- •Preface
- •Acknowledgements
- •Contents
- •1.1 Introduction
- •1.2 Classical Physics Between the End of the XIX and the Dawn of the XX Century
- •1.2.1 Maxwell Equations
- •1.2.2 Luminiferous Aether and the Michelson Morley Experiment
- •1.2.3 Maxwell Equations and Lorentz Transformations
- •1.3 The Principle of Special Relativity
- •1.3.1 Minkowski Space
- •1.4 Mathematical Definition of the Lorentz Group
- •1.4.1 The Lorentz Lie Algebra and Its Generators
- •1.4.2 Retrieving Special Lorentz Transformations
- •1.5 Representations of the Lorentz Group
- •1.5.1 The Fundamental Spinor Representation
- •1.6 Lorentz Covariant Field Theories and the Little Group
- •1.8 Criticism of Special Relativity: Opening the Road to General Relativity
- •References
- •2.1 Introduction
- •2.2 Differentiable Manifolds
- •2.2.1 Homeomorphisms and the Definition of Manifolds
- •2.2.2 Functions on Manifolds
- •2.2.3 Germs of Smooth Functions
- •2.3 Tangent and Cotangent Spaces
- •2.4 Fibre Bundles
- •2.5 Tangent and Cotangent Bundles
- •2.5.1 Sections of a Bundle
- •2.5.2 The Lie Algebra of Vector Fields
- •2.5.3 The Cotangent Bundle and Differential Forms
- •2.5.4 Differential k-Forms
- •2.5.4.1 Exterior Forms
- •2.5.4.2 Exterior Differential Forms
- •2.6 Homotopy, Homology and Cohomology
- •2.6.1 Homotopy
- •2.6.2 Homology
- •2.6.3 Homology and Cohomology Groups: General Construction
- •2.6.4 Relation Between Homotopy and Homology
- •References
- •3.1 Introduction
- •3.2 A Historical Outline
- •3.2.1 Gauss Introduces Intrinsic Geometry and Curvilinear Coordinates
- •3.2.3 Parallel Transport and Connections
- •3.2.4 The Metric Connection and Tensor Calculus from Christoffel to Einstein, via Ricci and Levi Civita
- •3.2.5 Mobiles Frames from Frenet and Serret to Cartan
- •3.3 Connections on Principal Bundles: The Mathematical Definition
- •3.3.1 Mathematical Preliminaries on Lie Groups
- •3.3.1.1 Left-/Right-Invariant Vector Fields
- •3.3.1.2 Maurer-Cartan Forms on Lie Group Manifolds
- •3.3.1.3 Maurer Cartan Equations
- •3.3.2 Ehresmann Connections on a Principle Fibre Bundle
- •3.3.2.1 The Connection One-Form
- •Gauge Transformations
- •Horizontal Vector Fields and Covariant Derivatives
- •3.4 Connections on a Vector Bundle
- •3.5 An Illustrative Example of Fibre-Bundle and Connection
- •3.5.1 The Magnetic Monopole and the Hopf Fibration of S3
- •The U(1)-Connection of the Dirac Magnetic Monopole
- •3.6.1 Signatures
- •3.7 The Levi Civita Connection
- •3.7.1 Affine Connections
- •3.7.2 Curvature and Torsion of an Affine Connection
- •Torsion and Torsionless Connections
- •The Levi Civita Metric Connection
- •3.8 Geodesics
- •3.9 Geodesics in Lorentzian and Riemannian Manifolds: Two Simple Examples
- •3.9.1 The Lorentzian Example of dS2
- •3.9.1.1 Null Geodesics
- •3.9.1.2 Time-Like Geodesics
- •3.9.1.3 Space-Like Geodesics
- •References
- •4.1 Introduction
- •4.2 Keplerian Motions in Newtonian Mechanics
- •4.3 The Orbit Equations of a Massive Particle in Schwarzschild Geometry
- •4.3.1 Extrema of the Effective Potential and Circular Orbits
- •Minimum and Maximum
- •Energy of a Particle in a Circular Orbit
- •4.4 The Periastron Advance of Planets or Stars
- •4.4.1 Perturbative Treatment of the Periastron Advance
- •References
- •5.1 Introduction
- •5.2 Locally Inertial Frames and the Vielbein Formalism
- •5.2.1 The Vielbein
- •5.2.2 The Spin-Connection
- •5.2.3 The Poincaré Bundle
