Star Product for Second Class Constraint Systems from a BRST
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Functor and Natural Operators on Symplectic Manifolds
Mathematical Methods and Techniques in Engineering and Environmental Science Functor and natural operators on symplectic manifolds CONSTANTIN PĂTRĂŞCOIU Faculty of Engineering and Management of Technological Systems, Drobeta Turnu Severin University of Craiova Drobeta Turnu Severin, Str. Călugăreni, No.1 ROMANIA [email protected] http://www.imst.ro Abstract. Symplectic manifolds arise naturally in abstract formulations of classical Mechanics because the phase–spaces in Hamiltonian mechanics is the cotangent bundle of configuration manifolds equipped with a symplectic structure. The natural functors and operators described in this paper can be helpful both for a unified description of specific proprieties of symplectic manifolds and for finding links to various fields of geometric objects with applications in Hamiltonian mechanics. Key-words: Functors, Natural operators, Symplectic manifolds, Complex structure, Hamiltonian. 1. Introduction. diffeomorphism f : M → N , a vector bundle morphism The geometrics objects (like as vectors, covectors, T*f : T*M→ T*N , which covers f , where −1 tensors, metrics, e.t.c.) on a smooth manifold M, x = x :)*)(()*( x * → xf )( * NTMTfTfT are the elements of the total spaces of a vector So, the cotangent functor, )(:* → VBmManT and bundles with base M. The fields of such geometrics objects are the section in corresponding vector more general ΛkT * : Man(m) → VB , are the bundles. bundle functors from Man(m) to VB, where Man(m) By example, the vectors on a smooth manifold M (subcategory of Man) is the category of m- are the elements of total space of vector bundles dimensional smooth manifolds, the morphisms of this (TM ,π M , M); the covectors on M are the elements category are local diffeomorphisms between of total space of vector bundles (T*M , pM , M). -
Reduced Phase Space Quantization and Dirac Observables
Reduced Phase Space Quantization and Dirac Observables T. Thiemann∗ MPI f. Gravitationsphysik, Albert-Einstein-Institut, Am M¨uhlenberg 1, 14476 Potsdam, Germany and Perimeter Institute f. Theoretical Physics, Waterloo, ON N2L 2Y5, Canada Abstract In her recent work, Dittrich generalized Rovelli’s idea of partial observables to construct Dirac observables for constrained systems to the general case of an arbitrary first class constraint algebra with structure functions rather than structure constants. Here we use this framework and propose how to implement explicitly a reduced phase space quantization of a given system, at least in principle, without the need to compute the gauge equivalence classes. The degree of practicality of this programme depends on the choice of the partial observables involved. The (multi-fingered) time evolution was shown to correspond to an automorphism on the set of Dirac observables so generated and interesting representations of the latter will be those for which a suitable preferred subgroup is realized unitarily. We sketch how such a programme might look like for General Relativity. arXiv:gr-qc/0411031v1 6 Nov 2004 We also observe that the ideas by Dittrich can be used in order to generate constraints equivalent to those of the Hamiltonian constraints for General Relativity such that they are spatially diffeomorphism invariant. This has the important consequence that one can now quantize the new Hamiltonian constraints on the partially reduced Hilbert space of spatially diffeomorphism invariant states, just as for the recently proposed Master constraint programme. 1 Introduction It is often stated that there are no Dirac observables known for General Relativity, except for the ten Poincar´echarges at spatial infinity in situations with asymptotically flat boundary conditions. -
Theory of Systems with Constraints
Theory of systems with Constraints Javier De Cruz P´erez Facultat de F´ısica, Universitat de Barcelona, Diagonal 645, 08028 Barcelona, Spain.∗ Abstract: We discuss systems subject to constraints. We review Dirac's classical formalism of dealing with such problems and motivate the definition of objects such as singular and nonsingular Lagrangian, first and second class constraints, and the Dirac bracket. We show how systems with first class constraints can be considered to be systems with gauge freedom. We conclude by studing a classical example of systems with constraints, electromagnetic field I. INTRODUCTION II. GENERAL CONSIDERATIONS Consider a system with a finite number, k , of degrees of freedom is described by a Lagrangian L = L(qs; q_s) that don't depend on t. The action of the system is [3] In the standard case, to obtain the equations of motion, Z we follow the usual steps. If we use the Lagrangian for- S = dtL(qs; q_s) (1) malism, first of all we find the Lagrangian of the system, calculate the Euler-Lagrange equations and we obtain the If we apply the least action principle action δS = 0, we accelerations as a function of positions and velocities. All obtain the Euler-Lagrange equations this is possible if and only if the Lagrangian of the sys- tems is non-singular, if not so the system is non-standard @L d @L − = 0 s = 1; :::; k (2) and we can't apply the standard formalism. Then we say @qs dt @q_s that the Lagrangian is singular and constraints on the ini- tial data occur. -
