Lie Symmetries of Differential Equations: Classical Results and Recent Contributions
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Molecular Symmetry
Molecular Symmetry Symmetry helps us understand molecular structure, some chemical properties, and characteristics of physical properties (spectroscopy) – used with group theory to predict vibrational spectra for the identification of molecular shape, and as a tool for understanding electronic structure and bonding. Symmetrical : implies the species possesses a number of indistinguishable configurations. 1 Group Theory : mathematical treatment of symmetry. symmetry operation – an operation performed on an object which leaves it in a configuration that is indistinguishable from, and superimposable on, the original configuration. symmetry elements – the points, lines, or planes to which a symmetry operation is carried out. Element Operation Symbol Identity Identity E Symmetry plane Reflection in the plane σ Inversion center Inversion of a point x,y,z to -x,-y,-z i Proper axis Rotation by (360/n)° Cn 1. Rotation by (360/n)° Improper axis S 2. Reflection in plane perpendicular to rotation axis n Proper axes of rotation (C n) Rotation with respect to a line (axis of rotation). •Cn is a rotation of (360/n)°. •C2 = 180° rotation, C 3 = 120° rotation, C 4 = 90° rotation, C 5 = 72° rotation, C 6 = 60° rotation… •Each rotation brings you to an indistinguishable state from the original. However, rotation by 90° about the same axis does not give back the identical molecule. XeF 4 is square planar. Therefore H 2O does NOT possess It has four different C 2 axes. a C 4 symmetry axis. A C 4 axis out of the page is called the principle axis because it has the largest n . By convention, the principle axis is in the z-direction 2 3 Reflection through a planes of symmetry (mirror plane) If reflection of all parts of a molecule through a plane produced an indistinguishable configuration, the symmetry element is called a mirror plane or plane of symmetry . -
Arxiv:1910.10745V1 [Cond-Mat.Str-El] 23 Oct 2019 2.2 Symmetry-Protected Time Crystals
A Brief History of Time Crystals Vedika Khemania,b,∗, Roderich Moessnerc, S. L. Sondhid aDepartment of Physics, Harvard University, Cambridge, Massachusetts 02138, USA bDepartment of Physics, Stanford University, Stanford, California 94305, USA cMax-Planck-Institut f¨urPhysik komplexer Systeme, 01187 Dresden, Germany dDepartment of Physics, Princeton University, Princeton, New Jersey 08544, USA Abstract The idea of breaking time-translation symmetry has fascinated humanity at least since ancient proposals of the per- petuum mobile. Unlike the breaking of other symmetries, such as spatial translation in a crystal or spin rotation in a magnet, time translation symmetry breaking (TTSB) has been tantalisingly elusive. We review this history up to recent developments which have shown that discrete TTSB does takes place in periodically driven (Floquet) systems in the presence of many-body localization (MBL). Such Floquet time-crystals represent a new paradigm in quantum statistical mechanics — that of an intrinsically out-of-equilibrium many-body phase of matter with no equilibrium counterpart. We include a compendium of the necessary background on the statistical mechanics of phase structure in many- body systems, before specializing to a detailed discussion of the nature, and diagnostics, of TTSB. In particular, we provide precise definitions that formalize the notion of a time-crystal as a stable, macroscopic, conservative clock — explaining both the need for a many-body system in the infinite volume limit, and for a lack of net energy absorption or dissipation. Our discussion emphasizes that TTSB in a time-crystal is accompanied by the breaking of a spatial symmetry — so that time-crystals exhibit a novel form of spatiotemporal order. -
1 the Basic Set-Up 2 Poisson Brackets