- •5.3 The Structure of Classical Electrodynamics and Yang-Mills Theories
- •5.3.1 Hodge Duality
- •5.3.2 Geometrical Rewriting of the Gauge Action
- •5.3.3 Yang-Mills Theory in Vielbein Formalism
- •5.4 Soldering of the Lorentz Bundle to the Tangent Bundle
- •5.4.1 Gravitational Coupling of Spinorial Fields
- •5.5 Einstein Field Equations
- •5.6 The Action of Gravity
- •5.6.1 Torsion Equation
- •5.6.1.1 Torsionful Connections
- •The Torsion of Dirac Fields
- •Dilaton Torsion
- •5.6.2 The Einstein Equation
- •5.6.4 Examples of Stress-Energy-Tensors
- •The Stress-Energy Tensor of the Yang-Mills Field
- •The Stress-Energy Tensor of a Scalar Field
- •5.7 Weak Field Limit of Einstein Equations
- •5.7.1 Gauge Fixing
- •5.7.2 The Spin of the Graviton
- •5.8 The Bottom-Up Approach, or Gravity à la Feynmann
- •5.9 Retrieving the Schwarzschild Metric from Einstein Equations
- •References
- •6.1 Introduction and Historical Outline
- •6.2 The Stress Energy Tensor of a Perfect Fluid
- •6.3 Interior Solutions and the Stellar Equilibrium Equation
- •6.3.1 Integration of the Pressure Equation in the Case of Uniform Density
- •6.3.1.1 Solution in the Newtonian Case
- •6.3.1.2 Integration of the Relativistic Pressure Equation
- •6.3.2 The Central Pressure of a Relativistic Star
- •6.4 The Chandrasekhar Mass-Limit
- •6.4.1.1 Idealized Models of White Dwarfs and Neutron Stars
- •White Dwarfs
- •Neutron Stars
- •6.4.2 The Equilibrium Equation
- •6.4.3 Polytropes and the Chandrasekhar Mass
- •6.5 Conclusive Remarks on Stellar Equilibrium
- •References
- •7.1 Introduction
- •7.1.1 The Idea of GW Detectors
- •7.1.2 The Arecibo Radio Telescope
- •7.1.2.1 Discovery of the Crab Pulsar
- •7.1.2.2 The 1974 Discovery of the Binary System PSR1913+16
- •7.1.3 The Coalescence of Binaries and the Interferometer Detectors
- •7.2 Green Functions
- •7.2.1 The Laplace Operator and Potential Theory
- •7.2.2 The Relativistic Propagators
- •7.2.2.1 The Retarded Potential
- •7.3 Emission of Gravitational Waves
- •7.3.1 The Stress Energy 3-Form of the Gravitational Field
- •7.3.2 Energy and Momentum of a Plane Gravitational Wave
- •7.3.2.1 Calculation of the Spin Connection
- •7.3.3 Multipolar Expansion of the Perturbation
- •7.3.3.1 Multipolar Expansion
- •7.3.4 Energy Loss by Quadrupole Radiation
- •7.3.4.1 Integration on Solid Angles
- •7.4 Quadruple Radiation from the Binary Pulsar System
- •7.4.1 Keplerian Parameters of a Binary Star System
- •7.4.2 Shrinking of the Orbit and Gravitational Waves
- •7.4.2.1 Calculation of the Moment of Inertia Tensor
- •7.4.3 The Fate of the Binary System
- •7.4.4 The Double Pulsar
- •7.5 Conclusive Remarks on Gravitational Waves
- •References
- •Appendix A: Spinors and Gamma Matrix Algebra
- •A.2 The Clifford Algebra
- •A.2.1 Even Dimensions
- •A.2.2 Odd Dimensions
- •A.3 The Charge Conjugation Matrix
- •A.4 Majorana, Weyl and Majorana-Weyl Spinors
- •Appendix B: Mathematica Packages
- •B.1 Periastropack
- •Programme
- •Main Programme Periastro
- •Subroutine Perihelkep
- •Subroutine Perihelgr
- •Examples
- •B.2 Metrigravpack
- •Metric Gravity
- •Routines: Metrigrav
- •Mainmetric
- •Metricresume
- •Routine Metrigrav
- •Calculation of the Ricci Tensor of the Reissner Nordstrom Metric Using Metrigrav
- •Index
3.3 Connections on Principal Bundles: The Mathematical Definition |
121 |
X VuP π X = 0 |
(3.3.75) |
where π is the push-forward of the projection map.
