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Connections on Bundles Md
Dhaka Univ. J. Sci. 60(2): 191-195, 2012 (July) Connections on Bundles Md. Showkat Ali, Md. Mirazul Islam, Farzana Nasrin, Md. Abu Hanif Sarkar and Tanzia Zerin Khan Department of Mathematics, University of Dhaka, Dhaka 1000, Bangladesh, Email: [email protected] Received on 25. 05. 2011.Accepted for Publication on 15. 12. 2011 Abstract This paper is a survey of the basic theory of connection on bundles. A connection on tangent bundle , is called an affine connection on an -dimensional smooth manifold . By the general discussion of affine connection on vector bundles that necessarily exists on which is compatible with tensors. I. Introduction = < , > (2) In order to differentiate sections of a vector bundle [5] or where <, > represents the pairing between and ∗. vector fields on a manifold we need to introduce a Then is a section of , called the absolute differential structure called the connection on a vector bundle. For quotient or the covariant derivative of the section along . example, an affine connection is a structure attached to a differentiable manifold so that we can differentiate its Theorem 1. A connection always exists on a vector bundle. tensor fields. We first introduce the general theorem of Proof. Choose a coordinate covering { }∈ of . Since connections on vector bundles. Then we study the tangent vector bundles are trivial locally, we may assume that there is bundle. is a -dimensional vector bundle determine local frame field for any . By the local structure of intrinsically by the differentiable structure [8] of an - connections, we need only construct a × matrix on dimensional smooth manifold . each such that the matrices satisfy II. -
Riemannian Geometry and Multilinear Tensors with Vector Fields on Manifolds Md
International Journal of Scientific & Engineering Research, Volume 5, Issue 9, September-2014 157 ISSN 2229-5518 Riemannian Geometry and Multilinear Tensors with Vector Fields on Manifolds Md. Abdul Halim Sajal Saha Md Shafiqul Islam Abstract-In the paper some aspects of Riemannian manifolds, pseudo-Riemannian manifolds, Lorentz manifolds, Riemannian metrics, affine connections, parallel transport, curvature tensors, torsion tensors, killing vector fields, conformal killing vector fields are focused. The purpose of this paper is to develop the theory of manifolds equipped with Riemannian metric. I have developed some theorems on torsion and Riemannian curvature tensors using affine connection. A Theorem 1.20 named “Fundamental Theorem of Pseudo-Riemannian Geometry” has been established on Riemannian geometry using tensors with metric. The main tools used in the theorem of pseudo Riemannian are tensors fields defined on a Riemannian manifold. Keywords: Riemannian manifolds, pseudo-Riemannian manifolds, Lorentz manifolds, Riemannian metrics, affine connections, parallel transport, curvature tensors, torsion tensors, killing vector fields, conformal killing vector fields. —————————— —————————— I. Introduction (c) { } is a family of open sets which covers , that is, 푖 = . Riemannian manifold is a pair ( , g) consisting of smooth 푈 푀 manifold and Riemannian metric g. A manifold may carry a (d) ⋃ is푈 푖푖 a homeomorphism푀 from onto an open subset of 푀 ′ further structure if it is endowed with a metric tensor, which is a 푖 . 푖 푖 휑 푈 푈 natural generation푀 of the inner product between two vectors in 푛 ℝ to an arbitrary manifold. Riemannian metrics, affine (e) Given and such that , the map = connections,푛 parallel transport, curvature tensors, torsion tensors, ( ( ) killingℝ vector fields and conformal killing vector fields play from푖 푗 ) to 푖 푗 is infinitely푖푗 −1 푈 푈 푈 ∩ 푈 ≠ ∅ 휓 important role to develop the theorem of Riemannian manifolds. -
1 HESTENES' TETRAD and SPIN CONNECTIONS Frank
