- •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
2.6 Homotopy, Homology and Cohomology |
81 |
Fig. 2.31 Homology versus cohomology groups
2.6.3 Homology and Cohomology Groups: General Construction
Let π : X → Y be a linear map between vector spaces. We define kernel of π and we denote ker π the subspace of X whose elements have the property of being mapped into 0 Y by π :
ker π = ,x X/π(x) = 0 Y - |
(2.6.38) |
We call image of π and we denote Im π the subspace of Y whose elements have the property that they are the image through π of some element of X:
Im π = ,y Y / x X/π(x) = y-
A nilpotent operator that acts on a sequence of vector spaces Xi of linear maps πi :
π1 |
π2 |
πi |
X1 −→ X2 |
−→ X3 |
−→ · · · −→ Xi −→ Xi+1 |
that have the following property:
(2.6.39)
defines a sequence
(2.6.40)
Im πi ker πi+1 |
(2.6.41) |
The inclusion of Im πi in ker πi+1 is what has been pictorially described in Fig. 2.31 and applies both to the boundary and to the exterior derivative operator. This situation suggests the following terminology:
Definition 2.6.9 In every space Ck (M , R) we name cycles the elements of ker ∂, namely the chains C , whose boundary vanishes ∂C = 0. Similarly in every space Λk (M ) we name closed forms or cocycles the elements of ker d, namely the differential forms ω such that dω = 0.
82 |
2 Manifolds and Fibre Bundles |
|
At the same time: |
Definition 2.6.10 In every space Ck (M , R) we name boundaries all k-chains that are the boundary of a k + 1-chain:
C (k) = boundary C (k) = ∂C (k+1) |
(2.6.42) |
Similarly in every space Λk (M ) we name exact forms or coboundaries all dif-
ferential forms ω(k) such that they can be written as the exterior derivative of a (k − 1)-form: ω(k) = dω(k−1).
Clearly (2.6.41) can be translated by saying that every boundary is a cycle and every coboundary is a cocycle. The reverse statement, however, is not true in general. There are cycles that are not boundaries and there are cocycles that are not coboundaries.
The concept of homology (or cohomology) previously discussed in an intuitive way can be formalized in the following way.
Definition 2.6.11 Consider the k-cycles. We say that two cycles C1(k) and C2(k) are homologous and we write C1(k) C2(k) if their difference is a boundary:
C(k) |
|
C(k) |
|
C(k+1) |
/C(k) |
− |
C(k) |
= |
∂C(k+1) |
(2.6.43) |
1 |
2 |
3 |
1 |
2 |
3 |
|
Clearly homology is an equivalence relation since:
C1(k) |
|
C2(k) |
= |
∂Ca(k+1) . |
|
(k) |
(k) |
(k |
+ |
1) |
(k |
+ |
1) |
|
(2.6.44) |
C(k) |
− C(k) |
∂C(k+1) |
C1 |
− C3 |
= ∂ Ca |
|
+ Cb |
|
|||||||
2 |
− |
3 |
= |
b |
|
|
|
|
|
|
|
|
|
|
|
Definition 2.6.12 We name kth homology group and we denote Hk (M , R) the group of equivalence classes of the kth cycles with respect to the k-boundaries.
Similarly we define kth cohomology group and we denote H k (M , R) the group of equivalence classes of the k-cocycles with respect to the kth coboundaries. Indeed we say that two closed forms ω and ω are cohomologous if their difference is an exact form: ω ω φ/ω − ω = dφ.
More generally when we have a sequence of vector spaces Xi as in (2.6.40) and a sequence of linear maps πi satisfying (2.6.41) we define the cohomology groups relative to the operator π as:
H(πi |
ker πi |
|
) ≡ Im πi−1 |
(2.6.45) |
The relation existing between homology and cohomology is fully contained in the following formula which generalizes to an arbitrary smooth manifold and to
2.6 Homotopy, Homology and Cohomology |
83 |
differential forms of any degree the familiar Gauss lemma or Stokes lemma:
|
(k |
+ |
1) ω(k) = |
|
(k |
+ |
1) dω(k) |
(2.6.46) |
∂C |
|
|
C |
|
|
|
Equation (2.6.46), whose general proof we omit, implies that in the case C (k) is a cycle we have:
|
ω(k) |
+ |
dφ(k−1) |
|
ω(k) |
(2.6.47) |
C (k) |
|
|
= |
C (k) |
|
namely the integral of a closed differential form along a cycle depends only on the cohomology class and not on the choice of the representative. Similarly if ω(k) is a closed form:
|
|
ω(k) = |
ω(k) |
(2.6.48) |
C (k)+∂C (k+1) |
C (k) |
|
namely the integral of a cocycle along a cycle depends on the homology class of the class and not on the choice of the representative inside the class.
2.6.4 Relation Between Homotopy and Homology
The relation between homotopy and homology groups of a manifold is provided by a fundamental theorem of algebraic geometry that we state without proof:
Theorem 2.6.4 Let M be a smooth manifold. Then there exists a homomorphism:
χ : π1(M ) → H1(M , Z) |
(2.6.49) |
that sends the homotopy class of each loop γ into the 1-simplex γ . If M is arcwise connected, then the map χ is surjective and the kernel of χ is the subgroup of commutators in π1(M ).
We recall that the subgroup of commutators of a discrete group G is the group G generated by all elements of the form x−1y−1xy for some x, y G.
From this theorem we have two consequences:
Corollary 2.6.1 If π1(M ) is Abelian, then H1(M ) π1(M ), namely the homotopy and cohomology groups coincide.
Corollary 2.6.2 If a manifold M is simply connected (π1(M ) = 1) then also the first homology group is trivial H1(M ) = 0.
The second of the above corollaries implies that in a simply connected manifold every closed loop is homologous to zero, namely it is the boundary of some region.