Having defined the vertical subspace of the tangent space one would be interested in giving a definition also of the horizontal subspace HuP , which, intuitively, must be somehow parallel to the tangent space Tp M to the base manifold at the projection point p = π(u). The dimension of the vertical space is the same as the dimension of the fibre, namely n = dim G. The dimension of the horizontal space HuP must be the same as the dimension of the base manifold m = dim M . Indeed HuP should be the orthogonal complement of VuP . Easy to say, but orthogonal with respect to what? This is precisely the point. Is there an a priori intrinsically defined way of defining the orthogonal complement to the vertical subspace Vu TuP ? The answer is that there is not. Given a basis {vμ} of n vectors for the subspace VuP , there are infinitely many ways of finding m extra vectors {hi } which complete this basis to a basis of TuP . The span of any such collection of m vectors {hi } is a possible legitimate definition of the orthogonal complement HuP . This arbitrariness is the root of the mathematical notion of a connection. Providing a fibre bundle with a connection precisely means introducing a rule that uniquely defines the orthogonal complement HuP .
Definition 3.3.5 Let P (M, G) rule which at any point u P into the vertical subspace VuP the following properties:
be a principal fibre-bundle. A connection on P is a defines a unique splitting of the tangent space TuP and into a horizontal complement HuP satisfying
(i)TuP = HuP VuP .
(ii)Any smooth vector field X Γ (T P , P ) separates into the sum of two smooth
vector fields X = XH + XV such that at any point u P we have XHu HuP and XVu VuP .
(iii)g G we have that HguP = Lg HuP .
The third defining property of the connection states that all the horizontal spaces along the same fibre are related to each other by the push-forward of the lefttranslation on the group manifold.
This beautiful purely geometrical definition of the connection due to Ehresmann emphasizes that it is just an intrinsic attribute of the principle fibre-bundle. In a trivial bundle, which is a direct product of manifolds, the splitting between vertical and horizontal spaces is done once for ever. Vertical space is the tangent space to the fibre, horizontal space is the tangent space to the base. In a non-trivial bundle the splitting between vertical and horizontal directions has to be reconsidered at every next point and fixing this ambiguity is the task of the connection.
3.3.2.1 The Connection One-Form
The algorithmic way to implement the splitting rule advocated by Definition 3.3.5 is provided by introducing a connection one-form A which is just a Lie algebra valued one-form on the bundle P satisfying two precise requirements.
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3 Connections and Metrics |
Definition 3.3.6 Let P (M , G) be a principle fibre-bundle with structural Lie group G, whose Lie algebra we denote by G. A connection one-form on this bundle is a Lie algebra valued section of the cotangent bundle A G Γ (T P , P ) which satisfies the following defining properties:
(i)X G : A X# = X.
(ii)g G : LgA = Adjg−1 A ≡ g−1Ag.
Given the connection one-form A the splitting between vertical and horizontal subspaces is performed through the following
Definition 3.3.7 At any u P , the horizontal subspace HuP of the tangent space to the bundle is provided by the kernel of A:
HuP ≡ ,X TuP | A(X) = 0- |
(3.3.76) |
The actual meaning of Definitions 3.3.6, 3.3.7 and their coherence with Definition 3.3.5 becomes clear if we consider a local trivialization of the bundle.