HESTENES’ TETRAD AND SPIN CONNECTIONS Frank Reifler and Randall Morris Lockheed Martin Corporation MS2 (137-205) 199 Borton Landing Road Moorestown, New Jersey 08057 ABSTRACT Defining a spin connection is necessary for formulating Dirac’s bispinor equation in a curved space-time. Hestenes has shown that a bispinor field is equivalent to an orthonormal tetrad of vector fields together with a complex scalar field. In this paper, we show that using Hestenes’ tetrad for the spin connection in a Riemannian space-time leads to a Yang-Mills formulation of the Dirac Lagrangian in which the bispinor field Ψ is mapped to a set of × K ρ SL(2,R) U(1) gauge potentials Fα and a complex scalar field . This result was previously proved for a Minkowski space-time using Fierz identities. As an application we derive several different non-Riemannian spin connections found in the literature directly from an arbitrary K linear connection acting on the tensor fields (Fα ,ρ) . We also derive spin connections for which Dirac’s bispinor equation is form invariant. Previous work has not considered form invariance of the Dirac equation as a criterion for defining a general spin connection. 1 I. INTRODUCTION Defining a spin connection to replace the partial derivatives in Dirac’s bispinor equation in a Minkowski space-time, is necessary for the formulation of Dirac’s bispinor equation in a curved space-time. All the spin connections acting on bispinors found in the literature first introduce a local orthonormal tetrad field on the space-time manifold and then require that the Dirac Lagrangian be invariant under local change of tetrad [1] – [8]. -
Arxiv:1907.02341V1 [Gr-Qc]
Different types of torsion and their effect on the dynamics of fields Subhasish Chakrabarty1, ∗ and Amitabha Lahiri1, † 1S. N. Bose National Centre for Basic Sciences Block - JD, Sector - III, Salt Lake, Kolkata - 700106 One of the formalisms that introduces torsion conveniently in gravity is the vierbein-Einstein- Palatini (VEP) formalism. The independent variables are the vierbein (tetrads) and the components of the spin connection. The latter can be eliminated in favor of the tetrads using the equations of motion in the absence of fermions; otherwise there is an effect of torsion on the dynamics of fields. We find that the conformal transformation of off-shell spin connection is not uniquely determined unless additional assumptions are made. One possibility gives rise to Nieh-Yan theory, another one to conformally invariant torsion; a one-parameter family of conformal transformations interpolates between the two. We also find that for dynamically generated torsion the spin connection does not have well defined conformal properties. In particular, it affects fermions and the non-minimally coupled conformal scalar field. Keywords: Torsion, Conformal transformation, Palatini formulation, Conformal scalar, Fermion arXiv:1907.02341v1 [gr-qc] 4 Jul 2019 ∗ [email protected] † [email protected] 2 I. INTRODUCTION Conventionally, General Relativity (GR) is formulated purely from a metric point of view, in which the connection coefficients are given by the Christoffel symbols and torsion is set to zero a priori. Nevertheless, it is always interesting to consider a more general theory with non-zero torsion. The first attempt to formulate a theory of gravity that included torsion was made by Cartan [1]. -
FROM DIFFERENTIATION in AFFINE SPACES to CONNECTIONS Jovana -Duretic 1. Introduction Definition 1. We Say That a Real Valued
THE TEACHING OF MATHEMATICS 2015, Vol. XVIII, 2, pp. 61–80 FROM DIFFERENTIATION IN AFFINE SPACES TO CONNECTIONS Jovana Dureti´c- Abstract. Connections and covariant derivatives are usually taught as a basic concept of differential geometry, or more precisely, of differential calculus on smooth manifolds. In this article we show that the need for covariant derivatives may arise, or at lest be motivated, even in a linear situation. We show how a generalization of the notion of a derivative of a function to a derivative of a map between affine spaces naturally leads to the notion of a connection. Covariant derivative is defined in the framework of vector bundles and connections in a way which preserves standard properties of derivatives. A special attention is paid on the role played by zero–sets of a first derivative in several contexts. MathEduc Subject