Hamiltonian and Symplectic Symmetries: an Introduction
BULLETIN (New Series) OF THE AMERICAN MATHEMATICAL SOCIETY Volume 54, Number 3, July 2017, Pages 383–436 http://dx.doi.org/10.1090/bull/1572 Article electronically published on March 6, 2017 HAMILTONIAN AND SYMPLECTIC SYMMETRIES: AN INTRODUCTION ALVARO´ PELAYO In memory of Professor J.J. Duistermaat (1942–2010) Abstract. Classical mechanical systems are modeled by a symplectic mani- fold (M,ω), and their symmetries are encoded in the action of a Lie group G on M by diffeomorphisms which preserve ω. These actions, which are called sym- plectic, have been studied in the past forty years, following the works of Atiyah, Delzant, Duistermaat, Guillemin, Heckman, Kostant, Souriau, and Sternberg in the 1970s and 1980s on symplectic actions of compact Abelian Lie groups that are, in addition, of Hamiltonian type, i.e., they also satisfy Hamilton’s equations. Since then a number of connections with combinatorics, finite- dimensional integrable Hamiltonian systems, more general symplectic actions, and topology have flourished. In this paper we review classical and recent re- sults on Hamiltonian and non-Hamiltonian symplectic group actions roughly starting from the results of these authors. This paper also serves as a quick introduction to the basics of symplectic geometry. 1. Introduction Symplectic geometry is concerned with the study of a notion of signed area, rather than length, distance, or volume. It can be, as we will see, less intuitive than Euclidean or metric geometry and it is taking mathematicians many years to understand its intricacies (which is work in progress). The word “symplectic” goes back to the 1946 book [164] by Hermann Weyl (1885–1955) on classical groups. -
Arxiv:Math-Ph/9812022 V2 7 Aug 2000
Local quantum constraints Hendrik Grundling Fernando Lledo´∗ Department of Mathematics, Max–Planck–Institut f¨ur Gravitationsphysik, University of New South Wales, Albert–Einstein–Institut, Sydney, NSW 2052, Australia. Am M¨uhlenberg 1, [email protected] D–14476 Golm, Germany. [email protected] AMS classification: 81T05, 81T10, 46L60, 46N50 Abstract We analyze the situation of a local quantum field theory with constraints, both indexed by the same set of space–time regions. In particular we find “weak” Haag–Kastler axioms which will ensure that the final constrained theory satisfies the usual Haag–Kastler axioms. Gupta– Bleuler electromagnetism is developed in detail as an example of a theory which satisfies the “weak” Haag–Kastler axioms but not the usual ones. This analysis is done by pure C*– algebraic means without employing any indefinite metric representations, and we obtain the same physical algebra and positive energy representation for it than by the usual means. The price for avoiding the indefinite metric, is the use of nonregular representations and complex valued test functions. We also exhibit the precise connection with the usual indefinite metric representation. We conclude the analysis by comparing the final physical algebra produced by a system of local constrainings with the one obtained from a single global constraining and also consider the issue of reduction by stages. For the usual spectral condition on the generators of the translation group, we also find a “weak” version, and show that the Gupta–Bleuler example satisfies it. arXiv:math-ph/9812022 v2 7 Aug 2000 1 Introduction In many quantum field theories there are constraints consisting of local expressions of the quantum fields, generally written as a selection condition for the physical subspace (p). -
Lagrangian Constraint Analysis of First-Order Classical Field Theories with an Application to Gravity
