Module II: Relativity and Electrodynamics Lecture 5: Metric and Higher-Rank 4-Tensors
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Arxiv:0911.0334V2 [Gr-Qc] 4 Jul 2020
Classical Physics: Spacetime and Fields Nikodem Poplawski Department of Mathematics and Physics, University of New Haven, CT, USA Preface We present a self-contained introduction to the classical theory of spacetime and fields. This expo- sition is based on the most general principles: the principle of general covariance (relativity) and the principle of least action. The order of the exposition is: 1. Spacetime (principle of general covariance and tensors, affine connection, curvature, metric, tetrad and spin connection, Lorentz group, spinors); 2. Fields (principle of least action, action for gravitational field, matter, symmetries and conservation laws, gravitational field equations, spinor fields, electromagnetic field, action for particles). In this order, a particle is a special case of a field existing in spacetime, and classical mechanics can be derived from field theory. I dedicate this book to my Parents: Bo_zennaPop lawska and Janusz Pop lawski. I am also grateful to Chris Cox for inspiring this book. The Laws of Physics are simple, beautiful, and universal. arXiv:0911.0334v2 [gr-qc] 4 Jul 2020 1 Contents 1 Spacetime 5 1.1 Principle of general covariance and tensors . 5 1.1.1 Vectors . 5 1.1.2 Tensors . 6 1.1.3 Densities . 7 1.1.4 Contraction . 7 1.1.5 Kronecker and Levi-Civita symbols . 8 1.1.6 Dual densities . 8 1.1.7 Covariant integrals . 9 1.1.8 Antisymmetric derivatives . 9 1.2 Affine connection . 10 1.2.1 Covariant differentiation of tensors . 10 1.2.2 Parallel transport . 11 1.2.3 Torsion tensor . 11 1.2.4 Covariant differentiation of densities . -
On the Representation of Symmetric and Antisymmetric Tensors
Max-Planck-Institut fur¨ Mathematik in den Naturwissenschaften Leipzig On the Representation of Symmetric and Antisymmetric Tensors (revised version: April 2017) by Wolfgang Hackbusch Preprint no.: 72 2016 On the Representation of Symmetric and Antisymmetric Tensors Wolfgang Hackbusch Max-Planck-Institut Mathematik in den Naturwissenschaften Inselstr. 22–26, D-04103 Leipzig, Germany [email protected] Abstract Various tensor formats are used for the data-sparse representation of large-scale tensors. Here we investigate how symmetric or antiymmetric tensors can be represented. The analysis leads to several open questions. Mathematics Subject Classi…cation: 15A69, 65F99 Keywords: tensor representation, symmetric tensors, antisymmetric tensors, hierarchical tensor format 1 Introduction We consider tensor spaces of huge dimension exceeding the capacity of computers. Therefore the numerical treatment of such tensors requires a special representation technique which characterises the tensor by data of moderate size. These representations (or formats) should also support operations with tensors. Examples of operations are the addition, the scalar product, the componentwise product (Hadamard product), and the matrix-vector multiplication. In the latter case, the ‘matrix’belongs to the tensor space of Kronecker matrices, while the ‘vector’is a usual tensor. In certain applications the subspaces of symmetric or antisymmetric tensors are of interest. For instance, fermionic states in quantum chemistry require antisymmetry, whereas bosonic systems are described by symmetric tensors. The appropriate representation of (anti)symmetric tensors is seldom discussed in the literature. Of course, all formats are able to represent these tensors since they are particular examples of general tensors. However, the special (anti)symmetric format should exclusively produce (anti)symmetric tensors. -
Tensor Calculus and Differential Geometry