Classification: I 95, G 95 MSC Subject Classification: 97 I 99, 97 G 99, 53–01 Key words and phrases: Affine space; second derivative; connection; vector bun- dle. 1. Introduction Definition 1. We say that a real valued function f :(a; b) ! R is differen- tiable at a point x0 2 (a; b) ½ R if a limit f(x) ¡ f(x ) lim 0 x!x0 x ¡ x0 0 exists. We denote this limit by f (x0) and call it a derivative of a function f at a point x0. We can write this limit in a different form, as 0 f(x0 + h) ¡ f(x0) (1) f (x0) = lim : h!0 h This expression makes sense if the codomain of a function is Rn, or more general, if the codomain is a normed vector space. -
3. Introducing Riemannian Geometry
3. Introducing Riemannian Geometry We have yet to meet the star of the show. There is one object that we can place on a manifold whose importance dwarfs all others, at least when it comes to understanding gravity. This is the metric. The existence of a metric brings a whole host of new concepts to the table which, collectively, are called Riemannian geometry.Infact,strictlyspeakingwewillneeda slightly di↵erent kind of metric for our study of gravity, one which, like the Minkowski metric, has some strange minus signs. This is referred to as Lorentzian Geometry and a slightly better name for this section would be “Introducing Riemannian and Lorentzian Geometry”. However, for our immediate purposes the di↵erences are minor. The novelties of Lorentzian geometry will become more pronounced later in the course when we explore some of the physical consequences such as horizons. 3.1 The Metric In Section 1, we informally introduced the metric as a way to measure distances between points. It does, indeed, provide this service but it is not its initial purpose. Instead, the metric is an inner product on each vector space Tp(M). Definition:Ametric g is a (0, 2) tensor field that is: Symmetric: g(X, Y )=g(Y,X). • Non-Degenerate: If, for any p M, g(X, Y ) =0forallY T (M)thenX =0. • 2 p 2 p p With a choice of coordinates, we can write the metric as g = g (x) dxµ dx⌫ µ⌫ ⌦ The object g is often written as a line element ds2 and this expression is abbreviated as 2 µ ⌫ ds = gµ⌫(x) dx dx This is the form that we saw previously in (1.4). -
The Category of Affine Connection Control Systems 3
Proceedings of the 39th IEEE Conference on Decision and Control pages 5119{5124, December 2000 doi: 10.1109/CDC.2001.914762 2000 IEEE. Personal use of this material is permitted. However, permission to reprint/republish this material for advertising or promotional purposes or for creating new collective works for resale or redistribution to servers or lists, or to reuse any copyrighted component of this work in other works must be obtained from the IEEE The category of affine connection control systems∗ Andrew D. Lewisy 2000/02/28 Last updated: 2003/07/23 Abstract The category of affine connection control systems is one whose objects are control systems whose drift vector field is the geodesic spray of an affine connection, and whose control vector fields are vertical lifts to the tangent bundle of vector fields on configu- ration space. We investigate morphisms (feedback transformations) in this category. Keywords. control of mechanical systems, affine connections AMS Subject Classifications (2020). 53B05, 70Q05, 93B29 1. Introduction It is apparent that the study of what we will in this paper call “affine connection control systems" has a significant r^oleto play in the field of mechanical control systems. In a series of papers, [e.g., Bullo, Leonard, and Lewis 2000, Lewis 1998, Lewis 1999, Lewis and Murray 1997a, Lewis and Murray 1997b], the author and various coauthors have shown how the affine connection framework is useful in looking at mechanical systems whose Lagrangian is the kinetic energy with respect to a Riemannian metric, possibly in the presence of constraints linear in velocity [e.g., Lewis 1997, Lewis 2000]. -
Weyl's Spin Connection
