- •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
3.4 Connections on a Vector Bundle |
127 |
3.4 Connections on a Vector Bundle
π
Let us now consider a generic vector bundle E = M of rank r. Its standard fi- bre is an r-dimensional vector space V and the transition functions from one local trivialization to another one are maps:
#
ψαβ : Uα Uβ → Hom(V, V) GL(r, R) (3.4.1)
In other words, without further restrictions the structural group of a generic vector bundle is just GL(r, R).
The notion of a connection on generic vector bundles is formulated according to the following:
π π
Definition 3.4.1 Let E = M be a vector bundle, T M = M the tangent bundle to the base manifold M (dim M = m) and let Γ (E, M ) be the space of sections of E: a connection on E is a rule that, to each vector field X Γ (T M , M ) associates a map:
X : Γ (E, M ) → Γ (E, M ) |
(3.4.2) |
satisfying the following defining properties:
(a)X(a1s1 + b1s2) = a1 Xs1 + a2 Xs2
(b)a1X1+a2X2 s = a1 X1 s + a2 X2 s
(c)X(f · s) = X(f ) · s + f · Xs
(d)f ·Xs = f · Xs
where a1,2 R are real numbers, s1,2 Γ (E, M ) are section of the vector bundle and f C∞(M ) is a smooth function.
The abstract description of a connection provided by Definition 3.4.1 becomes more explicit if we consider bases of sections for the two involved vector bundles.
π
To this effect let {si (p)} be a basis of sections of the vector bundle E = M (i = 1, 2, . . . , r = rank E) and let {eμ(p)}, (μ = 1, 2, . . . , m = dim M ) be a basis
π
of sections for the tangent bundle to the base manifold T M = M . Then we can write:
eμ si ≡ μsi = Θμi j sj |
(3.4.3) |
where the local functions Θμi j (p), ( p M ) are named the coefficients of the connection. They are necessary and sufficient to specify the connection on an arbitrary section of the vector bundle. To this effect let s Γ (E, M ). By definition of basis of sections we can write:
s = ci (p)si (p) |
(3.4.4) |
and correspondingly we obtain:
128 |
3 Connections and Metrics |
μs = μci · si
(3.4.5)
μci ≡ ∂μci + Θμj i cj
having defined ∂μci ≡ eμ(ci ). Confronting this with the discussions at the end of Sect. 3.3.2.1, we see that in the language of physicists μci can be identified as the covariant derivatives of the vector components ci . Let us now observe that for any
π
vector bundle E = M if:
r ≡ rank(E)
is the rank, namely the dimension of the standard fibre and:
m ≡ dim M
is the dimension of the base manifold, the connection coefficients can be viewed as a set of m matrices, each of them r × r:
eμ(p) : Θμj i = (Θeμ )j i |
(3.4.6) |
Hence more abstractly we can say that the connection on a vector bundle associates to each vector field defined on the base manifold a matrix of dimension equal to the rank of the bundle:
X Γ (T M , M ) :
: X → ΘX = r × r-matrix depending on the base-point p M (3.4.7)
The relevant question is the following: can we relate the matrix ΘX to a one-form and make a bridge between the above definition of a connection and that provided by the Ehresmann approach? The answer is yes and it is encoded in the following equivalent:
π |
π |
Definition 3.4.2 Let E = M be a vector bundle, T |
M = M the cotangent |
bundle to the base manifold M (dim M = m) and let Γ (E, M ) be the space of sections of E: a connection on E is a map:
: Γ (E, M ) → Γ (E, M ) T M |
(3.4.8) |
which to each section s Γ (E, M ) associates a one-form s |
with values in |
Γ(E, M ) such that the following defining properties are satisfied:
(a)(a1s1 + b1s2) = a1 s1 + a2 s2
(b)(f · s) = df · s + f · s
where a1,2 R are real numbers, s1,2 Γ (E, M ) are section of the vector bundle and f C∞(M ) is a smooth function.
The relation between the two definitions of a connection on a vector bundle is now easily obtained by stating that for each section s Γ (E, M ) and for each vector field X Γ (T M , M ) we have:
3.4 Connections on a Vector Bundle |
129 |
Xs = s(X) |
(3.4.9) |
The reader can easily convince himself that using (3.4.9) and relying on the properties of s established by Definition 3.4.2 those of X s required by Definition 3.4.1 are all satisfied.
Consider now, just as before, a basis of sections of the vector bundle {si (p)}. According to its second Definition 3.4.2 a connection singles out an r × r matrixvalued one-form Θ Γ (T M , M ) through the equation:
si = Θi j sj |
(3.4.10) |
Clearly the connection coefficients introduced in (3.4.7) are nothing else but the values of Θ on each vector field X:
ΘX = Θ(X) |
(3.4.11) |
A natural question which arises at this point is the following. In view of our comments at the end of Sect. 3.3.2.1 could we identify Θ with the matrix representation of A , the principal connection on the corresponding principal bundle? In other words could we write:
Θ = D(A )? |
(3.4.12) |
For a single generic vector bundle this question seems tautological. Indeed the structural group is simply GL(r, R) and being the corresponding Lie algebra gl(r, R) made by the space of generic matrices it looks like obvious that Θ could be viewed as Lie algebra valued. The real question however is another. The identification (3.4.12) is legitimate if and only if Θ transforms as the matrix representation of A . This is precisely the case. Let us demonstrate it. Consider the intersection of two-
"
local trivializations. On Uα Uβ the relation between two bases of sections is given by:
si(α) = D(t(αβ))ij sj(β) |
(3.4.13) |
where t(αβ) is the transition function seen as an abstract group element. Equation (3.4.13) implies:
Θ(α) = D(dt(αβ)) · D(t(αβ))−1 + D(t(αβ)) · Θ(β) · D(t(αβ))−1 |
(3.4.14) |
which is consistent with the gauge transformation rule (3.3.89) if we identify Θ as in (3.4.12).
The outcome of the above discussion is that once we have defined a connection one-form A on a principle bundle P (M , G) a connection is induced on any
π
associated vector bundle E = M . It is simply defined as follows:
s Γ (E, M ) : s = ds + D(A )s |
(3.4.15) |
where D() denotes the linear representation of both G and G that define the associated bundle.