玻色子CERN欧洲核子研究中心★Magnetic Resonance Imaging磁共振成像,核磁共振ion implantation 离子注入radiocarbon dating放射性碳年代测定法geology地质学archaeology考古学stellar 恒星cosmology宇宙论celestial bodies 天体Hubble diagram 哈勃图Rival竞争的★Big Bang大爆炸nucleo-synthesis核聚合,核合成pillar支柱cosmological principle宇宙学原理ΛCDM modelΛ-冷暗物质模型cosmic inflation宇宙膨胀1 Physics 物理学fabricate制造,建造spintronics自旋电子元件,自旋电子学★neutrinos 中微子superstring 超弦baryon重子turbulence湍流,扰动,骚动catastrophes突变,灾变,灾难heterogeneous collections异质性集合pattern formation模式形成University Physics2 Classical mechanics 经典力学IntroductionIn physics, classical mechanics is one of the two major sub-fields of mechanics, which is concerned with the set of physical laws describing the motion of bodies under the action of a system of forces. The study of the motion of bodies is an ancient one, making classical mechanics one of the oldest and largest subjects in science, engineering and technology.Classical mechanics describes the motion of macroscopic objects, from projectiles to parts of machinery, as well as astronomical objects, such as spacecraft, planets, stars, and galaxies. Besides this, many specializations within the subject deal with gases, liquids, solids, and other specific sub-topics.Classical mechanics provides extremely accurate results as long as the domain of study is restricted to large objects and the speeds involved do not approach the speed of light. When the objects being dealt with become sufficiently small, it becomes necessary to introduce the other major sub-field of mechanics, quantum mechanics, which reconciles the macroscopic laws of physics with the atomic nature of matter and handles the wave–particle duality of atoms and molecules. In the case of high velocity objects approaching the speed of light, classical mechanics is enhanced by special relativity. General relativity unifies special relativity with Newton's law of universal gravitation, allowing physicists to handle gravitation at a deeper level.The initial stage in the development of classical mechanics is often referred to as Newtonian mechanics, and is associated with the physical concepts employed by and the mathematical methods invented by Newton himself, in parallel with Leibniz【莱布尼兹】, and others.Later, more abstract and general methods were developed, leading to reformulations of classical mechanics known as Lagrangian mechanics and Hamiltonian mechanics. These advances were largely made in the 18th and 19th centuries, and they extend substantially beyond Newton's work, particularly through their use of analytical mechanics. Ultimately, the mathematics developed for these were central to the creation of quantum mechanics.Description of classical mechanicsThe following introduces the basic concepts of classical mechanics. For simplicity, it often2 Classical mechanics 经典力学models real-world objects as point particles, objects with negligible size. The motion of a point particle is characterized by a small number of parameters: its position, mass, and the forces applied to it.In reality, the kind of objects that classical mechanics can describe always have a non-zero size. (The physics of very small particles, such as the electron, is more accurately described by quantum mechanics). Objects with non-zero size have more complicated behavior than hypothetical point particles, because of the additional degrees of freedom—for example, a baseball can spin while it is moving. However, the results for point particles can be used to study such objects by treating them as composite objects, made up of a large number of interacting point particles. The center of mass of a composite object behaves like a point particle.Classical mechanics uses common-sense notions of how matter and forces exist and interact. It assumes that matter and energy have definite, knowable attributes such as where an object is in space and its speed. It also assumes that objects may be directly influenced only by their immediate surroundings, known as the principle of locality.In quantum mechanics objects