Just as before, let xμ be the coordinates on the base-manifold and αi the group parameters. With respect to this local patch, the connection one-form A has the following appearance:
A = A2+ |
μ |
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I |
(3.3.77) |
A |
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Aμ TI |
(3.3.78) |
A = Ai dαi = dαi AiI TI |
(3.3.79) |
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where, a priori, both the components A2μ(x, α) and Ai (x, α) could depend on both xμ and αi . The second equality in (3.3.79) and (3.3.78) is due to the fact that A and A are Lie algebra valued, hence they can be expanded along a basis of generators of G. Actually the dependence on the group parameters or better on the group element g(α) is completely fixed by the defining axioms. Let us consider
first the implications of property (i) in Definition 3.3.6. To thisAeffect let X G be |
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expanded along the same basis of generators, namely X = X TA. As |
we already |
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remarked in (3.3.74), the image of X through the map # is X# = XATA |
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3.3 Connections on Principal Bundles: The Mathematical Definition |
123 |
(r)
Therefore AIi =ΣiA(α) and the vertical component of the one-form connection is nothing else but the right-invariant one-form:
A = σ(R) ≡ dg g−1 |
(3.3.82) |
Consider now the implications of defining property (ii). In the chosen local trivialization the left action of any element γ of the structural group G is Lγ : (x, g(α)) → (x, γ · g(α)) and its pull-back acts on the right-invariant one-form σ(R) by adjoint transformations:
Lγ : σ(R) → d(γ · g)(γ · g)−1 = γ · σ(R) · γ −1 |
(3.3.83) |
Property (ii) of Definition 3.3.6 requires that the same should be true for the complete connection one-form A. This fixes the g dependence of A2, namely we must have:
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(3.3.84) |
A (x, g) |
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is a G Lie algebra valued one-form on the base manifold M . Consequently we can summarize the content of Definition 3.3.6 by stating that in any local trivialization u = (x, g) the connection one-form has the following structure:
A = g · A · g−1 + dg · g−1 |
(3.3.86) |
Gauge Transformations From (3.3.86) we easily work out the action on the oneform connection of the transition function from one local trivialization to another one. Let us recall (2.4.8) and (2.4.9). In the case of a principal bundle the transition function tαβ (x) is just a map from the intersection of two open neighborhoods of the base space into the structural group:
tαβ : M Uα # Uβ → G |
(3.3.87) |
and we have: |
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transition : (x, gα ) → (x, gβ ) = x, gα · tαβ (x) |
(3.3.88) |
Correspondingly, combining this information with (3.3.86) we conclude that:
Aα → Aβ
Aα = g · Aα · g−1 + dg · g−1
(3.3.89)
Aβ = g · Aβ · g−1 + dg · g−1
Aβ = tαβ (x) · Aα · t−αβ1(x) + dtαβ (x) · t−αβ1(x)
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The last equation of (3.3.89) is the most significant one for the bridge from Mathematics to Physics and provides the common stem of Yang’s picture in Fig. 3.1. The one-form A defined over the base-manifold M , which in particular can be space-time, is what physicists name a gauge potential, the prototype of which is the gauge-potential of electrodynamics; the transformation from one local trivialization to another one, encoded in the last of (3.3.89), is what physicists name a gauge transformation. The basic idea about gauge-transformations is that of local symmetry. Some physical system or rather some physical law is invariant with respect to the transformations of a group G but not only globally, rather also locally, namely the transformation can be chosen differently from one point of space-time to the next one. The basic mathematical structure realizing this physical idea is that of fibre-bundle and the one-form connection on a fibre-bundle is the appropriate mathematical structure which encompasses all mediators of all physical interactions.
Horizontal Vector Fields and Covariant Derivatives Let us come back to Definition 3.3.7 of horizontal vector fields. In a local trivialization a generic vector field on P is of the form:
X = Xμ∂μ + Xi ∂i |
(3.3.90) |
where we have used the short-writing ∂μ = ∂/∂xμ and ∂i = ∂/∂αi . The horizontality condition in (3.3.76) becomes:
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XμA Ag |
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A · |
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(3.3.91) |
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Multiplying on the left by g−1 and on the right by g, (3.3.91) can be easily solved for Xi obtaining in this way the general form of a horizontal vector field on a principal fibre-bundle P (M , G) endowed with a connection one-form A ↔ A . We get:
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TA |
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A |
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∂ |
(3.3.92) |
To obtain the above result we made use of the following identities:
g− |
1 |
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i g = |
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A |
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−→i ; |
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δA |
(3.3.93) |
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which follow from the definitions of left-invariant one-forms and vector fields discussed in previous subsections.
Equation (3.3.92) is equally relevant for the bridge between Mathematics and Physics as (3.3.89). Indeed from (3.3.92) we realize that the mathematical notion of horizontal vector fields coincides with the physical notion of covariant derivative. Expressions like that in the bracket of (3.3.92), firstly appeared in the early decades of the XXth century when Classical Electrodynamics was rewritten in the language of Special Relativity and the quadri-potential Aμ was introduced. Indeed with the development first of Dirac equation and then of Quantum Electrodynamics, the covariant derivative of the electron wave-function made its entrance in the language of theoretical physics:
3.3 Connections on Principal Bundles: The Mathematical Definition |
125 |
μψ = (∂μ − iAμ)ψ |
(3.3.94) |
The operator μ might be assimilated with the action of a horizontal vector field (3.3.92) if we just had a one dimensional structural group U(1) with a single generator and if we were acting on functions over P (M , U(1)) that are eigenstates of the unique left-invariant vector field T(L) with eigenvalue i. This is indeed the case
of Electrodynamics. The group U(1) is composed by all unimodular complex num-
−→
bers exp[iα] and the left-invariant vector field is simply T(L) = ∂ /∂α. The wavefunction ψ(x) is actually a section of the principle bundle P (M4, U(1)) since it is a
complex spinor whose overall phase factor exp[iα(x)] takes values in the U(1)-fibre over x M4. Since T(L) exp[iα] = i exp[iα], the covariant derivative (3.3.94) is of
the form (3.3.92).
This shows that the one-form connection coincides, at least in the case of electrodynamics, with the physical notion of gauge-potential which, upon quantization, describes the photon-field, namely the mediator of electromagnetic interactions. The 1954 invention of non-Abelian gauge-theories by Yang and Mills started from the generalization of the covariant derivative (3.3.94) to the case of the su(2) Lie algebra. Introducing three gauge potentials AμA, corresponding to the three standard generators JA of su(2):
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(A, B, C = 1, 2, 3) |
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where σ A denote the 2 × 2 Pauli matrices: |
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they wrote: |
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From the su(2) × u(1) standard model of electro-weak interactions of Glashow, Salam and Weinberg (see Fig. 3.14) we know nowadays that, in appropriate combinations with Aμ, the three gauge fields AμA, describe the W ± and Z0 particles discovered at CERN in 1983 by the UA1 experiment of Carlo Rubbia. They have spin one and mediate the weak interactions.
The mentioned examples show that the Lie algebra-valued connection one-form defined by Ehresmann on principle bundles is clearly related to the gauge-fields of particle physics since it enters the construction of covariant derivatives via the notion of horizontal vector fields. On the other hand the same one-form must be related to gravitation as well, since also there one deals with covariant derivatives (3.2.8) sustained by the Levi Civita connection and the Christoffel symbols (3.2.7). The key to understand the unifying point of view offered by the notion of Ehresmann connection on a principle bundle is obtained by recalling what we just emphasized in Chap. 2 when we introduced the very notion of fibre-bundles. Following Definition 2.4.5 let us recall that to each principle bundle P (M , G) one can associate as many associated vector bundles as there are linear representations of the structural
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Fig. 3.14 Sheldon Glashow, Steven Weinberg and Abdus Salam shared the 1979 Nobel Prize in Physics for their 1968 formulation of a gauge theory of the electro-weak interactions based on the choice of a gauge group G = SU(2) × U(1). In the language of Mathematics this is the structural group of a principle-bundle, whose one-form connection contains four fields. These fields correspond to as many elementary particles: the W + , W − , the photon γ and another neutral massive particle Z0. While the existence of the W ± particles could be indirectly inferred from the known weak decays, the Z0 particle had no experimental motivation at the time when the SU(2) × U(1) was formulated. Yet in 1973 the neutral current interactions were discovered at CERN. Their effect was revealed by otherwise unexplicable electron tracks photographed at the Gargamelle Bubble Chamber. The direct production of the W ± and Z0 particles had to wait the construction of the Super Proton Synchrotron and the UA1 experiment of 1983 which revealed them. In 1984 Carlo Rubbia and the accelerator engineer Simon van der Meer, who invented the adiabatic cooling system at the basis of the experimental success, obtained the Nobel Prize in Physics for the experimental verification of the gauge theory description of electro-weak interactions
group G, namely infinitely many. It suffices to use as transition functions the corresponding linear representations of the transition functions of the principle bundle as displayed in (2.4.20). In all such associated bundles the fibres are vector spaces of dimension r (the rank of the bundle) and the transition functions are r × r matrices. Every linear representation of a Lie group G of dimension r induces a linear representation of its Lie algebra G, where the left- (right-)invariant vector fields T(L/R)A are mapped into r × r matrices:
TA(L/R) → D(TA) |
(3.3.98) |
satisfying the same commutation relations: |
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D(TA), D(TB ) = CAB C D(TC ) |
(3.3.99) |
It is therefore tempting to assume that given a one-form connection A ↔ A on a principle-bundle one can define a one-form connection on every associated vector bundle by taking its r × r matrix representation D(A) ↔ D(A ). In which sense this matrix-valued one-form defines a connection on the considered vector bundle? To answer such a question we obviously need first to define connections on generic vector bundles, which is what we do in the next section.
