Time-Dependent Hamiltonian Mechanics on a Locally Conformal
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Hamiltonian Systems on Symplectic Manifolds
This is page 147 Printer: Opaque this 5 Hamiltonian Systems on Symplectic Manifolds Now we are ready to geometrize Hamiltonian mechanics to the context of manifolds. First we make phase spaces nonlinear, and then we study Hamiltonian systems in this context. 5.1 Symplectic Manifolds Definition 5.1.1. A symplectic manifold is a pair (P, Ω) where P is a manifold and Ω is a closed (weakly) nondegenerate two-form on P .IfΩ is strongly nondegenerate, we speak of a strong symplectic manifold. As in the linear case, strong nondegeneracy of the two-form Ω means that at each z ∈ P, the bilinear form Ωz : TzP × TzP → R is nondegenerate, that is, Ωz defines an isomorphism → ∗ Ωz : TzP Tz P. Fora(weak) symplectic form, the induced map Ω : X(P ) → X∗(P )be- tween vector fields and one-forms is one-to-one, but in general is not sur- jective. We will see later that Ω is required to be closed, that is, dΩ=0, where d is the exterior derivative, so that the induced Poisson bracket sat- isfies the Jacobi identity and so that the flows of Hamiltonian vector fields will consist of canonical transformations. In coordinates zI on P in the I J finite-dimensional case, if Ω = ΩIJ dz ∧ dz (sum over all I<J), then 148 5. Hamiltonian Systems on Symplectic Manifolds dΩ=0becomes the condition ∂Ω ∂Ω ∂Ω IJ + KI + JK =0. (5.1.1) ∂zK ∂zJ ∂zI Examples (a) Symplectic Vector Spaces. If (Z, Ω) is a symplectic vector space, then it is also a symplectic manifold. -
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} = − . -
Canonical Transformations (Lecture 4)
Canonical transformations (Lecture 4) January 26, 2016 61/441 Lecture outline We will introduce and discuss canonical transformations that conserve the Hamiltonian structure of equations of motion. Poisson brackets are used to verify that a given transformation is canonical. A practical way to devise canonical transformation is based on usage of generation functions. The motivation behind this study is to understand the freedom which we have in the choice of various sets of coordinates and momenta. Later we will use this freedom to select a convenient set of coordinates for description of partilcle's motion in an accelerator. 62/441 Introduction Within the Lagrangian approach we can choose the generalized coordinates as we please. We can start with a set of coordinates qi and then introduce generalized momenta pi according to Eqs. @L(qk ; q_k ; t) pi = ; i = 1;:::; n ; @q_i and form the Hamiltonian ! H = pi q_i - L(qk ; q_k ; t) : i X Or, we can chose another set of generalized coordinates Qi = Qi (qk ; t), express the Lagrangian as a function of Qi , and obtain a different set of momenta Pi and a different Hamiltonian 0 H (Qi ; Pi ; t). This type of transformation is called a point transformation. The two representations are physically equivalent and they describe the same dynamics of our physical system. 63/441 Introduction A more general approach to the problem of using various variables in Hamiltonian formulation of equations of motion is the following. Let us assume that we have canonical variables qi , pi and the corresponding Hamiltonian H(qi ; pi ; t) and then make a transformation to new variables Qi = Qi (qk ; pk ; t) ; Pi = Pi (qk ; pk ; t) : i = 1 ::: n: (4.1) 0 Can we find a new Hamiltonian H (Qi ; Pi ; t) such that the system motion in new variables satisfies Hamiltonian equations with H 0? What are requirements on the transformation (4.1) for such a Hamiltonian to exist? These questions lead us to canonical transformations. -
Classical Mechanics Examples (Canonical Transformation)