may have unknowable position or velocity, or instantaneously interact with other objects at a distance.Position and its derivativesThe position of a point particle is defined with respect to an arbitrary fixed reference point, O, in space, usually accompanied by a coordinate system, with the reference point located at the origin of the coordinate system. It is defined as the vector r from O to the particle.In general, the point particle need not be stationary relative to O, so r is a function of t, the time elapsed since an arbitrary initial time.In pre-Einstein relativity (known as Galilean relativity), time is considered an absolute, i.e., the time interval between any given pair of events is the same for all observers. In addition to relying on absolute time, classical mechanics assumes Euclidean geometry for the structure of space.Velocity and speedThe velocity, or the rate of change of position with time, is defined as the derivative of the position with respect to time. In classical mechanics, velocities are directly additive and subtractive as vector quantities; they must be dealt with using vector analysis.When both objects are moving in the same direction, the difference can be given in terms of speed only by ignoring direction.University PhysicsAccelerationThe acceleration , or rate of change of velocity, is the derivative of the velocity with respect to time (the second derivative of the position with respect to time).Acceleration can arise from a change with time of the magnitude of the velocity or of the direction of the velocity or both . If only the magnitude v of the velocity decreases, this is sometimes referred to as deceleration , but generally any change in the velocity with time, including deceleration, is simply referred to as acceleration.Inertial frames of referenceWhile the position and velocity and acceleration of a particle can be referred to any observer in any state of motion, classical mechanics assumes the existence of a special family of reference frames in terms of which the mechanical laws of nature take a comparatively simple form. These special reference frames are called inertial frames .An inertial frame is such that when an object without any force interactions (an idealized situation) is viewed from it, it appears either to be at rest or in a state of uniform motion in a straight line. This is the fundamental definition of an inertial frame. They are characterized by the requirement that all forces entering the observer's physical laws originate in identifiable sources (charges, gravitational bodies, and so forth).A non-inertial reference frame is one accelerating with respect to an inertial one, and in such a non-inertial frame a particle is subject to acceleration by fictitious forces that enter the equations of motion solely as a result of its accelerated motion, and do not originate in identifiable sources. These fictitious forces are in addition to the real forces recognized in an inertial frame.A key concept of inertial frames is the method for identifying them. For practical purposes, reference frames that are un-accelerated with respect to the distant stars are regarded as good approximations to inertial frames.Forces; Newton's second lawNewton was the first to mathematically express the relationship between force and momentum . Some physicists interpret Newton's second law of motion as a definition of force and mass, while others consider it a fundamental postulate, a law of nature. Either interpretation has the same mathematical consequences, historically known as "Newton's Second Law":a m t v m t p F ===d )(d d dThe quantity m v is called the (canonical ) momentum . The net force on a particle is thus equal to rate of change of momentum of the particle with time.So long as the force acting on a particle is known, Newton's second law is sufficient to。

