- •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
3.7 The Levi Civita Connection |
141 |
The tri-index symbols Γμνρ encode, patch by patch, the considered affine connection. According to Definition 3.7.1 these connection coefficients are equivalently defined by setting
eμ eν ≡ eν (eμ) = Γμν ρ eρ |
(3.7.5) |
3.7.2 Curvature and Torsion of an Affine Connection
To every connection one-form A on a principal bundle P (M , G), we can associate a curvature 2-form:
F ≡ dA + A A |
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A K TI |
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which is G Lie algebra valued and whose fundamental properties and profound physical meaning will be analyzed in Chap. 5 of this volume. Here we just note that,
π
evaluated on any associated vector bundle E = M , the connection A becomes a matrix and the same is true of the curvature F . In that case the first line of (3.7.6) is to be understood in the sense both of matrix multiplication and of wedge product, namely the element (i, j ) of A A is calculated as Ai k Ak j , with summation over the dummy index k.
We can apply the general formula (3.7.6) to the case of an affine connection. In that case the curvature 2-form is traditionally denoted with the letter R in honor of
Riemann. We obtain: |
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R ≡ dΓ + Γ Γ |
(3.7.7) |
which, using the basis {eμ} for the tangent bundle and its dual {ων } for the cotangent bundle, becomes:
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Rμν = dΓμ ν + Γμ ρ Γρ ν |
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the four index symbols R |
ν being, by definition, twice the components of the 2- |
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form along the μ |
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we denote by x , we can choose the |
holonomic basis of sections e |
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whose dual is provided by the differentials ω |
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Rλσ μν = ∂λΓσ μ ν − ∂σ Γλμ ν + Γλμ |
ρ Γσρ ν − Γσ μ ρ Γλρ ν |
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(3.7.9) |
Comparing (3.7.9) with the Riemann-Christoffel symbols of (3.2.10), we see that the latter could be identified with the components of the curvature two-form of an affine connection Γ if the Christoffel symbols introduced in (3.2.7) were the coefficients
142 |
3 Connections and Metrics |
of such a connection. Which connection is the one described by the Christoffel symbols and how is it defined? The answer is: the Levi Civita connection. Its definition follows in the next paragraph.
Torsion and Torsionless Connections The notion of torsion was briefly anticipated in our historical outline. It applies only to affine connections and distinguishes them from general connections on generic fibre bundles. Intuitively torsion has to do with the fact that when we parallel transport vectors along a loop the transported vector can differ from the original one not only through a rotation but also through a displacement. While the infinitesimal rotation angle is related to the curvature tensor, the infinitesimal displacement is related to the torsion tensor. This was explicitly displayed in (3.2.12). Rigorously we have the following:
Definition 3.7.2 Let M be an m-dimensional manifold and denote an affine connection on its tangent bundle. The torsion T is a map:
T : X(M ) × X(M ) → X(M )
defined as follows:
X, Y X(M ) : T (X, Y) = −T (Y, X) ≡ XY − YX − [X, Y] X(M )
Given a basis of sections of the tangent bundle {−→ } we can calculate their com- e μ
mutators:
[eμ, eν ] = Kμν ρ (p)eρ |
(3.7.10) |
where the point dependent coefficients Kμν ρ (p) are named the contorsion coefficients. They do not form a tensor, since they depend on the choice of basis. For instance in the holonomic basis eμ = ∂μ the contorsion coefficients are zero, while they do not vanish in other bases. Notwithstanding their non-tensorial character they can be calculated in any basis and once this is done we obtain a true tensor, namely the torsion from Definition 3.7.2. Explicitly we have:
T (eμ, eν ) = Tμνρ eρ
(3.7.11)
Tμνρ = Γμν ρ − Γνμ ρ − Kμν ρ
Definition 3.7.3 An affine connection is named torsionless if its torsion tensor vanishes identically, namely if T (X, Y) = 0, X, Y X(M )
It follows from (3.7.12) that the coefficients of a torsionless affine connection are symmetric in the lower indices in the holonomic basis. Indeed if the contorsion vanishes, imposing zero torsion reduces to the condition:
Γμν ρ = Γνμ ρ |
(3.7.12) |
3.7 The Levi Civita Connection |
143 |
The Levi Civita Metric Connection Consider now the case where the manifold M is endowed with a metric g. Independently from the signature of the latter (Riemannian or pseudo-Riemannian) we can define a unique affine connection which preserves the scalar products defined by g and is torsionless. That affine connection is the Levi Civita connection. Explicitly we have the following
Definition 3.7.4 Let (M , g) be a (pseudo-)Riemannian manifold. The associated Levi Civita connection g is that unique affine connection which satisfies the following two conditions:
(i)g is torsionless, namely T g (, ) = 0,
(ii)The metric is covariantly constant under the transport defined by g , that is:
Z, X, Y X(M ) : Zg(X, Y) = g( Zg X, Y) + g(X, Zg Y).
The idea behind such a definition is very simple and intuitive. Consider two vector fields X, Y. We can measure their scalar product and hence the angle they form by evaluating g(X, Y). Consider now a third vector field Z and let us parallel transport the previously given vectors in the direction defined by Z. For an infinitesimal displacement we have X → X + ZX and Y → Y + ZY. We can compare the scalar product of the parallel transported vectors with that of the original ones. Imposing the second condition listed in Definition 3.7.4 corresponds to stating that the scalar product of the parallel transported vectors should just be the increment along Z of the scalar product of the original ones. This is the very intuitive notion of parallelism.
It is now very easy to verify that the Christoffel symbols, defined in (3.2.7) are just the coefficients of the Levi Civita connection in the holonomic basis eμ = ∂μ ≡ ∂/∂xμ. As we already remarked, in this case the contorsion vanishes and a torsionsless connection has symmetric coefficients according to (3.7.12). On the other hand the second condition of Definition 3.7.4 translates into:
∂λgμν = Γλμ σ gσ ν + Γλν σ gμσ |
(3.7.13) |
which admits the Christoffel symbols (3.2.7) as unique solution. There is a standard trick to see this and solve (3.7.13) for Γ . Just write three copies of the same equation with cyclically permuted indices:
∂λgμν = Γλμ |
σ gσ ν + Γλν |
σ gμσ |
(3.7.14) |
∂μgνλ = Γμν |
σ gσ λ + Γμλ |
σ gνσ |
(3.7.15) |
∂ν gλμ = Γνλ |
σ gσ μ + Γνμ |
σ gλσ |
(3.7.16) |
Next sum (3.7.14) with (3.7.15) and subtract (3.7.16). In the result of this linear combination use the symmetry of Γλμ σ in its lower indices. With this procedure
you will obtain that Γλμ σ is equal to the Christoffel symbols.