Classical Mechanics Examples (Canonical Transformation) Dipan Kumar Ghosh Centre for Excellence in Basic Sciences Kalina, Mumbai 400098 November 10, 2016 1 Introduction In classical mechanics, there is no unique prescription for one to choose the generalized coordinates for a problem. As long as the coordinates and the corresponding momenta span the entire phase space, it becomes an acceptable set. However, it turns out in prac- tice that some choices are better than some others as they make a given problem simpler while still preserving the form of Hamilton's equations. Going over from one set of chosen coordinates and momenta to another set which satisfy Hamilton's equations is done by canonical transformation. For instance, if we consider the central force problem in two dimensions and choose Carte- k sian coordinate, the potential is − . However, if we choose (r; θ) coordinates, px2 + y2 k the potential is − and θ is cyclic, which greatly simplifies the problem. The number of r cyclic coordinates in a problem may depend on the choice of generalized coordinates. A cyclic coordinate results in a constant of motion which is its conjugate momentum. The example above where we replace one set of coordinates by another set is known as point transformation. In the Hamiltonian formalism, the coordinates and momenta are given equal status and the dynamics occurs in what we know as the phase space. In dealing with phase space dynamics, we need point transformations in the phase space where the new coordinates (Qi) and the new momenta (Pi) are functions of old coordinates (pi) and old momenta (pi): Qi = Qi(fqjg; fpjg; t) Pi = Pi(fqjg; fpjg; t) 1 c D. -
Conformal Hamiltonian Systems
Journal of Geometry and Physics 39 (2001) 276–300 Conformal Hamiltonian systems Robert McLachlan∗, Matthew Perlmutter IFS, Massey University, Palmerston North, New Zealand 5301 Received 4 August 2000; received in revised form 23 January 2001 Abstract Vector fields whose flow preserves a symplectic form up to a constant, such as simple mechanical systems with friction, are called “conformal”. We develop a reduction theory for symmetric con- formal Hamiltonian systems, analogous to symplectic reduction theory. This entire theory extends naturally to Poisson systems: given a symmetric conformal Poisson vector field, we show that it induces two reduced conformal Poisson vector fields, again analogous to the dual pair construction for symplectic manifolds. Conformal Poisson systems form an interesting infinite-dimensional Lie algebra of foliate vector fields. Manifolds supporting such conformal vector fields include cotan- gent bundles, Lie–Poisson manifolds, and their natural quotients. © 2001 Elsevier Science B.V. All rights reserved. MSC: 53C57; 58705 Sub. Class.: Dynamical systems Keywords: Hamiltonian systems; Conformal Poisson structure 1. Introduction The fields of symplectic geometry and geometric mechanics are closely linked, indeed almost synonymous [10,14]. One of their most important features is that the symplectic diffeomorphisms on a manifold form a group. This property can be taken as the definition of “geometry;” it is natural to try and generalize it. In 1913 Cartan [5,24] found that, subject to certain restrictions, there are just six classes of groups of diffeomorphisms on any manifold, namely (i) Diff itself; (ii) Diffω, the diffeomorphisms preserving a symplectic 2-form ω; (iii) Diffµ, the diffeomorphisms preserving a volume form µ; (iv) Diffα, the diffeomorphisms c preserving a contact form α up to a function; and the conformal groups, (v) Diffω and (vi) c Diffµ, the diffeomorphisms preserving the form ω or µ up to a constant. -
PHYS 705: Classical Mechanics Canonical Transformation 2