Course Notes Tensor Calculus and Differential Geometry 2WAH0 Luc Florack March 10, 2021 Cover illustration: papyrus fragment from Euclid’s Elements of Geometry, Book II [8]. Contents Preface iii Notation 1 1 Prerequisites from Linear Algebra 3 2 Tensor Calculus 7 2.1 Vector Spaces and Bases . .7 2.2 Dual Vector Spaces and Dual Bases . .8 2.3 The Kronecker Tensor . 10 2.4 Inner Products . 11 2.5 Reciprocal Bases . 14 2.6 Bases, Dual Bases, Reciprocal Bases: Mutual Relations . 16 2.7 Examples of Vectors and Covectors . 17 2.8 Tensors . 18 2.8.1 Tensors in all Generality . 18 2.8.2 Tensors Subject to Symmetries . 22 2.8.3 Symmetry and Antisymmetry Preserving Product Operators . 24 2.8.4 Vector Spaces with an Oriented Volume . 31 2.8.5 Tensors on an Inner Product Space . 34 2.8.6 Tensor Transformations . 36 2.8.6.1 “Absolute Tensors” . 37 CONTENTS i 2.8.6.2 “Relative Tensors” . 38 2.8.6.3 “Pseudo Tensors” . 41 2.8.7 Contractions . 43 2.9 The Hodge Star Operator . 43 3 Differential Geometry 47 3.1 Euclidean Space: Cartesian and Curvilinear Coordinates . 47 3.2 Differentiable Manifolds . 48 3.3 Tangent Vectors . 49 3.4 Tangent and Cotangent Bundle . 50 3.5 Exterior Derivative . 51 3.6 Affine Connection . 52 3.7 Lie Derivative . 55 3.8 Torsion . 55 3.9 Levi-Civita Connection . 56 3.10 Geodesics . 57 3.11 Curvature . 58 3.12 Push-Forward and Pull-Back . 59 3.13 Examples . 60 3.13.1 Polar Coordinates in the Euclidean Plane . -
The Language of Differential Forms
Appendix A The Language of Differential Forms This appendix—with the only exception of Sect.A.4.2—does not contain any new physical notions with respect to the previous chapters, but has the purpose of deriving and rewriting some of the previous results using a different language: the language of the so-called differential (or exterior) forms. Thanks to this language we can rewrite all equations in a more compact form, where all tensor indices referred to the diffeomorphisms of the curved space–time are “hidden” inside the variables, with great formal simplifications and benefits (especially in the context of the variational computations). The matter of this appendix is not intended to provide a complete nor a rigorous introduction to this formalism: it should be regarded only as a first, intuitive and oper- ational approach to the calculus of differential forms (also called exterior calculus, or “Cartan calculus”). The main purpose is to quickly put the reader in the position of understanding, and also independently performing, various computations typical of a geometric model of gravity. The readers interested in a more rigorous discussion of differential forms are referred, for instance, to the book [22] of the bibliography. Let us finally notice that in this appendix we will follow the conventions introduced in Chap. 12, Sect. 12.1: latin letters a, b, c,...will denote Lorentz indices in the flat tangent space, Greek letters μ, ν, α,... tensor indices in the curved manifold. For the matter fields we will always use natural units = c = 1. Also, unless otherwise stated, in the first three Sects. -
Semi-Classical Scalar Propagators in Curved Backgrounds: Formalism and Ambiguities
Semi-classical scalar propagators in curved backgrounds : formalism and ambiguities J. Grain1,2 & A. Barrau1 1Laboratory for Subatomic Physics and Cosmology, Grenoble Universit´es, CNRS, IN2P3 53, avenue de Martyrs, 38026 Grenoble cedex, France 2AstroParticle & Cosmology, Universit´eParis 7, CNRS, IN2P3 10, rue Alice Domon et L´eonie Duquet, 75205 Paris cedex 13, France Abstract The phenomenology of quantum systems in curved space-times is among the most fascinating fields of physics, allowing –often at the gedankenexperiment level– constraints on tentative the- ories of quantum gravity. Determining the dynamics of fields in curved backgrounds remains however a complicated task because of the highly intricate partial differential equations in- volved, especially when the space metric exhibits no symmetry. In this article, we provide –in a pedagogical way– a general formalism to determine this dynamics at the semi-classical order. To this purpose, a generic expression for the semi-classical propagator is computed and the equation of motion for the probability four-current is derived. Those results underline a direct analogy between the computation of the propagator in general relativistic quantum mechanics and the computation of the propagator for stationary systems in non-relativistic quantum me- chanics. PACS numbers: 04.62.+v, 11.15.Kc arXiv:0705.4393v1 [hep-th] 30 May 2007 1 Introduction The dynamics of a scalar field propagating in a curved background is governed by partial differ- ential equations which, in most cases, have no analytical solution. Investigating the behavior of those fields in the semi-classical approximation is a promising alternative to numerical studies, allowing accurate predictions for many phenomena including the Hawking radiation process [1, 2, 3, 4] and the primordial power spectrum [5, 6]. -
Constructing $ P, N $-Forms from $ P $-Forms Via the Hodge Star Operator and the Exterior Derivative
Constructing p, n-forms from p-forms via the Hodge star operator and the exterior derivative Jun-Jin Peng1,2∗ 1School of Physics and Electronic Science, Guizhou Normal University, Guiyang, Guizhou 550001, People’s Republic of China; 2Guizhou Provincial Key Laboratory of Radio Astronomy and Data Processing, Guizhou Normal University, Guiyang, Guizhou 550001, People’s Republic of China Abstract In this paper, we aim to explore the properties and applications on the operators consisting of the Hodge star operator together with the exterior derivative, whose action on an arbi- trary p-form field in n-dimensional spacetimes makes its form degree remain invariant. Such operations are able to generate a variety of p-forms with the even-order derivatives of the p- form. To do this, we first investigate the properties of the operators, such as the Laplace-de Rham operator, the codifferential and their combinations, as well as the applications of the arXiv:1909.09921v2 [gr-qc] 23 Mar 2020 operators in the construction of conserved currents. On basis of two general p-forms, then we construct a general n-form with higher-order derivatives. Finally, we propose that such an n-form could be applied to define a generalized Lagrangian with respect to a p-form field according to the fact that it incudes the ordinary Lagrangians for the p-form and scalar fields as special cases. Keywords: p-form; Hodge star; Laplace-de Rham operator; Lagrangian for p-form. ∗ [email protected] 1 1 Introduction Differential forms are a powerful tool developed to deal with the calculus in differential geom- etry and tensor analysis. -
Tensors (February 5, 2011)
Lars Davidson: Numerical Methods for Turbulent Flow http://www.tfd.chalmers.se/gr-kurs/MTF071 59 Tensors (February 5, 2011) The convection-diffusion equation for temperature reads ∂ ∂ ∂ (ρUT ) + (ρV T ) + (ρW T ) = ∂x ∂y ∂z ∂ ∂T ∂ ∂T ∂ ∂T Γ + Γ + Γ ∂x ∂x ∂y ∂y ∂z ∂z Using tensor notation it can be written as ∂ ∂ ∂T (ρUjT ) = Γ ∂xj ∂xj ∂xj The Navier-Stokes equation reads (incompr. and µ = const.) ∂ ∂ ∂ (UU) + (VU) + (WU) = ∂x ∂y ∂z 1 ∂P ∂2U ∂2U ∂2U + ν + + − ρ ∂x ∂x2 ∂y2 ∂z2 ∂ ∂ ∂ (UV ) + (V V ) + (W V ) = ∂x ∂y ∂z 1 ∂P ∂2V ∂2V ∂2V + ν + + − ρ ∂x ∂x2 ∂y2 ∂z2 ∂ ∂ ∂ (UW ) + (VW ) + (WW ) = ∂x ∂y ∂z 1 ∂P ∂2W ∂2W ∂2W + ν + + − ρ ∂x ∂x2 ∂y2 ∂z2 Using tensor notation it can be written as 2 ∂ 1 ∂P ∂ Ui (UjUi) = + ν (62) ∂xj −ρ ∂xi ∂xj∂xj Tensors Lars Davidson: Numerical Methods for Turbulent Flow http://www.tfd.chalmers.se/gr-kurs/MTF071 60 a: A tensor of zeroth rank (scalar) 2 ¨* ¨ ai = 1 ai: A tensor of first rank (vector) ¨ ¨ 0 aij: A tensor of second rank (tensor) A common tensor in fluid mechanics (and solid mechan- ics) is the stress tensor σij σ11 σ12 σ13 σij = σ21 σ22 σ23 σ31 σ32 σ33 It is symmetric, i.e. σij = σji. For fully, developed flow in a 2D channel (flow between infinite plates) σij has the form: dU1 dU σ12 = σ21 = µ (= µ ) dx2 dy and the other components are zero. As indicated above, the coordinate directions (x1,x2,x3) correspond to (x,y,z), and the velocity vector (U1,U2,U3) corresponds to (U,V,W ). -
Geodesic Witten Diagrams with Anti-Symmetric Exchange