MATHEMATICS 7302 (Analytical Dynamics) YEAR 2016–2017, TERM 2 HANDOUT #12: THE HAMILTONIAN APPROACH TO MECHANICS These notes are intended to be read as a supplement to the handout from Gregory, Classical Mechanics, Chapter 14. 1 The basic set-up I assume that you have already studied Gregory, Sections 14.1–14.4. The following is intended only as a succinct summary. We are considering a system whose equations of motion are written in Hamiltonian form. This means that: 1. The phase space of the system is parametrized by canonical coordinates q =(q1,...,qn) and p =(p1,...,pn). 2. We are given a Hamiltonian function H(q, p, t). 3. The dynamics of the system is given by Hamilton’s equations of motion ∂H q˙i = (1a) ∂pi ∂H p˙i = − (1b) ∂qi for i =1,...,n. In these notes we will consider some deeper aspects of Hamiltonian dynamics. 2 Poisson brackets Let us start by considering an arbitrary function f(q, p, t). Then its time evolution is given by n df ∂f ∂f ∂f = q˙ + p˙ + (2a) dt ∂q i ∂p i ∂t i=1 i i X n ∂f ∂H ∂f ∂H ∂f = − + (2b) ∂q ∂p ∂p ∂q ∂t i=1 i i i i X 1 where the first equality used the definition of total time derivative together with the chain rule, and the second equality used Hamilton’s equations of motion. The formula (2b) suggests that we make a more general definition. Let f(q, p, t) and g(q, p, t) be any two functions; we then define their Poisson bracket {f,g} to be n def ∂f ∂g ∂f ∂g {f,g} = − . -
Poisson Structures and Integrability
Poisson Structures and Integrability Peter J. Olver University of Minnesota http://www.math.umn.edu/ olver ∼ Hamiltonian Systems M — phase space; dim M = 2n Local coordinates: z = (p, q) = (p1, . , pn, q1, . , qn) Canonical Hamiltonian system: dz O I = J H J = − dt ∇ ! I O " Equivalently: dpi ∂H dqi ∂H = = dt − ∂qi dt ∂pi Lagrange Bracket (1808): n ∂pi ∂qi ∂qi ∂pi [ u , v ] = ∂u ∂v − ∂u ∂v i#= 1 (Canonical) Poisson Bracket (1809): n ∂u ∂v ∂u ∂v u , v = { } ∂pi ∂qi − ∂qi ∂pi i#= 1 Given functions u , . , u , the (2n) (2n) matrices with 1 2n × respective entries [ u , u ] u , u i, j = 1, . , 2n i j { i j } are mutually inverse. Canonical Poisson Bracket n ∂F ∂H ∂F ∂H F, H = F T J H = { } ∇ ∇ ∂pi ∂qi − ∂qi ∂pi i#= 1 = Poisson (1809) ⇒ Hamiltonian flow: dz = z, H = J H dt { } ∇ = Hamilton (1834) ⇒ First integral: dF F, H = 0 = 0 F (z(t)) = const. { } ⇐⇒ dt ⇐⇒ Poisson Brackets , : C∞(M, R) C∞(M, R) C∞(M, R) { · · } × −→ Bilinear: a F + b G, H = a F, H + b G, H { } { } { } F, a G + b H = a F, G + b F, H { } { } { } Skew Symmetric: F, H = H, F { } − { } Jacobi Identity: F, G, H + H, F, G + G, H, F = 0 { { } } { { } } { { } } Derivation: F, G H = F, G H + G F, H { } { } { } F, G, H C∞(M, R), a, b R. ∈ ∈ In coordinates z = (z1, . , zm), F, H = F T J(z) H { } ∇ ∇ where J(z)T = J(z) is a skew symmetric matrix. − The Jacobi identity imposes a system of quadratically nonlinear partial differential equations on its entries: ∂J jk ∂J ki ∂J ij J il + J jl + J kl = 0 ! ∂zl ∂zl ∂zl " #l Given a Poisson structure, the Hamiltonian flow corresponding to H C∞(M, R) is the system of ordinary differential equati∈ons dz = z, H = J(z) H dt { } ∇ Lie’s Theory of Function Groups Used for integration of partial differential equations: F , F = G (F , . -
TASI 2008 Lectures: Introduction to Supersymmetry And
TASI 2008 Lectures: Introduction to Supersymmetry and Supersymmetry Breaking Yuri Shirman Department of Physics and Astronomy University of California, Irvine, CA 92697. [email protected] Abstract These lectures, presented at TASI 08 school, provide an introduction to supersymmetry and supersymmetry breaking. We present basic formalism of supersymmetry, super- symmetric non-renormalization theorems, and summarize non-perturbative dynamics of supersymmetric QCD. We then turn to discussion of tree level, non-perturbative, and metastable supersymmetry breaking. We introduce Minimal Supersymmetric Standard Model and discuss soft parameters in the Lagrangian. Finally we discuss several mech- anisms for communicating the supersymmetry breaking between the hidden and visible sectors. arXiv:0907.0039v1 [hep-ph] 1 Jul 2009 Contents 1 Introduction 2 1.1 Motivation..................................... 2 1.2 Weylfermions................................... 4 1.3 Afirstlookatsupersymmetry . .. 5 2 Constructing supersymmetric Lagrangians 6 2.1 Wess-ZuminoModel ............................... 6 2.2 Superfieldformalism .............................. 8 2.3 VectorSuperfield ................................. 12 2.4 Supersymmetric U(1)gaugetheory ....................... 13 2.5 Non-abeliangaugetheory . .. 15 3 Non-renormalization theorems 16 3.1 R-symmetry.................................... 17 3.2 Superpotentialterms . .. .. .. 17 3.3 Gaugecouplingrenormalization . ..... 19 3.4 D-termrenormalization. ... 20 4 Non-perturbative dynamics in SUSY QCD 20 4.1 Affleck-Dine-Seiberg -