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a r X i v :n l i n /0311009v 1 [n l i n .C D ] 6 N o v 2003Control of chaos in Hamiltonian systemsG.CiraoloFacolt`a di Ingegneria,Universit`a di Firenze,via S.Marta,I-50129Firenze,Italy,I.N.F.N.Sezione di Firenze and I.N.F.M.UdR FirenzeC.Chandre,R.Lima,M.VittotCPT-CNRS,Luminy Case 907,F-13288Marseille Cedex 9,FranceM.PettiniIstituto Nazionale di Astrofisica,Osservatorio Astrofisico di Arcetri,Largo Enrico Fermi 5,I-50125Firenze,Italy,and I.N.F.M.UdR FirenzeWe present a technique to control chaos in Hamiltonian systems which are close to integrable.By adding a small and simple control term to the perturbation,the system becomes more regular than the original one.We apply this technique to a forced pendulum model and show numerically that the control is able to drastically reduced chaos.I.INTRODUCTIONIn this article,the problem we address is how to control chaos in Hamiltonian systems which are close to integrable.We consider the class of Hamiltonian systems that can be written in the form H =H 0+ǫV that is an integrable Hamiltonian H 0(with action-angle variables)plus a small perturbation ǫV .The problem of control in Hamiltonian systems is the following one:For the perturbed Hamiltonian H 0+ǫV ,the aim is to devise a control term f such that the dynamics of the controlled Hamiltonian H 0+ǫV +f has more regular trajectories (e.g.on invariant tori)or less diffusion than the uncontrolled one.In practice,we do not require that the controlled Hamiltonian is integrable since it is a too strong requirement,but only that it has a more regular behavior than the original system.Obviously f =−ǫV is a solution since the resulting Hamiltonian is integrable.However,it is a useless solution since the control is of the same order as the perturbation.For practical purposes,the desired control term should be small (with respect to the perturbation ǫV ),localized in phase space (meaning that the subset of phase space where f is non-zero is finite or small enough),or f should be of a specific shape (e.g.a sum of given Fourier modes,or with a certain regularity).Moreover,the control should be as simple as possible in order to be implemented in experiments.Therefore,the control appears to be a trade-offbetween the requirement on the reduction of chaos and the requirement on the simplicity of the control.In this article,we provide an algorithm for finding a control term f of order O (ǫ2)such that H =H 0+ǫV +f is integrable.This control term is expressed as a series whose terms can be explicitly and easily computed by recursion.It is shown on an example that truncations and approximations of this control term f provides a simple and easy way to control the system.II.CONTROL THEORY OF HAMILTONIAN SYSTEMS.In this section,we follow the exposition of control theory developed in Ref.[8].Let A be the algebra of real functions defined on phase space.For H ∈A ,let {H }be the linear operator acting on A such that{H }H ′={H,H ′},for any H ′∈A ,where {·,·}is the Poisson bracket.The time-evolution of a function V ∈A following the flow of H is given bydVif H is time independent,and wheree t{H}=∞ n=0t n∂A·∂H′∂ϕ·∂H′∂A.A possible choice ofΓisΓV(A,ϕ)= k∈Z nω(A)·k=0V k(A)We notice that this choice ofΓcommutes with{H0}.For a given V∈A,R V is the resonant part of V and N V is the non-resonant part:R V= k V k(A)χ(ω(A)·k=0)e i k·ϕ,(2)N V= k V k(A)χ(ω(A)·k=0)e i k·ϕ,(3) whereχ(α)vanishes when propositionαis wrong and it is equal to1whenαis true.From these operators defined for the integrable part H0,we construct a control term for the perturbed Hamiltonian H0+V where V∈A,i.e.we construct f such that H0+V+f is canonically conjugate to H0+R V.Proposition1:For V∈A andΓconstructed from H0,we have the following equatione{ΓV}(H0+V+f)=H0+R V,(4) wheref(V)=e−{ΓV}R V+1−e−{ΓV}{ΓV}=∞ n=0(−1)n(n+1)!{ΓV}n(n R+1)V.