1 PHYS 705: Classical Mechanics Canonical Transformation 2 Canonical Variables and Hamiltonian Formalism As we have seen, in the Hamiltonian Formulation of Mechanics, qj, p j are independent variables in phase space on equal footing The Hamilton’s Equation for q j , p j are “symmetric” (symplectic, later) H H qj and p j pj q j This elegant formal structure of mechanics affords us the freedom in selecting other appropriate canonical variables as our phase space “coordinates” and “momenta” - As long as the new variables formally satisfy this abstract structure (the form of the Hamilton’s Equations. 3 Canonical Transformation Recall (from hw) that the Euler-Lagrange Equation is invariant for a point transformation: Qj Qqt j ( ,) L d L i.e., if we have, 0, qj dt q j L d L then, 0, Qj dt Q j Now, the idea is to find a generalized (canonical) transformation in phase space (not config. space) such that the Hamilton’s Equations are invariant ! Qj Qqpt j (, ,) (In general, we look for transformations which Pj Pqpt j (, ,) are invertible.) 4 Invariance of EL equation for Point Transformation First look at the situation in config. space first: dL L Given: 0, and a point transformation: Q Qqt( ,) j j dt q j q j dL L 0 Need to show: dt Q j Q j L Lqi L q i Formally, calculate: (chain rule) Qji qQ ij i qQ ij L L q L q i i Q j i qiQ j i q i Q j From the inverse point transformation equation q i qQt i ( ,) , we have, qi q q q q 0 and i i qi Q i Q i k j Q j Qj k Qk t 5 Invariance of EL equation -
SYMPLECTIC GEOMETRY Lecture Notes, University of Toronto
SYMPLECTIC GEOMETRY Eckhard Meinrenken Lecture Notes, University of Toronto These are lecture notes for two courses, taught at the University of Toronto in Spring 1998 and in Fall 2000. Our main sources have been the books “Symplectic Techniques” by Guillemin-Sternberg and “Introduction to Symplectic Topology” by McDuff-Salamon, and the paper “Stratified symplectic spaces and reduction”, Ann. of Math. 134 (1991) by Sjamaar-Lerman. Contents Chapter 1. Linear symplectic algebra 5 1. Symplectic vector spaces 5 2. Subspaces of a symplectic vector space 6 3. Symplectic bases 7 4. Compatible complex structures 7 5. The group Sp(E) of linear symplectomorphisms 9 6. Polar decomposition of symplectomorphisms 11 7. Maslov indices and the Lagrangian Grassmannian 12 8. The index of a Lagrangian triple 14 9. Linear Reduction 18 Chapter 2. Review of Differential Geometry 21 1. Vector fields 21 2. Differential forms 23 Chapter 3. Foundations of symplectic geometry 27 1. Definition of symplectic manifolds 27 2. Examples 27 3. Basic properties of symplectic manifolds 34 Chapter 4. Normal Form Theorems 43 1. Moser’s trick 43 2. Homotopy operators 44 3. Darboux-Weinstein theorems 45 Chapter 5. Lagrangian fibrations and action-angle variables 49 1. Lagrangian fibrations 49 2. Action-angle coordinates 53 3. Integrable systems 55 4. The spherical pendulum 56 Chapter 6. Symplectic group actions and moment maps 59 1. Background on Lie groups 59 2. Generating vector fields for group actions 60 3. Hamiltonian group actions 61 4. Examples of Hamiltonian G-spaces 63 3 4 CONTENTS 5. Symplectic Reduction 72 6. Normal forms and the Duistermaat-Heckman theorem 78 7. -
The Hamiltonian Formulation of Geodesics
U.U.D.M. Project Report 2021:36 The Hamiltonian formulation of geodesics Victor Hildebrandsson Examensarbete i matematik, 15 hp Handledare: Georgios Dimitroglou Rizell Examinator: Martin Herschend Juli 2021 Department of Mathematics Uppsala University Abstract We explore the Hamiltonian formulation of the geodesic equation. We start with the definition of a differentiable manifold. Then we continue with studying tensors and differential forms. We define a Riemannian manifold (M; g) and geodesics, the shortest path between two points, on such manifolds. Lastly, we define the symplectic manifold (T ∗M; d(pdq)), and study the connection between geodesics and the flow of Hamilton's equations. 2 Contents 1 Introduction 4 2 Background 5 2.1 Calculus of variations . .5 2.2 Differentiable manifolds . .8 2.3 Tensors and vector bundles . 10 3 Differential forms 13 3.1 Exterior and differential forms . 13 3.2 Integral and exterior derivative of differential forms . 14 4 Riemannian manifolds 17 5 Symplectic manifolds 20 References 25 3 1 Introduction In this thesis, we will study Riemannian manifolds and symplectic manifolds. More specifically, we will study geodesics, and their connection to the Hamilto- nian flow on the symplectic cotangent bundle. A manifold is a topological space which locally looks like Euclidean space. The study of Riemannian manifolds is called Riemannian geometry, the study of symplectic manifolds is called symplectic geometry. Riemannian geometry was first studied by Bernhard Riemann in his habil- itation address "Uber¨ die Hypothesen, welche der Geometrie zugrunde liegen" ("On the Hypotheses on which Geometry is Based"). In particular, it was the first time a mathematician discussed the concept of a differentiable manifold [1]. -
Odd and Even Poisson Brackets 1
Odd and even Poisson brackets 1 Y. Kosmann-Schwarzbach Centre de Math´ematiques (Unit´eMixte de Recherches du C.N.R.S. 7640) Ecole Polytechnique F-91128 Palaiseau, France Abstract On a Poisson manifold, the divergence of a hamiltonian vector field is a derivation of the algebra of functions, called the modular vector field. In the case of an odd Poisson bracket on a supermanifold, the divergence of a hamilto- nian vector field is a generator of the odd bracket, and it is nontrivial, whether the Poisson structure is symplectic or not. The quantum master equation is a Maurer-Cartan equation written in terms of an odd Poisson bracket (an- tibracket) and of a generator of square 0 of this bracket. The derived bracket of the antibracket with respect to the quantum BRST differential defines the even graded Lie algebra structure of the space of quantum gauge parameters. 1 Introduction In the “geometry of Batalin-Vilkovisky quantization” [13] [14], a supermanifold (M, A) of dimension n|n is equipped with an odd Poisson structure. More precisely, A is a sheaf of Z2-graded Gerstenhaber algebras. A Z2-graded Gerstenhaber algebra A is a Z2-graded commutative, associative algebra, with a bracket, [ , ], satisfying [f,g]= −(−1)(|f|−1)(|g|−1)[g, f] , [f, [g, h]] = [[f,g], h]+(−1)(|f|−1)(|g|−1)[g, [f, h]] , [f,gh] = [f,g]h +(−1)(|f|−1)|g|g[f, h] , 1Quantum Theory and Symmetries, H.-D. Doebner et al.. eds., World Scientific, 2000, 565-571. 1 for all f,g,h ∈ A, where |f| denotes the degree of f. -
To Be Completed. LECTURE NOTES 1. Hamiltonian
to be completed. LECTURE NOTES HONGYU HE 1. Hamiltonian Mechanics Let us consider the classical harmonic oscillator mx¨ = −kx (x ∈ R). This is a second order differential equation in terms of Newtonian mechanics. We can convert it into 1st order ordinary differential equations by introducing the momentum p = mx˙; q = x. Then we have p q˙ = , p˙ = −kq. m p The map (q, p) → m i − kqj defines a smooth vector field. The flow curve of this vector field gives the time evolution from any initial state (q(0), p(0)). p2 kq2 Let H(q, p) = 2m + 2 be the Hamiltonian. It represents the energy function. Then ∂H ∂H p = kq, = . ∂q ∂p m So we have ∂H ∂H q˙ = , p˙ = − . ∂p ∂q Generally speaking, for p, q ∈ Rn, for H(q, p) the Hamiltonian, ∂H ∂H q˙ = , p˙ = − . ∂p ∂q is called the Hamiltonian equation. The vector field ∂H ∂H (q, p) → ( , − ) ∂p ∂q 2n is called the Hamiltonian vector field, denoted by XH . In this case, {(q, p)} = R is called the phase space. Any (q, p) is called a state. Any functions on (q, p) is called an observable. In particular H is an observable. Suppose that H is smooth. Then the Hamiltonian equation has local solutions. In other words, 2n for each (q0, p0) ∈ R , there exists > 0 and a function (q(t), p(t))(t ∈ [0, )) such that ∂H ∂H q˙(t) = (q(t), p(t)), p˙(t) = − (q(t), p(t)) ∂p ∂q and q(0) = q0, p(0) = p0. Put φ(q0, p0, t) = (q(t), p(t)). -