Observability and Symmetries of Linear Control Systems
S S symmetry Article Observability and Symmetries of Linear Control Systems Víctor Ayala 1,∗, Heriberto Román-Flores 1, María Torreblanca Todco 2 and Erika Zapana 2 1 Instituto de Alta Investigación, Universidad de Tarapacá, Casilla 7D, Arica 1000000, Chile; [email protected] 2 Departamento Académico de Matemáticas, Universidad, Nacional de San Agustín de Arequipa, Calle Santa Catalina, Nro. 117, Arequipa 04000, Peru; [email protected] (M.T.T.); [email protected] (E.Z.) * Correspondence: [email protected] Received: 7 April 2020; Accepted: 6 May 2020; Published: 4 June 2020 Abstract: The goal of this article is to compare the observability properties of the class of linear control systems in two different manifolds: on the Euclidean space Rn and, in a more general setup, on a connected Lie group G. For that, we establish well-known results. The symmetries involved in this theory allow characterizing the observability property on Euclidean spaces and the local observability property on Lie groups. Keywords: observability; symmetries; Euclidean spaces; Lie groups 1. Introduction For general facts about control theory, we suggest the references, [1–5], and for general mathematical issues, the references [6–8]. In the context of this article, a general control system S can be modeled by the data S = (M, D, h, N). Here, M is the manifold of the space states, D is a family of differential equations on M, or if you wish, a family of vector fields on the manifold, h : M ! N is a differentiable observation map, and N is a manifold that contains all the known information that you can see of the system through h. -
The History of the Abel Prize and the Honorary Abel Prize the History of the Abel Prize
The History of the Abel Prize and the Honorary Abel Prize The History of the Abel Prize Arild Stubhaug On the bicentennial of Niels Henrik Abel’s birth in 2002, the Norwegian Govern- ment decided to establish a memorial fund of NOK 200 million. The chief purpose of the fund was to lay the financial groundwork for an annual international prize of NOK 6 million to one or more mathematicians for outstanding scientific work. The prize was awarded for the first time in 2003. That is the history in brief of the Abel Prize as we know it today. Behind this government decision to commemorate and honor the country’s great mathematician, however, lies a more than hundred year old wish and a short and intense period of activity. Volumes of Abel’s collected works were published in 1839 and 1881. The first was edited by Bernt Michael Holmboe (Abel’s teacher), the second by Sophus Lie and Ludvig Sylow. Both editions were paid for with public funds and published to honor the famous scientist. The first time that there was a discussion in a broader context about honoring Niels Henrik Abel’s memory, was at the meeting of Scan- dinavian natural scientists in Norway’s capital in 1886. These meetings of natural scientists, which were held alternately in each of the Scandinavian capitals (with the exception of the very first meeting in 1839, which took place in Gothenburg, Swe- den), were the most important fora for Scandinavian natural scientists. The meeting in 1886 in Oslo (called Christiania at the time) was the 13th in the series. -
Lecture 3 1.1. a Lie Algebra Is a Vector Space Along with a Map [.,.] : 多 多 多 Such That, [Αa+Βb,C] = Α[A,C]+Β[B,C] B