PHYSICAL REVIEW D 102, 065015 (2020) Lagrangian constraint analysis of first-order classical field theories with an application to gravity † ‡ Verónica Errasti Díez ,1,* Markus Maier ,1,2, Julio A. M´endez-Zavaleta ,1, and Mojtaba Taslimi Tehrani 1,§ 1Max-Planck-Institut für Physik (Werner-Heisenberg-Institut), Föhringer Ring 6, 80805 Munich, Germany 2Universitäts-Sternwarte, Ludwig-Maximilians-Universität München, Scheinerstrasse 1, 81679 Munich, Germany (Received 19 August 2020; accepted 26 August 2020; published 21 September 2020) We present a method that is optimized to explicitly obtain all the constraints and thereby count the propagating degrees of freedom in (almost all) manifestly first-order classical field theories. Our proposal uses as its only inputs a Lagrangian density and the identification of the a priori independent field variables it depends on. This coordinate-dependent, purely Lagrangian approach is complementary to and in perfect agreement with the related vast literature. Besides, generally overlooked technical challenges and problems derived from an incomplete analysis are addressed in detail. The theoretical framework is minutely illustrated in the Maxwell, Proca and Palatini theories for all finite d ≥ 2 spacetime dimensions. Our novel analysis of Palatini gravity constitutes a noteworthy set of results on its own. In particular, its computational simplicity is visible, as compared to previous Hamiltonian studies. We argue for the potential value of both the method and the given examples in the context of generalized Proca and their coupling to gravity. The possibilities of the method are not exhausted by this concrete proposal. DOI: 10.1103/PhysRevD.102.065015 I. INTRODUCTION In this work, we focus on singular classical field theories It is hard to overemphasize the importance of field theory that are manifestly first order and analyze them employing in high-energy physics. -
Arxiv:1505.02430V1 [Math.CT] 10 May 2015 Bundle Functors and Fibrations
Bundle functors and fibrations Anders Kock Introduction The notions of bundle, and bundle functor, are useful and well exploited notions in topology and differential geometry, cf. e.g. [12], as well as in other branches of mathematics. The category theoretic set up relevant for these notions is that of fibred category, likewise a well exploited notion, but for certain considerations in the context of bundle functors, it can be carried further. In particular, we formalize and develop, in terms of fibred categories, some of the differential geometric con- structions: tangent- and cotangent bundles, (being examples of bundle functors, respectively star-bundle functors, as in [12]), as well as jet bundles (where the for- mulation of the functorality properties, in terms of fibered categories, is probably new). Part of the development in the present note was expounded in [11], and is repeated almost verbatim in the Sections 2 and 4 below. These sections may have interest as a piece of pure category theory, not referring to differential geometry. 1 Basics on Cartesian arrows We recall here some classical notions. arXiv:1505.02430v1 [math.CT] 10 May 2015 Let π : X → B be any functor. For α : A → B in B, and for objects X,Y ∈ X with π(X) = A and π(Y ) = B, let homα (X,Y) be the set of arrows h : X → Y in X with π(h) = α. The fibre over A ∈ B is the category, denoted XA, whose objects are the X ∈ X with π(X) = A, and whose arrows are arrows in X which by π map to 1A; such arrows are called vertical (over A). -
Cotangent Bundles
This is page 165 Printer: Opaque this 6 Cotangent Bundles In many mechanics problems, the phase space is the cotangent bundle T ∗Q of a configuration space Q. There is an “intrinsic” symplectic structure on T ∗Q that can be described in various equivalent ways. Assume first that Q is n-dimensional, and pick local coordinates (q1,... ,qn)onQ. Since 1 n ∗ ∈ ∗ i (dq ,... ,dq )isabasis of Tq Q,wecan write any α Tq Q as α = pi dq . 1 n This procedure defines induced local coordinates (q ,... ,q ,p1,... ,pn)on T ∗Q. Define the canonical symplectic form on T ∗Q by i Ω=dq ∧ dpi. This defines a two-form Ω, which is clearly closed, and in addition, it can be checked to be independent of the choice of coordinates (q1,... ,qn). Furthermore, observe that Ω is locally constant, that is, the coefficient i multiplying the basis forms dq ∧ dpi, namely the number 1, does not ex- 1 n plicitly depend on the coordinates (q ,... ,q ,p1,... ,pn)ofphase space points. In this section we show how to construct Ω intrinsically, and then we will study this canonical symplectic structure in some detail. 6.1 The Linear Case To motivate a coordinate-independent definition of Ω, consider the case in which Q is a vector space W (which could be infinite-dimensional), so that T ∗Q = W × W ∗.Wehave already described the canonical two-form on 166 6. Cotangent Bundles W × W ∗: Ω(w,α)((u, β), (v, γ)) = γ,u−β,v , (6.1.1) where (w, α) ∈ W × W ∗ is the base point, u, v ∈ W , and β,γ ∈ W ∗. -
The Hypoelliptic Laplacian on the Cotangent Bundle