THE SPIN CONNECTION IN WEYL SPACE c William O. Straub, PhD Pasadena, California “The use of general connections means asking for trouble.” —Abraham Pais In addition to his seminal 1929 exposition on quantum mechanical gauge invariance1, Hermann Weyl demonstrated how the concept of a spinor (essentially a flat-space two-component quantity with non-tensor- like transformation properties) could be carried over to the curved space of general relativity. Prior to Weyl’s paper, spinors were recognized primarily as mathematical objects that transformed in the space of SU (2), but in 1928 Dirac showed that spinors were fundamental to the quantum mechanical description of spin—1/2 particles (electrons). However, the spacetime stage that Dirac’s spinors operated in was still Lorentzian. Because spinors are neither scalars nor vectors, at that time it was unclear how spinors behaved in curved spaces. Weyl’s paper provided a means for this description using tetrads (vierbeins) as the necessary link between Lorentzian space and curved Riemannian space. Weyl’selucidation of spinor behavior in curved space and his development of the so-called spin connection a ab ! band the associated spin vector ! = !ab was noteworthy, but his primary purpose was to demonstrate the profound connection between quantum mechanical gauge invariance and the electromagnetic field. Weyl’s 1929 paper served to complete his earlier (1918) theory2 in which Weyl attempted to derive electrodynamics from the geometrical structure of a generalized Riemannian manifold via a scale-invariant transformation of the metric tensor. This attempt failed, but the manifold he discovered (known as Weyl space), is still a subject of interest in theoretical physics. -
Spin Connection Resonance in Gravitational General Relativity∗
Vol. 38 (2007) ACTA PHYSICA POLONICA B No 6 SPIN CONNECTION RESONANCE IN GRAVITATIONAL GENERAL RELATIVITY∗ Myron W. Evans Alpha Institute for Advanced Study (AIAS) (Received August 16, 2006) The equations of gravitational general relativity are developed with Cartan geometry using the second Cartan structure equation and the sec- ond Bianchi identity. These two equations combined result in a second order differential equation with resonant solutions. At resonance the force due to gravity is greatly amplified. When expressed in vector notation, one of the equations obtained from the Cartan geometry reduces to the Newton inverse square law. It is shown that the latter is always valid in the off resonance condition, but at resonance, the force due to gravity is greatly amplified even in the Newtonian limit. This is a direct consequence of Cartan geometry. The latter reduces to Riemann geometry when the Cartan torsion vanishes and when the spin connection becomes equivalent to the Christoffel connection. PACS numbers: 95.30.Sf, 03.50.–z, 04.50.+h 1. Introduction It is well known that the gravitational general relativity is based on Rie- mann geometry with a Christoffel connection. This type of geometry is a special case of Cartan geometry [1] when the torsion form is zero. There- fore gravitation general relativity can be expressed in terms of this limit of Cartan geometry. In this paper this procedure is shown to produce a sec- ond order differential equation with resonant solutions [2–20]. Off resonance the mathematical form of the Newton inverse square law is obtained from a well defined approximation to the complete theory, but the relation between the gravitational potential field and the gravitational force field is shown to contain the spin connection in general. -
Entanglement on Spin Networks Loop Quantum
ENTANGLEMENT ON SPIN NETWORKS IN LOOP QUANTUM GRAVITY Clement Delcamp London - September 2014 Imperial College London Blackett Laboratory Department of Theoretical Physics Submitted in partial fulfillment of the requirements for the degree of Master of Science of Imperial College London I would like to thank Pr. Joao Magueijo for his supervision and advice throughout the writ- ing of this dissertation. Besides, I am grateful to him for allowing me to choose the subject I was interested in. My thanks also go to Etera Livine for the initial idea and for introducing me with Loop Quantum Gravity. I am also thankful to William Donnelly for answering the questions I had about his article on the entanglement entropy on spin networks. Contents Introduction 7 1 Review of Loop Quantum Gravity 11 1.1 Elements of general relativity . 