Lecture 3 1. LIE ALGEBRAS 1.1. A Lie algebra is a vector space along with a map [:;:] : L ×L ! L such that, [aa + bb;c] = a[a;c] + b[b;c] bi − linear [a;b] = −[b;a] Anti − symmetry [[a;b];c] + [[b;c];a][[c;a];b] = 0; Jacobi identity We will only think of real vector spaces. Even when we talk of matrices with complex numbers as entries, we will assume that only linear combina- tions with real combinations are taken. 1.1.1. A homomorphism is a linear map among Lie algebras that preserves the commutation relations. 1.1.2. An isomorphism is a homomorphism that is invertible; that is, there is a one-one correspondence of basis vectors that preserves the commuta- tion relations. 1.1.3. An homomorphism to a Lie algebra of matrices is called a represe- tation. A representation is faithful if it is an isomorphism. 1.2. Examples. (1) The basic example is the cross-product in three dimensional Eu- clidean space. Recall that i j k a × b = a1 a2 a3 b1 b2 b3 The bilinearity and anti-symmetry are obvious; the Jacobi identity can be verified through tedious calculations. Or you can use the fact that any cross product is determined by the cross-product of the basis vectors through linearity; and verify the Jacobi identity on the basis vectors using the cross products i × j = k; j × k = i; k×i= j Under many different names, this Lie algebra appears everywhere in physics. It is the single most important example of a Lie algebra. -
About Symmetries in Physics
LYCEN 9754 December 1997 ABOUT SYMMETRIES IN PHYSICS Dedicated to H. Reeh and R. Stora1 Fran¸cois Gieres Institut de Physique Nucl´eaire de Lyon, IN2P3/CNRS, Universit´eClaude Bernard 43, boulevard du 11 novembre 1918, F - 69622 - Villeurbanne CEDEX Abstract. The goal of this introduction to symmetries is to present some general ideas, to outline the fundamental concepts and results of the subject and to situate a bit the following arXiv:hep-th/9712154v1 16 Dec 1997 lectures of this school. [These notes represent the write-up of a lecture presented at the fifth S´eminaire Rhodanien de Physique “Sur les Sym´etries en Physique” held at Dolomieu (France), 17-21 March 1997. Up to the appendix and the graphics, it is to be published in Symmetries in Physics, F. Gieres, M. Kibler, C. Lucchesi and O. Piguet, eds. (Editions Fronti`eres, 1998).] 1I wish to dedicate these notes to my diploma and Ph.D. supervisors H. Reeh and R. Stora who devoted a major part of their scientific work to the understanding, description and explo- ration of symmetries in physics. Contents 1 Introduction ................................................... .......1 2 Symmetries of geometric objects ...................................2 3 Symmetries of the laws of nature ..................................5 1 Geometric (space-time) symmetries .............................6 2 Internal symmetries .............................................10 3 From global to local symmetries ...............................11 4 Combining geometric and internal symmetries ...............14 -
Institut F¨Ur Informatik Und Praktische Mathematik Christian-Albrechts-Universit¨At Kiel
INSTITUT FUR¨ INFORMATIK UND PRAKTISCHE MATHEMATIK Pose Estimation Revisited Bodo Rosenhahn Bericht Nr. 0308 September 2003 CHRISTIAN-ALBRECHTS-UNIVERSITAT¨ KIEL Institut f¨ur Informatik und Praktische Mathematik der Christian-Albrechts-Universit¨at zu Kiel Olshausenstr. 40 D – 24098 Kiel Pose Estimation Revisited Bodo Rosenhahn Bericht Nr. 0308 September 2003 e-mail: [email protected] “Dieser Bericht gibt den Inhalt der Dissertation wieder, die der Verfasser im April 2003 bei der Technischen Fakult¨at der Christian-Albrechts-Universit¨at zu Kiel eingereicht hat. Datum der Disputation: 19. August 2003.” 