Classical Mechanics
Classical Mechanics Joseph Conlon April 9, 2014 Abstract These are the current notes for the S7 Classical Mechanics course as of 9th April 2014. They contain the complete text and diagrams of the notes. There will be no more substantive revisions of these notes until Hilary 2014-15 (small typographical revisions may occur inbetween). Contents 1 Course Summary 3 2 Calculus of Variations 5 3 Lagrangian Mechanics 10 3.1 Lagrange's Equations . 10 3.2 Rotating Frames . 16 3.3 Normal Modes . 22 3.4 Particle in an Electromagnetic Field . 25 3.5 Rigid Bodies . 27 3.6 Noether's Theorem . 30 4 Hamiltonian Mechanics 33 4.1 Hamilton's Equations . 33 4.2 Hamilton's Equations from the Action Principle . 35 4.3 Poisson Brackets . 36 4.4 Liouville's Theorem . 39 4.5 Canonical Transformations . 42 5 Advanced Topics 50 5.1 The Hamilton-Jacobi Equation . 50 5.2 The Path Integral Formulation of Quantum Mechanics . 55 5.3 Integrable systems and Action/Angle Variables . 60 2 Chapter 1 Course Summary This course is the S7 Classical Mechanics short option (for physicists) and also the B7 Classical Mechanics option for those doing Physics and Philosophy. It consists of 16 lectures in total, and aims to cover advanced classical me- chanics, and in particular the theoretical aspects of Lagrangian and Hamiltonian mechanics. Approximately, the first 12 lectures cover material that is examinable for both courses, whereas the last four lectures (approximately) cove material that is examinable only for B7. General Comments Why be interested in classical mechanics and why be interested in this course? Classical mechanics has a beautiful theoretical structure which is obscured simply by a presentation of Newton's laws along the lines of F = ma. -
On the AKSZ Formulation of the Poisson Sigma Model
Cattaneo, A S (2001). On the AKSZ formulation of the Poisson sigma model. Letters in Mathematical Physics, 56(2):163-179. Postprint available at: http://www.zora.uzh.ch University of Zurich Posted at the Zurich Open Repository and Archive, University of Zurich. Zurich Open Repository and Archive http://www.zora.uzh.ch Originally published at: Letters in Mathematical Physics 2001, 56(2):163-179. Winterthurerstr. 190 CH-8057 Zurich http://www.zora.uzh.ch Year: 2001 On the AKSZ formulation of the Poisson sigma model Cattaneo, A S Cattaneo, A S (2001). On the AKSZ formulation of the Poisson sigma model. Letters in Mathematical Physics, 56(2):163-179. Postprint available at: http://www.zora.uzh.ch Posted at the Zurich Open Repository and Archive, University of Zurich. http://www.zora.uzh.ch Originally published at: Letters in Mathematical Physics 2001, 56(2):163-179. On the AKSZ formulation of the Poisson sigma model Abstract We review and extend the Alexandrov-Kontsevich-Schwarz-Zaboronsky construction of solutions of the Batalin-Vilkovisky classical master equation. In particular, we study the case of sigma models on manifolds with boundary. We show that a special case of this construction yields the Batalin-Vilkovisky action functional of the Poisson sigma model on a disk. As we have shown in a previous paper, the perturbative quantization of this model is related to Kontsevich's deformation quantization of Poisson manifolds and to his formality theorem. We also discuss the action of diffeomorphisms of the target manifolds. ON THE AKSZ FORMULATION OF THE POISSON SIGMA MODEL ALBERTO S.