- •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
62 |
2 Manifolds and Fibre Bundles |
Fig. 2.19 The 2-sphere
and hence:
∞ |
d |
∞ |
d |
∞ |
t = − ck zS2−k |
|
= dk zSk |
|
= − dk zN2−k |
dzS |
dzS |
|||
k=0 |
|
k=0 |
|
k=0 |
The only way for (2.5.16) to be self consistent is to have:
k > 2 ck = dk = 0; c0 = −d2, c1 = −d1,
d |
∞ |
d |
|
|
= ck zNk |
|
|
dzN |
dzN |
||
|
k=0 |
(2.5.16) |
|
|
|
||
c2 |
= −d0 |
(2.5.17) |
This shows that the space of holomorphic sections of the tangent bundle T S2 is a finite dimensional vector space of dimension three spanned by the three differential operators:
L0 |
= −z |
d |
|
||||
|
|
|
|
|
|||
dz |
|
||||||
L1 |
= − |
d |
(2.5.18) |
||||
|
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|
|||||
dz |
|||||||
L−1 |
= −z2 |
|
d |
|
|||
|
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||||||
dz |
|
We will have more to say about these operators in the sequel.
What we have so far discussed can be summarized by stating the transformation rule of vector field components when we change coordinate patch form xμ to xμ :
∂xμ |
|
tμ x = tν (x) ∂xν |
(2.5.19) |
Indeed a convenient way of defining a fibre-bundle is provided by specifying the way its sections transform from one local trivialization to another one which amounts to giving all the transition functions. This method can be used to discuss the construction of the cotangent bundle.
2.5.2 The Lie Algebra of Vector Fields
In Sect. 2.3 we saw that the tangent space TpM at point p M of a manifold can be identified with the vector space of derivations of the algebra of germs (see
2.5 Tangent and Cotangent Bundles |
63 |
Definition 2.3.5). After gluing together all tangent spaces into the tangent bundle T M such an identification of tangent vectors with the derivations of an algebra can be extended from the local to the global level. The crucial observation is that the set of smooth functions on a manifold C∞(M ) constitutes an algebra with respect to point-wise multiplication just as the set of germs at point p. The vector fields, namely the sections of the tangent bundle, are derivations of this algebra. Indeed each vector field X Γ (T M , M ) is a linear map of the algebra C∞(M ) into itself:
X : C∞(M ) → C∞(M ) |
(2.5.20) |
that satisfies the analogue properties of those mentioned in (2.3.21) for tangent vectors, namely:
X(αf + βg) = αX(f ) + βX(g) |
|
X(f · g) = X(f ) · g + f · X(g) |
(2.5.21) |
α, β R (or C); f, g C∞(M ) |
|
On the other hand the set of vector fields, renamed for this reason: |
|
Diff(M ) ≡ Γ (T M , M ) |
(2.5.22) |
forms a Lie algebra with respect to the following Lie bracket operation: |
|
[X, Y]f = X Y(f ) − Y X(f ) |
(2.5.23) |
Indeed the set of vector fields is a vector space with respect the scalar numbers (R or C, depending on the type of manifold, real or complex), namely we can take linear combinations of the following form:
λ, μ R or C X, Y Diff(M ) : λX + μY Diff(M ) |
(2.5.24) |
having defined:
[λX + μY](f ) = λ X(f ) + μ Y(f ) , f C∞(M ) |
(2.5.25) |
Furthermore the operation (2.5.23) is the commutator of two maps and as such it is antisymmetric and satisfies the Jacobi identity.
The Lie algebra of vector fields is named Diff(M ) since each of its elements can be interpreted as the generator of an infinitesimal diffeomorphism of the manifold onto itself. As we are going to see Diff(M ) is a Lie algebra of infinite dimension, but it can contain finite dimensional subalgebras generated by particular vector fields. The typical example will be the case of the Lie algebra of a Lie group: this is the finite dimensional subalgebra G Diff(G) spanned by those vector fields defined on the Lie group manifold that have an additional property of invariance with respect to either left or right translations (see Chap. 3).