1. Gutachter Prof. G. Sommer (Kiel) 2. Gutachter Prof. D. Betten (Kiel) 3. Gutachter Dr. L. Dorst (Amsterdam) Datum der m¨undlichen Pr¨ufung: 19.08.2003 ABSTRACT The presented thesis deals with the 2D-3D pose estimation problem. Pose estimation means to estimate the relative position and orientation of a 3D ob- ject with respect to a reference camera system. The main focus concentrates on the geometric modeling and application of the pose problem. To deal with the different geometric spaces (Euclidean, affine and projective ones), a homogeneous model for conformal geometry is applied in the geometric algebra framework. It allows for a compact and linear modeling of the pose scenario. In the chosen embedding of the pose problem, a rigid body motion is represented as an orthogonal transformation whose parameters can be es- timated efficiently in the corresponding Lie algebra. In addition, the chosen algebraic embedding allows the modeling of extended features derived from sphere concepts in contrast to point concepts used in classical vector cal- culus. -
Symmetries in Physics Are [2, 4, 5]
Symmetries in physics ∗ Roelof Bijker ICN-UNAM, AP 70-543, 04510 M´exico, DF, M´exico E-mail: [email protected] August 24, 2005 Abstract The concept of symmetries in physics is briefly reviewed. In the first part of these lecture notes, some of the basic mathematical tools needed for the understanding of symmetries in nature are presented, namely group theory, Lie groups and Lie algebras, and Noether’s theorem. In the sec- ond part, some applications of symmetries in physics are discussed, ranging from isospin and flavor symmetry to more recent developments involving the interacting boson model and its extension to supersymmetries in nuclear physics. 1 Introduction Symmetry and its mathematical framework—group theory—play an increasingly important role in physics. Both classical and quantum systems usually display great complexity, but the analysis of their symmetry properties often gives rise to simplifications and new insights which can lead to a deeper understanding. In addition, symmetries themselves can point the way toward the formulation of a correct physical theory by providing constraints and guidelines in an otherwise intractable situation. It is remarkable that, in spite of the wide variety of systems one may consider, all the way from classical ones to molecules, nuclei, and elementary particles, group theory applies the same basic principles and extracts the same kind of useful information from all of them. This universality in the applicability of symmetry considerations is one of the most attractive features of group theory. Most people have an intuitive understanding of symmetry, particularly in its most obvious manifestation in terms of geometric transformations that leave a body arXiv:nucl-th/0509007v1 2 Sep 2005 or system invariant. -
Norway Establishes Abel Prize in Mathematics, Volume 49, Number 1
Norway Establishes Abel Prize in Mathematics In August 2001, the prime close contact with its minister of Norway an- counterpart in Sweden, nounced the establish- which administers the ment of the Abel Prize, a Nobel Prizes. In consul- new international prize tation with the Interna- in mathematics. Named tional Mathematical in honor of the Norwe- Union (IMU), the Norwe- gian mathematician Niels gian Academy will appoint Henrik Abel (1802–1829), a prize selection commit- the prize will be awarded for tee of perhaps five members the first time in 2003. The and a larger scientific advi- prize fund will have an initial sory panel of twenty to thirty capital of 200 million Norwegian members. The panel will generate kroner (about US$23 million). The nominations to be forwarded to the amount of the prize will fluctuate ac- selection committee. The committee cording to the yield of the fund but will be and panel will be international and will in- similar to the amount of a Nobel Prize. The pre- clude a substantial number of mathematicians liminary figure for the Abel Prize is 5 million Nor- from outside Norway. wegian kroner (about US$570,000). Various details of the prize have yet to be worked The idea of an international prize in honor of out, such as whether it can be given to more than Abel was first suggested by the Norwegian math- one individual and whether recipients of the Fields ematician Sophus Lie near the end of the nine- Medal, long thought of as the “Nobel of mathe- teenth century.