- •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
5.3 The Structure of Classical Electrodynamics and Yang-Mills Theories |
195 |
having collectively denoted TI = {Pa , Jbc}. Next we can collect the vielbein Ea and the spin-connection ωab into a single object, namely into a principle connection on the Poincaré bundle:
Ω = ΩI TI ≡ Ea Pa + ωabJab |
(5.2.25) |
and following the general prescription displayed in (3.7.6) we can construct the curvature two-form of such a Poincaré connection:
Θ ≡ dΩ + Ω Ω |
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Expanding Θ along the generators we discover that the Torsion Ta and the curvature Rab are just the components of the overall Poincaré curvature Θ along the translation and rotation generators respectively.
Thus it appears that the main ingredients apt to describe the gravitational field, once Cartan’s viewpoint is adopted, are encoded into a principal connection, one on the Poincaré bundle with structural group ISO(1, m − 1).2 Such an observation is very tempting since it seems to imply that, at the end of the day, gravitation is explained in terms of a gauge theory just as all the other fundamental interactions of Nature. Up to this point the similarities are several and it is worth summarizing them for comparison. For this reason we open a digression on classical Electrodynamics and classical Yang-Mills theories. We will see that notwithstanding the many striking analogies, gravity involves an extra geometric structure, the soldering, which differentiates the gauge theory of gravitational interactions from all the others and makes it unique and special.
5.3The Structure of Classical Electrodynamics and Yang-Mills Theories
Let us begin by reviewing Classical Electrodynamics in the most frequently utilized approach.
There are some matter fields, typically the spinor field ψα (x), describing the electron/positron, or some other electrically charged fermionic particles3 and one considers the standard action for such fields, the free Dirac action:4
ADirac |
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2From now one we choose p = 1 which is the physically most interesting case.
3All leptons and quarks fall into this category.
4For the conventions on spinors and gamma-matrix algebra see Appendix A.
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5 Einstein Versus Yang-Mills Field Equations |
The electrically charged matter fields can also be spin zero fields, namely complex scalars φ(x), in which case the standard free action is the Klein-Gordon one:
AKG |
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The matter action, namely ADirac and /or AKG has a global symmetry under the transformations of a U(1) Lie group defined as follows:
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where e, q are the electric charges of the considered fields. Indeed as long as the angle θ is constant and independent from the space-time location, performing the replacements (5.3.3) leaves the actions (5.3.1) and (5.3.2) invariant.
The basic idea of Electrodynamics is to transform this symmetry from a global into a local one, namely to allow for a space-time dependence of the gauge angle θ → θ (x). The appropriate mathematical apparatus for this operation was developed in Chap. 3.
We consider the classical matter fields ψ(x) or φ(x) as sections of a rank one
π
holomorphic vector bundle E = M that has the space-time manifold M as base manifold, U(1) as structural group and C as standard fibre. This vector bundle is associated to a principle bundle P (M , U(1)). Next we introduce a principle connection on this latter bundle, namely a U(1) Lie algebra valued one-form on the total space P , with the structure dictated by (3.3.86):
A = i Aμ dxμ + dθ |
(5.3.4) |
In the case of U(1) the Lie algebra is made by just one generator that can be identified with the imaginary unity i. According to the discussion of Sect. 3.3.2.1, the existence of the connection allows to define the covariant derivatives:
μψ ≡ (∂μ − ieAμ)ψ |
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Global symmetry is promoted to a local one, if ordinary derivatives are replaced by covariant ones in the actions (5.3.1), (5.3.2) which become:
ADirac = |
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Indeed the transformations (5.3.3) with an x-dependent gauge angle θ (x) are interpreted as the transition functions from a local trivialization of the U(1) bundle
5.3 The Structure of Classical Electrodynamics and Yang-Mills Theories |
197 |
Fig. 5.2 The interaction vertex of electrodynamics
to another one and under such changes of local trivializations the connection oneform changes according the general rule (3.3.89). In the case of electrodynamics this reduces to:
Aμ → Aμ + ∂μθ |
(5.3.9) |
The new Lagrangians (5.3.7), (5.3.8) contain now interaction vertices of the original fields ψ or φ with the gauge field Aμ. For example, in the case of spinor electrodynamics, the interaction vertex is depicted in Fig. 5.2. Hence the gauge field Aμ should be equipped with a kinetic Lagrangian which defines its propagator. The answer is known since the time when Maxwell equations were rewritten in compact relativistic notation. The curvature two-form of the electromagnetic U(1)- connection is:
F = dA = 1 Fμν dxμ dxν
2
(5.3.10)
Fμν = ∂μAν − ∂ν Aμ
and its components Fμν encode the electric and magnetic fields according to the following identifications:
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Classical Maxwell equations are reproduced by the following differential statements on the field strength:
∂[λFμν] = 0 |
(5.3.12) |
∂μFμν = eJν |
(5.3.13) |
where Jν = ψγ μψ is the electric current. There is a fundamental difference between the first equation (5.3.12) and the second (5.3.13). Equation (5.3.12) is just an identity, the Bianchi identity for the curvature of a U(1)-connection:
dF = d dA = 0 |
(5.3.14) |
while (5.3.13) is a true dynamical equation which follows upon variation in δAν of the following action:
Atot = Agauge + Amatter |
(5.3.15) |
198 |
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5 Einstein Versus Yang-Mills Field Equations |
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(5.3.17) |
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One important observation is that Maxwell equations are consistent with the conservation of the electric charge since the left hand side of the second equation satisfies the identity:
∂ν ∂μFμν = 0 ∂ν Jν = 0 |
(5.3.18) |
which implies the vanishing of the electric current divergence and hence the global conservation of the electric charge. One might wonder whether the actual structure of Maxwell equations is an accident or whether it is uniquely determined by first principles. The correct answer is the second. Indeed we can easily show that, as long as Aμ is interpreted as a connection on a principle U(1)-bundle, namely, as long as the transformation (5.3.9) is required to be a symmetry of the field equations, and as long as the latter are assumed to be Lorentz invariant, linear differential equations of the second order, there is no alternative. Indeed let us see what is the most general form of such equations for the field Aν . Considering all possible index contractions we arrive at the following candidate equation:
Aν + α∂ν ∂μAμ + mAν = eJν |
(5.3.19) |
where α, m are coefficients to be determined. If we require that this equation should be invariant with respect to the gauge transformation (5.3.9) we obtain:
α = −1, m = 0 |
(5.3.20) |
Exactly the same result is obtained by imposing that the divergence of the right hand side should vanish as a consequence of the field equation. In this way, we realize that gauge invariance and electric current conservation imply each other. On the other hand the choice (5.3.20) of the parameters reproduces (5.3.13). Hence the gauge action (5.3.16), which is quadratic in the curvature tensor Fμν , is uniquely selected by the fundamental physical principle of electric charge conservation encoding the full structure of electrodynamical interactions. Let us analyze the geometrical structure of the action (5.3.16). To this effect we need to introduce a new involutive operation acting on differential forms which is named Hodge duality.
5.3.1 Hodge Duality
Consider a Riemannian manifold (M , g) of dimension m and let us construct the graded algebra of differential forms on M , defined by (2.5.59), which we repeat here for reader’s convenience:
