- •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 |
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m |
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A (M ) = * Ak (M ) where m = dim M |
(5.3.21) |
k=0 |
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For the above construction of differential forms, the manifold structure is sufficient, the existence of a metric being completely irrelevant. Yet if a metric structure is present, the algebra A (M ) can be equipped with a linear (anti-)involutive operation, named Hodge duality which maps forms of degree k into forms of degree m − k:
: Ak (M ) → Am−k (M ) |
(5.3.22) |
and is explicitly realized as follows. Let ω(k) Ak (M ) be a k-form. In any coordinate patch we have:
ω(k) = ωμ1...μk dxμ1 · · · dxμk |
(5.3.23) |
The Hodge dual of ω(k), denoted ω(k) is the m − k form with the following components:
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ω(k) = |
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· · · dxνm−k εμ1...μkν1...νm−k |
(5.3.24) |
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In the above equation εμ1...μkν |
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Civita symbol whose first k indices have been raised by means of the metric tensor. As a consequence of the above definition we find:
2ω(k) = (−1)(m−k)k det(sign)ω(k) |
(5.3.25) |
where det(sign) denotes the determinant of the signature of the considered metric which is either +1 or −1.
5.3.2 Geometrical Rewriting of the Gauge Action
Using the Hodge dual operation we can easily rewrite the gauge action (5.3.16) in the following way:
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Fμν F μν d4x |
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What we learnt from the above discussion is that the structure of Maxwell equations is completely determined by the gauge nature of the electromagnetic field and this fact is just the mathematical transcription of the Physical Conservation Law of Electric Charge. On the other hand the unique structure of Maxwell equations implies an Action Principle (5.3.27) which is quadratic in the curvature F of the
200 |
5 Einstein Versus Yang-Mills Field Equations |
principle connection A and cannot be written without the use of the Hodge dual. The latter contains the metric tensor gμν in disguise. In other words, although the electromagnetic field Aμ coincides with a principle connection on a U(1)-fibre bundle, whose construction involves only the manifold structure of the space-time base manifold M , the classical dynamics of Aμ, i.e. its propagation equations and interaction with other fields, can neither be formulated nor solved without invoking the metric structure of M . In short the electromagnetic U(1)-bundle needs to be constructed on a (pseudo-)Riemannian base manifold.
This is the first signal of the basic difference between gravity and the other fundamental interactions. All interactions are mediated by gauge fields which happen to be principle connections on fibre bundles, yet the connections involved by gravity are special in that they deal with the tangent bundle T M of the spacetime manifold M , which is the base manifold not only for T M , but also for all the other principle-bundles P (M , G) associated with non-gravitational interactions. The structure (5.3.27) implies an obligatory and a priori predetermined interaction of every other gauge field with the gravitational one, namely with the metric. Here is the source of universality for gravity.
5.3.3 Yang-Mills Theory in Vielbein Formalism
In view of our advertised preference for the Cartan viewpoint and of our announced plan of trading the metric for the vielbein, a natural question arises about the formulation of electrodynamics in vielbein formalism. If we are going to discard the metric tensor, how can we rewrite the action principle (5.3.27) without using Hodge duality? The answer we presently provide to such a question illustrates the basic spirit of the Repère Mobile philosophy: all fundamental operations are lifted to the Lorentz fibres, where they take the same appearance as in flat Minkowski space. What happens in the Lorentz bundle is then transmitted to the tangent bundle through the soldering of the two-bundles which is implemented by the vielbein, via the vanishing of the Torsion.
Since there is no difference, in this respect, between the Abelian gauge theory of Electrodynamics and the non-Abelian Yang-Mills theories utilized in the description of electro-weak and strong interactions, we immediately address the most general case. We consider a principle bundle P (M , G) where G is the structural group (= gauge group in physical parlance) and the G -Lie algebra valued one-form A = A I TI is a principle connection (i.e. a gauge field in physical parlance). The corresponding curvature two-form is defined below:
F ≡ dA + A A |
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5.3 The Structure of Classical Electrodynamics and Yang-Mills Theories |
201 |
the bracket in the second line of (5.3.28) providing the explicit definition of the two-forms FI . Each of these latter can be expanded along a basis of differentials:5
FI = FμνI dxμ dxν |
(5.3.29) |
In terms of the field strength FμνI the Yang-Mills action in m-dimensions takes a form which is the obvious generalization of (5.3.16) and (5.3.27), namely:
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F J |μν dmx |
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Tr(F |
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(5.3.30) |
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In (5.3.30) the symbol γI J denotes the G-invariant Killing metric on the Lie algebra G. Typically, choosing a linear representation of G, the generators TI become matrices that can be normalized in such a way that:6
Tr(TI TJ ) = γI J |
(5.3.31) |
The above equation explains the second identity in (5.3.30).
Let us then solve the task of recasting the Yang-Mills action (5.3.30) into the framework of the vielbein formalism. To this effect we begin from the volume form, namely from the generally covariant integration measure on an m-dimensional space-time. In metric formalism, if we are supposed to integrate any scalar function f(x) on a (pseudo-)Riemannian manifold, we just write:
f(x)Volg = f(x) − det g dmx (5.3.32)
In view of the identification (5.2.9), the above equation can be rewritten as follows:
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5Note that from now on we omit the factor 12 introduced in the electromagnetic analogue of (5.3.29), namely in (5.3.10). There such a factor was used in order for Fμν to have the traditional normalization Fμν = ∂μAν − ∂ν Aμ . Omitting this factor the normalization of Fμν becomes the less traditional one: Fμν = 12 (∂μAν − ∂ν Aμ + A A − terms). Paying this moderate price all formulae become much neater and deprived of annoying prefactors.
6An important comment is obligatory at this point. A fundamental theorem of Lie Algebra Theory, states that the Killing metric of a compact semi-simple Lie algebra is always negative definite. So, as long as, the gauge group G is chosen compact, as it is the case in all standard gauge theories of non-gravitational interactions, the kinetic term of the gauge fields defined by the action (5.3.31) turns out to have correct positive definiteness properties and the corresponding quanta have physical propagators. In the case of non-compact gauge algebras the action (5.3.31) introduces negative norm states in the spectrum. This does not mean that non-compact gauge groups are altogether forbidden. Actually they appear in supergravity theories yet the corresponding kinetic terms have a more sophisticated structure which takes care of unitarity.
202 |
5 Einstein Versus Yang-Mills Field Equations |
where εa1...am denotes the completely antisymmetric Levi Civita tensor with flat indices. Indeed it suffices to observe that:
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· · · Eam εa1...am |
= |
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· · · dxμm |
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(5.3.34) |
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In the above equation the writing det E denotes the determinant of the square matrix Eμa (x) and the last identity follows from (5.2.9) which implies det g = (det E)2 × (det η) = −(det E)2.
This being clarified the gauge action (5.3.30) of a Yang-Mills field in a m- dimensional, Lorentz signature, space-time can be rewritten in the vielbein approach, utilizing a first order formalism. Consider the following action functional:
AY M = − |
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Tr F abF Ec1 · · · Ecm−2 |
εc1...cm−2ab |
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Tr F abFab |
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where Fab = FabI TI is a 0-form transforming as a section of the second antisym-
π
metric power of the Lorentz vector bundle Vso(1,m−1) → M mentioned in (5.2.13):
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FabI Γ 7 2Vso(1,m−1), M |
(5.3.36) |
In addition, F I |
is also a section of an associated vector bundle to the principle |
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gauge bundle P (M , G), to be precise, the vector bundle of the adjoint representation. This object should be regarded as an independent dynamical variable with respect to which we are supposed to vary the action functional (5.3.35). Performing such a variation we find the equation:
0 = − |
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Ec1 · · · Ecm−2 |
εc1...cm−2ab |
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which admits a unique solution: |
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FI = FabI Ea Eb |
(5.3.38) |
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The argument goes as follows. Since the curvature FI is a horizontal two-form leaving on the cotangent bundle of the base manifold M it can always be expanded along a basis of local sections of T M , namely along an independent basis of oneforms. The coordinate differentials dxμ provide such a basis but, by construction,
5.3 The Structure of Classical Electrodynamics and Yang-Mills Theories |
203 |
the vielbein {Ea } provide another possible basis. Hence, without loss of generalities we can always pose:
FI = FabI Ea Eb |
(5.3.39) |
where FabI is just the name given to the components of FI |
in the vielbein basis. |
Inserting (5.3.39) into (5.3.37) we easily realize that it reduces to the algebraic condition FabI = FabI and (5.3.38) follows.
The obtained result implies that the 0-form field FabI is identified, through its own equation of motion with the gauge field strength with flattened indices, namely:
FabI |
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= FμνI EaμEbν |
the symbol Eaμ denoting the inverse vielbein. Using (5.3.40) we find
Tr F abFab = Tr F μν Fμν
while using (5.3.38) we get:
− (m |
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which implies that
A2Y M = 1 Tr(F F)
2
(5.3.40)
(5.3.41)
(5.3.42)
(5.3.43)
once (5.3.40) is implemented.
In this way we have shown how to rewrite the Yang-Mills action (5.3.30) without using neither the operation of Hodge duality nor the metric. The price we had to pay was the introduction of a new auxiliary field which satisfies an algebraic equation of motion and can be eliminated inserting the solution of the latter back into the action. Furthermore, the action in the form (5.3.35) displays the coupling of the Yang-Mills fields to the Poincaré connection. The spin connection ωab is not present, yet the vielbein Ea appears explicitly and is an essential ingredient of the construction.
The reconstruction of classical Yang-Mills theory can now be completed in the set up of (5.3.35) by considering the variation with respect to the connection oneform A I . This yields the following equation:
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where |
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F I |ab |
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ωbcF I |acη |
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