JOURNAL OF THE AMERICAN MATHEMATICAL SOCIETY Volume 18, Number 2, Pages 379–476 S 0894-0347(05)00479-0 Article electronically published on February 28, 2005 THE HYPOELLIPTIC LAPLACIAN ON THE COTANGENT BUNDLE JEAN-MICHEL BISMUT Contents Introduction 380 1. Generalized metrics and determinants 386 1.1. Determinants 386 1.2. A generalized metric on E· 387 · 1.3. The Hodge theory of hE 387 1.4. A generalized metric on det E· 389 1.5. Determinant of the generalized Laplacian and generalized metrics 391 1.6. Truncating the spectrum of the generalized Laplacian 392 1.7. Generalized metrics on determinant bundles 393 1.8. Determinants and flat superconnections 394 1.9. The Hodge theorem as an open condition 395 1.10. Generalized metrics and flat superconnections 395 1.11. Analyticity and the Hodge condition 397 1.12. The equivariant determinant 397 2. The adjoint of the de Rham operator on the cotangent bundle 399 2.1. Clifford algebras 400 2.2. Vector spaces and bilinear forms 400 2.3. The adjoint of the de Rham operator with respect to a nondegenerate bilinear form 402 2.4. The symplectic adjoint of the de Rham operator 403 2.5. The de Rham operator on T ∗X and its symplectic adjoint 404 ∗ 2.6. A bilinear form on T ∗X and the adjoint of dT X 407 2.7. A fundamental symmetry 408 2.8. A Hamiltonian function 409 2.9. The symmetry in the case where H is r-invariant 412 2.10. Poincar´e duality 412 2.11. A conjugation of the de Rham operator 413 2.12. -
On Gauge Fixing and Quantization of Constrained Hamiltonian Systems
BEFE IC/89/118 INTERIMATIOIMAL CENTRE FOR THEORETICAL PHYSICS ON GAUGE FIXING AND QUANTIZATION OF CONSTRAINED HAMILTONIAN SYSTEMS Omer F. Dayi INTERNATIONAL ATOMIC ENERGY AGENCY UNITED NATIONS EDUCATIONAL, SCIENTIFIC AND CULTURAL ORGANIZATION 1989 MIRAMARE-TRIESTE IC/89/118 International Atomic Energy Agency and United Nations Educational Scientific and Cultural Organization INTERNATIONAL CENTRE FOR THEORETICAL PHYSICS Quantization of a classical Hamiltonian system can be achieved by the canonical quantization method [1]. If we ignore the ordering problems, it consists of replacing the classical Poisson brackets by quantum commuta- tors when classically all the states on the phase space are accessible. This is no longer correct in the presence of constraints. An approach due to Dirac ON GAUGE FIXING AND QUANTIZATION [2] is widely used for quantizing the constrained Hamiltonian systems |3|, OF CONSTRAINED HAMILTONIAN SYSTEMS' [4]. In spite of its wide use there is confusion in the application of it in the physics literature. Obtaining the Hamiltonian which Bhould be used in gauge theories is not well-understood. This derives from the misunder- standing of the gauge fixing procedure. One of the aims of this work is to OmerF.Dayi" clarify this issue. The constraints, which are present when there are some irrelevant phase International Centre for Theoretical Physics, Trieste, Italy. space variables, can be classified as first and second class. Second class constraints are eliminated by altering some of the original Poisson bracket relations which is equivalent to imply the vanishing of the constraints as strong equations by using the Dirac procedure [2] or another method |Sj. ABSTRACT Vanishing of second class constraints strongly leads to a reduction in the number of the phase apace variables. -
Manifolds, Tangent Vectors and Covectors
Physics 250 Fall 2015 Notes 1 Manifolds, Tangent Vectors and Covectors 1. Introduction Most of the “spaces” used in physical applications are technically differentiable man- ifolds, and this will be true also for most of the spaces we use in the rest of this course. After a while we will drop the qualifier “differentiable” and it will be understood that all manifolds we refer to are differentiable. We will build up the definition in steps. A differentiable manifold is basically a topological manifold that has “coordinate sys- tems” imposed on it. Recall that a topological manifold is a topological space that is Hausdorff and locally homeomorphic to Rn. The number n is the dimension of the mani- fold. On a topological manifold, we can talk about the continuity of functions, for example, of functions such as f : M → R (a “scalar field”), but we cannot talk about the derivatives of such functions. To talk about derivatives, we need coordinates. 2. Charts and Coordinates Generally speaking it is impossible to cover a manifold with a single coordinate system, so we work in “patches,” technically charts. Given a topological manifold M of dimension m, a chart on M is a pair (U, φ), where U ⊂ M is an open set and φ : U → V ⊂ Rm is a homeomorphism. See Fig. 1. Since φ is a homeomorphism, V is also open (in Rm), and φ−1 : V → U exists. If p ∈ U is a point in the domain of φ, then φ(p) = (x1,...,xm) is the set of coordinates of p with respect to the given chart. -
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.