OU-HET 939 Geodesic Witten diagrams with anti-symmetric exchange Kotaro Tamaoka Department of Physics, Osaka University Toyonaka, Osaka 560-0043, JAPAN [email protected] Abstract We show the AdS/CFT correspondence between the conformal partial wave and the geodesic Witten diagram with anti-symmetric exchange. To this end, we introduce the embedding space formalism for anti-symmetric fields in AdS. Then we prove that the geodesic Witten diagram satisfies the conformal Casimir equation and the appropriate boundary condition. Furthermore, we discuss the connection between the geodesic Witten diagram and the shadow formalism by using the split representation of harmonic function for anti-symmetric fields. We also discuss the 3pt geodesic Witten diagrams and its extension to the mixed-symmetric tensors. arXiv:1707.07934v1 [hep-th] 25 Jul 2017 Contents 1 Introduction 1 2 Embedding formalism in AdSd+1 2 2.1 Anti-symmetric tensors in embedding space . .2 2.2 Anti-symmetric tensor propagators in embedding space . .4 2.2.1 Bulk-bulk propagator . .5 2.2.2 Bulk-boundary propagator . .5 2.3 Bulk-boundary propagator for the mixed-symmetric tensor . .6 3 Three point diagrams on the geodesics 7 3.1 Three point diagrams with p-form . .7 3.2 Scalar-vector-hook . .9 4 Conformal partial wave from geodesic Witten diagram 10 4.1 Proof by conformal Casimir equation . 10 4.2 Connection to the shadow formalism . 12 5 Summary and Discussion 13 A Split representation of the bulk-bulk propagators 13 1 Introduction Conformal Field Theory (CFT) has been studied in various contexts, for example, critical phenomena [1], exactly solvable models in two dimension [2], and the AdS/CFT correspondence [3, 4, 5]. -
C FW Math 321, Mar 5, 2004 Tensor Product and Tensors the Tensor Product Is Another Way to Multiply Vectors, in Addition To
c FW Math 321, Mar 5, 2004 Tensor Product and Tensors The tensor product is another way to multiply vectors, in addition to the dot and cross products. The tensor product of vectors a and b is denoted a ⊗ b in mathematics but simply ab with no special product symbol in mechanics. The result of the tensor product of a and b is not a scalar, like the dot product, nor a (pseudo)-vector like the cross-product. It is a new object called a tensor of second order ab that is defined indirectly through the following dot products between the tensor ab and any vector v: (ab) · v ≡ a(b · v), v · (ab) ≡ (v · a)b, ∀v. (1) The right hand sides of these equations are readily understood. These definitions clearly imply that ab 6= ba, the tensor product does not commute. However, v · (ab) = (ba) · v ≡ (ab)T · v, ∀v. (2) The product ba is the transpose of ab, denoted with a ‘T 0 superscript: (ab)T ≡ ba. We also deduce the following distributive properties, from (1): (ab) · (αu + βv) = α(ab) · u + β(ab) · v, (3) which hold for any scalars α, β and vectors u, v. A general tensor of 2nd order can be defined similarly as an object T such that T · v is a vector and T · (αu + βv) = αT · u + βT · v, ∀α, β, u, v. (4) Thus T · v is a linear transformation of v and T is a linear operator. The linearity property (4) allows us to figure out the effect of T on any vector v once we know its effect on a set of basis vectors. -
An Introduction to Space–Time Exterior Calculus
mathematics Article An Introduction to Space–Time Exterior Calculus Ivano Colombaro 1,* , Josep Font-Segura 1 and Alfonso Martinez 1 1 Department of Information and Communication Technologies, Universitat Pompeu Fabra, 08018 Barcelona, Spain; [email protected] (J.F.-S.); [email protected] (A.M.) * Correspondence: [email protected]; Tel.: +34-93-542-1496 Received: 21 May 2019; Accepted: 18 June 2019; Published: 21 June 2019 Abstract: The basic concepts of exterior calculus for space–time multivectors are presented: Interior and exterior products, interior and exterior derivatives, oriented integrals over hypersurfaces, circulation and flux of multivector fields. Two Stokes theorems relating the exterior and interior derivatives with circulation and flux, respectively, are derived. As an application, it is shown how the exterior-calculus space–time formulation of the electromagnetic Maxwell