64 |
2 Manifolds and Fibre Bundles |
2.5.3 The Cotangent Bundle and Differential Forms
Let us recall that a differential 1-form in the point p M of a manifold M , namely an element ωp Tp M of the cotangent space over such a point was defined as a real valued linear functional over the tangent space at p, namely
ωp Hom(Tp M , R) |
(2.5.26) |
which implies: |
|
tp Tp M ωp : tp → ωp(tp ) R |
(2.5.27) |
The expression of ωp in a coordinate patch around p is: |
|
ωp = ωμ(p) dxμ |
(2.5.28) |
where dxμ(p) are the differentials of the coordinates and ωμ(p) are real numbers. We can glue together all the cotangent spaces and construct the cotangent bundles by stating that a generic smooth section of such a bundle is of the form (2.5.28) where ωμ(p) are now smooth functions of the base manifold point p. Clearly if we change coordinate system, an argument completely similar to that employed in the case of the tangent bundle tells us that the coefficients ωμ(x) transform as follows:
∂xν |
|
ωμ x = ων (x) ∂xμ |
(2.5.29) |
and (2.5.29) can be taken as a definition of the cotangent bundle T M , whose sections transform with the Jacobian matrix rather than with the inverse Jacobian matrix as the sections of the tangent bundle do (see (2.5.19)). So we can write the
Definition 2.5.3 A differential 1-form ω on a manifold M is a section of the cotangent bundle, namely ω Γ (T M , M ).
This means that a differential 1-form is a map: |
|
ω : Γ (T M , M ) → C∞(M ) |
(2.5.30) |
from the space of vector fields (i.e. the sections of the tangent bundle) to smooth functions. Locally we can write:
|
|
Γ (T M , M ) ω = ωμ(x) dxμ |
(2.5.31) |
|||||
|
|
Γ T M , M t = tμ(x) |
∂ |
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||||
|
|
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|
||||
|
|
∂xμ |
|
|||||
and we obtain |
|
|
|
|
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|
|
|
|
= |
|
∂xν |
= |
|
|
|
|
ω(t) |
|
ωμ(x)tν (x) dxμ |
∂ |
|
|
ωμ(x)tμ(x) |
(2.5.32) |
|
|
|
|
using
2.5 Tangent and Cotangent Bundles |
65 |
dxμ |
∂ |
= δνμ |
(2.5.33) |
∂xν |
which is the statement that coordinate differentials and partial derivatives are dual bases for 1-forms and tangent vectors respectively.
Since T M is a vector bundle it is meaningful to consider the addition of its sections, namely the addition of vector fields and also their pointwise multiplication by smooth functions. Taking this into account we see that the map (2.5.30) used to define sections of the cotangent bundle, namely 1-forms is actually an F-linear map. This means the following. Considering any F-linear combination of two vector fields, namely:
f1t1 + f2t2, f1, f2 C∞(M ) t1, t2 Γ (T M , M ) |
(2.5.34) |
for any 1-form ω Γ (T M , M ) we have: |
|
ω(f1t1 + f2t2) = f1(p)ω(t1)(p) + f2(p)ω(t2)(p) |
(2.5.35) |
where p M is any point of the manifold M .
It is now clear that the definition of differential 1-form generalizes the concept of total differential of the germ of a smooth function. Indeed in an open neighborhood
U M of a point p we have: |
|
|
= |
|
|
||
|
|
|
p |
|
∂μf dxμ |
(2.5.36) |
|
|
f |
|
C∞(M ) |
df |
|
||
and the value of df at p on any tangent vector tp Tp M is defined to be: |
|
||||||
|
|
dfp (tp ) ≡ tp(f ) = tμ∂μf |
(2.5.37) |
which is the directional derivative of the local function f along tp in the point p. If rather than the germ of a function we take a global function f C∞(M ) we realize that the concept of 1-form generalizes the concept of total differential of such a function. Indeed the total differential df fits into the definition of a 1-form, since for any vector field t Γ (T M , M ) we have:
df (t) = tμ(x)∂μf (x) ≡ tf C∞(M ) |
(2.5.38) |
A first obvious question is the following. Is any 1-form ω = ωμ(x) dxμ the differential of some function? The answer is clearly no and in any coordinate patch there
is a simple test to see whether this is the case or not. Indeed, if ωμ(1)
germ f |
|
p |
|
|
|
|
|
C∞(M ) then we must have: |
|
|
|||
|
|
1 |
∂μων(1) − ∂ν ωμ(1) = |
1 |
[∂μ, ∂ν ]f = 0 |
|
|
|
|
|
|
||
|
|
2 |
2 |
= ∂μf for some
(2.5.39)
The left hand side of (2.5.39) are the components of what we will name a differential 2-form
ω(2) = ωμν(2) dxμ dxν |
(2.5.40) |