12 1.1.1 Hamiltonian formalism . 12 1.1.2 3+1 decomposition . 12 1.1.3 ADM variables . 13 1.1.4 Connection formalism . 14 1.2 Quantization of the theory . 17 1.2.1 Outlook of the construction of the Hilbert space . 17 1.2.2 Holonomies . 17 1.2.3 Structure of the kinematical Hilbert space . 19 1.2.4 Inner product . 20 1.2.5 Construction of the basis . 21 1.2.6 Aside on the meaning of diffeomorphism invariance . 25 1.2.7 Operators on spin networks . 25 1.2.8 Area operator . 27 1.2.9 Physical interpretation of spin networks . 28 1.2.10 Chunks of space as polyhedra . 30 1.3 Explicit calculations on spin networks . 32 2 Entanglement on spin networks 37 2.1 Outlook . -
GEOMETRIC INTERPRETATIONS of CURVATURE Contents 1. Notation and Summation Conventions 1 2. Affine Connections 1 3. Parallel Tran
GEOMETRIC INTERPRETATIONS OF CURVATURE ZHENGQU WAN Abstract. This is an expository paper on geometric meaning of various kinds of curvature on a Riemann manifold. Contents 1. Notation and Summation Conventions 1 2. Affine Connections 1 3. Parallel Transport 3 4. Geodesics and the Exponential Map 4 5. Riemannian Curvature Tensor 5 6. Taylor Expansion of the Metric in Normal Coordinates and the Geometric Interpretation of Ricci and Scalar Curvature 9 Acknowledgments 13 References 13 1. Notation and Summation Conventions We assume knowledge of the basic theory of smooth manifolds, vector fields and tensors. We will assume all manifolds are smooth, i.e. C1, second countable and Hausdorff. All functions, curves and vector fields will also be smooth unless otherwise stated. Einstein summation convention will be adopted in this paper. In some cases, the index types on either side of an equation will not match and @ so a summation will be needed. The tangent vector field @xi induced by local i coordinates (x ) will be denoted as @i. 2. Affine Connections Riemann curvature is a measure of the noncommutativity of parallel transporta- tion of tangent vectors. To define parallel transport, we need the notion of affine connections. Definition 2.1. Let M be an n-dimensional manifold. An affine connection, or connection, is a map r : X(M) × X(M) ! X(M), where X(M) denotes the space of smooth vector fields, such that for vector fields V1;V2; V; W1;W2 2 X(M) and function f : M! R, (1) r(fV1 + V2;W ) = fr(V1;W ) + r(V2;W ), (2) r(V; aW1 + W2) = ar(V; W1) + r(V; W2), for all a 2 R. -
Supergravities
Chapter 10 Supergravities. When we constructed the spectrum of the closed spinning string, we found in the 3 1 massless sector states with spin 2 , in addition to states with spin 2 and other states i ~j NS ⊗ NS : b 1 j0; piL ⊗ b 1 j0; piR with i; j = 1; 8 yields gij(x) with spin 2 − 2 − 2 (10.1) i 3 NS ⊗ R : b− 1 j0; piL ⊗ j0; p; αiR with i; α = 1; 8 yields χi,α(x) with spin 2 2 The massless states with spin 2 correspond to a gauge field theory: Einstein's theory 3 of General Relativity, but in 9 + 1 dimensions. The massless states with spin 2 are part of another gauge theory, an extension of Einstein gravity, called supergravity. That theory was first discovered in 1976 in d = 3 + 1 dimensions, but supergravity theories also exist in higher dimensions, through (up to and including) eleven dimensions. In this chapter we discuss supergravity theories. They are important in string theory because they are the low-energy limit of string theories. We do not assume that the reader has any familiarity with supergravity. We begin with the N = 1 theory in 3 + 1 dimensions, m also called simple supergravity, which has one gravitational vielbein field eµ , and one m α fermionic partner of eµ , called the gravitino field µ with spinor index α = 1; ··· ; 4 A ¯ _ (or two 2-component gravitinos µ and µ,A_ with A; A = 1; 2) and µ = 0; 1; 2; 3. This theory has one real local supersymmetry with a real (Majorana) 4-component spinorial α A ∗ _ parameter (or two 2-component parameters and ¯A_ = (A) with A; A = 1; 2).