equations and Lorentz force recovers the standard vector-calculus formulations, in both differential and integral forms. Keywords: exterior calculus, exterior algebra, electromagnetism, Maxwell equations, differential forms, tensor calculus 1. Introduction Vector calculus has, since its introduction by J. W. Gibbs [1] and Heaviside, been the tool of choice to represent many physical phenomena. In mechanics, hydrodynamics and electromagnetism, quantities such as forces, velocities and currents are modeled as vector fields in space, while flux, circulation, divergence or curl describe operations on the vector fields themselves. With relativity theory, it was observed that space and time are not independent but just coordinates in space–time [2] (pp. 111–120). Tensors like the Faraday tensor in electromagnetism were quickly adopted as a natural representation of fields in space–time [3] (pp. -
2 Differential Geometry
2 Differential Geometry The language of General relativity is Differential Geometry. The preset chap- ter provides a brief review of the ideas and notions of Differential Geometry that will be used in the book. In this role, it also serves the purpose of setting the notation and conventions to be used througout the book. The chapter is not intended as an introduction to Differential Geometry and as- sumes a prior knowledge of the subject at the level, say, of the first chapter of Choquet-Bruhat (2008) or Stewart (1991), or chapters 2 and 3 of Wald (1984). As such, rigorous definitions of concepts are not treated in depth —the reader is, in any case, refered to the literature provided in the text, and that given in the final section of the chapter. Instead, the decision has been taken of discussing at some length topics which may not be regarded as belonging to the standard bagage of a relativist. In particular, some detail is provided in the discussion of general (i.e. non Levi-Civita) connections, the sometimes 1+3 split of tensors (i.e. a split based on a congruence of timelike curves, rather than on a foliation as in the usual 3 + 1), and a discussion of submanifolds using a frame formalism. A discussion of conformal geometry has been left out of this chapter and will be undertaken in Chapter 5. 2.1 Manifolds The basic object of study in Differential Geometry is a differentiable man- ifold . Intuitively, a manifold is a space that locally looks like Rn for some n N. -
1 Special Relativity
1 Special relativity 1.1 Minkowski space Inertial frames and the principle of relativity Newton’s Lex Prima (or the Galilean law of inertia) states: Each force-less mass point stays at rest or moves on a straight line at constant speed. In a Cartesian inertial coordinate system, Newton’s lex prima becomes d2x d2y d2z = = = 0 . (1.1) dt2 dt2 dt2 Most often, we call such a coordinate system just an inertial frame. Newton’s first law is not just a trivial consequence of its second one, but may be seen as practical definition of those reference frames for which his following laws are valid. Since the symmetries of Euclidean space, translations a and rotations R, leave Eq. (1.1) invariant, all frames connected by x′ = Rx + a to an inertial frame are inertial frames too. Additionally, proper Galilean transformations x′ = x + vt connect inertial frames moving with relative speed v. The principle of relativity states that the physics in all inertial frames is the same. If we consider two frames with relative velocity along the x direction, then the most general linear transformation between the two frames is t′ At + Bx At + Bx ′ x Dt + Ex A(x vt) ′ = = − . (1.2) y y y ′ z z z Newtonian physics assumes the existence of an absolute time, t = t′, and thus A = 1 and B = 0. This leads to the “common sense” addition law of velocities. Time differences ∆t and space differences 2 2 2 2 ∆x12 = (x1 x2) + (y1 y2) + (z1 z2) (1.3) − − − are separately invariant. Lorentz transformations In special relativity, we replace the Galilean transformations as symmetry group of space and time by Lorentz transformations Λ.