(6) We notice that if V is of orderǫ,f(V)is of orderǫ2.Proposition1tells that the addition of a well chosen control term f makes the Hamiltonian canonically conjugate to H0+R V.Proposition2:Theflow of H0+V+f is conjugate to theflow of H0+R V:∀t∈R,e t{H0+V+f}=e−{ΓV}e t{H0}e t{R V}e{ΓV}.The remarkable fact is that theflow of R V commutes with the one of H0,since{H0}R=0.This allows the splitting of theflow of H0+R V into a product.We recall that H0is non-resonant iff∀A∈B,χ(ω(A)·k=0)=χ(k=0).If H0is non-resonant then with the addition of a control term f,the Hamiltonian H0+V+f is canonically conjugate to the integrable Hamiltonian H0+R V since R V is only a function of the actions[see Eq.(2)].If H0is resonant and R V=0,the controlled Hamiltonian H=H0+V+f is conjugate to H0.In the case R V=0,the series(6)which gives the expansion of the control term f,can be written asf(V)=∞s=2f s,(7)where f s is of orderǫs and given by the recursion formulaf s=−1Remark:A similar approach of control has been developed by G.Gallavotti in Refs.[4,5,6].The idea is tofind a control term(named counterterm)only depending on the actions,i.e.tofind N such thatH(A,ϕ)=H0(A)+V(A,ϕ)−N(A)is integrable.For isochronous systems,that isH0(A)=ω·Ait is shown that if the frequency vector satisfies a Diophantine condition and if the perturbation is sufficiently small and smooth,such a control term exists,and that an algorithm to compute it by recursion is provided by the proof. We notice that the resulting control term N is of the same order as the perturbation.III.APPLICATION TO A FORCED PENDULUM MODELWe consider the following model with1.5degrees of freedom1H(p,x,t)=p2+E+ε[cos x+cos(x−t)],(10)2where the actions are A=(p,E)and the angles areϕ=(x,t).The unperturbed Hamiltonian that will be used to construct the operatorsΓ,R and N is1H0(p,E)=The action of {H 0},Γ,R and N on functions V ∈A given byV (p,x,E,t )=k 1,k 2∈ZV k 1,k 2(p,E )e i (k 1x +k 2t ),is{H 0}V =k 1,k 2∈Zi (pk 1+k 2)V k 1,k 2(p,E )e i (k 1x +k 2t ),ΓV =k 1,k 2∈Zχ(pk 1+k 2=0)psin x +12{ΓV,V }=−1∂p∂V4 1(p −1)2cos 2(x −t )−ε2p 2+1FIG.2:Poincar´e surface of section of Hamiltonian (9)with the approximate control term (13)with ε=0.034.where α≤2and still get a lot of KAM tori in the vicinity of the region p =1/2.For instance,the control is stilleffective with α=ing the renormalization-group transformation [1],we have looked at the domain of existence of the golden-mean KAM torus which is the rotational invariant torus with frequency (3−√FIG.3:Frequency analysis of Hamiltonian(9)withε=0.034(a)without control term and(b)with control term(13).The fundamental frequencyω(p)is plotted versus p for p∈[0.15,0.45]for the trajectories with initial conditions(x=0,p).AcknowledgmentsWe acknowledge useful discussions with G.Gallavotti and skar.[1]Chandre,C.and Jauslin,H.R.:2002,‘Renormalization-group analysis for the transition to chaos in Hamiltonian systems’,Physics Reports365,1-64.[2]Ciraolo,G.,Chandre,C.,Lima,R.,Vittot,M.,Pettini,M.,Figarella,C.and Ghendrih,Ph.:2003,‘Control of chaotictransport in Hamiltonian systems’,archived in /nlin.CD/0304040.[3]G.Ciraolo,G.,Briolle,F.,Chandre,C.,Floriani,E.,Lima,R.,Vittot,M.,Pettini,M.,Figarella,C.and Ghendrih,Ph.:2003,‘Control of Hamiltonian chaos as a possible tool to control anomalous transport in fusion plasmas’,in preparation.[4]Gallavotti,G.:1982,‘A criterion of integrability for perturbed nonresonant harmonic oscillators.“Wick ordering”of theperturbations in classical mechanics and invariance of the frequency spectrum’,Commun.Math.Phys.87,365-383.[5]Gallavotti,G.:1985,‘Classical mechanics and renormalization-group’,In:G.Velo and A.S.Wightman(eds.),Regular andChaotic Motions in Dynamical Systems,Plenum,New York,pp.185-231.[6]Gentile,G.and Mastropietro,V.:1996,‘Methods for the analysis of the Lindstedt series for KAM tori and renormalizabilityin classical mechanics’,Rev.Math.Phys.8,393-444.[7]Laskar,J.:1999,‘Introduction to frequency map analysis’,In: C.Sim`o(ed.),Hamiltonian Systems with Three or MoreDegrees of Freedom,NATO ASI Series,Kluwer Academic Publishers,Dordrecht,pp.134.[8]Vittot,M.:2003,‘Perturbation Theory and Control in Classical or Quantum Mechanics by an Inversion Formula’,archivedin /math-ph/0303051.。

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