- •Preface
- •Acknowledgements
- •Contents
- •2.1 Introduction and a Short History of Black Holes
- •2.2 The Kruskal Extension of Schwarzschild Space-Time
- •2.2.1 Analysis of the Rindler Space-Time
- •2.2.2 Applying the Same Procedure to the Schwarzschild Metric
- •2.2.3 A First Analysis of Kruskal Space-Time
- •2.3 Basic Concepts about Future, Past and Causality
- •2.3.1 The Light-Cone
- •2.3.2 Future and Past of Events and Regions
- •Achronal Sets
- •Time-Orientability
- •Domains of Dependence
- •Cauchy surfaces
- •2.4.1 Conformal Mapping of Minkowski Space into the Einstein Static Universe
- •2.4.2 Asymptotic Flatness
- •2.5 The Causal Boundary of Kruskal Space-Time
- •References
- •3.1 Introduction
- •3.2 The Kerr-Newman Metric
- •3.2.1 Riemann and Ricci Curvatures of the Kerr-Newman Metric
- •3.3 The Static Limit in Kerr-Newman Space-Time
- •Static Observers
- •3.4 The Horizon and the Ergosphere
- •The Horizon Area
- •3.5 Geodesics of the Kerr Metric
- •3.5.2 The Hamilton-Jacobi Equation and the Carter Constant
- •3.5.3 Reduction to First Order Equations
- •3.5.4 The Exact Solution of the Schwarzschild Orbit Equation as an Application
- •3.5.5 About Explicit Kerr Geodesics
- •3.6 The Kerr Black Hole and the Laws of Thermodynamics
- •3.6.1 The Penrose Mechanism
- •3.6.2 The Bekenstein Hawking Entropy and Hawking Radiation
- •References
- •4.1 Historical Introduction to Modern Cosmology
- •4.2 The Universe Is a Dynamical System
- •4.3 Expansion of the Universe
- •4.3.1 Why the Night is Dark and Olbers Paradox
- •4.3.2 Hubble, the Galaxies and the Great Debate
- •4.3.4 The Big Bang
- •4.4 The Cosmological Principle
- •4.5 The Cosmic Background Radiation
- •4.6 The New Scenario of the Inflationary Universe
- •4.7 The End of the Second Millennium and the Dawn of the Third Bring Great News in Cosmology
- •References
- •5.1 Introduction
- •5.2 Mathematical Interlude: Isometries and the Geometry of Coset Manifolds
- •5.2.1 Isometries and Killing Vector Fields
- •5.2.2 Coset Manifolds
- •5.2.3 The Geometry of Coset Manifolds
- •5.2.3.1 Infinitesimal Transformations and Killing Vectors
- •5.2.3.2 Vielbeins, Connections and Metrics on G/H
- •5.2.3.3 Lie Derivatives
- •5.2.3.4 Invariant Metrics on Coset Manifolds
- •5.2.3.5 For Spheres and Pseudo-Spheres
- •5.3 Homogeneity Without Isotropy: What Might Happen
- •5.3.1 Bianchi Spaces and Kasner Metrics
- •5.3.1.1 Bianchi Type I and Kasner Metrics
- •5.3.2.1 A Ricci Flat Bianchi II Metric
- •5.3.3 Einstein Equation and Matter for This Billiard
- •5.3.4 The Same Billiard with Some Matter Content
- •5.3.5 Three-Space Geometry of This Toy Model
- •5.4 The Standard Cosmological Model: Isotropic and Homogeneous Metrics
- •5.4.1 Viewing the Coset Manifolds as Group Manifolds
- •5.5 Friedman Equations for the Scale Factor and the Equation of State
- •5.5.1 Proof of the Cosmological Red-Shift
- •5.5.2 Solution of the Cosmological Differential Equations for Dust and Radiation Without a Cosmological Constant
- •5.5.3 Embedding Cosmologies into de Sitter Space
- •5.6 General Consequences of Friedman Equations
- •5.6.1 Particle Horizon
- •5.6.2 Event Horizon
- •5.6.3 Red-Shift Distances
- •5.7 Conceptual Problems of the Standard Cosmological Model
- •5.8 Cosmic Evolution with a Scalar Field: The Basis for Inflation
- •5.8.1 de Sitter Solution
- •5.8.2 Slow-Rolling Approximate Solutions
- •5.8.2.1 Number of e-Folds
- •5.9 Primordial Perturbations of the Cosmological Metric and of the Inflaton
- •5.9.1 The Conformal Frame
- •5.9.2 Deriving the Equations for the Perturbation
- •5.9.2.1 Meaning of the Propagation Equation
- •5.9.2.2 Evaluation of the Effective Mass Term in the Slow Roll Approximation
- •5.9.2.3 Derivation of the Propagation Equation
- •5.9.3 Quantization of the Scalar Degree of Freedom
- •5.9.4 Calculation of the Power Spectrum in the Two Regimes
- •5.9.4.1 Short Wave-Lengths
- •5.9.4.2 Long Wave-Lengths
- •5.9.4.3 Gluing the Long and Short Wave-Length Solutions Together
- •5.9.4.4 The Spectral Index
- •5.10 The Anisotropies of the Cosmic Microwave Background
- •5.10.1 The Sachs-Wolfe Effect
- •5.10.2 The Two-Point Temperature Correlation Function
- •5.10.3 Conclusive Remarks on CMB Anisotropies
- •References
- •6.1 Historical Outline and Introduction
- •6.1.1 Fermionic Strings and the Birth of Supersymmetry
- •6.1.2 Supersymmetry
- •6.1.3 Supergravity
- •6.2 Algebro-Geometric Structure of Supergravity
- •6.3 Free Differential Algebras
- •6.3.1 Chevalley Cohomology
- •Contraction and Lie Derivative
- •Definition of FDA
- •Classification of FDA and the Analogue of Levi Theorem: Minimal Versus Contractible Algebras
- •6.4 The Super FDA of M Theory and Its Cohomological Structure
- •6.4.1 The Minimal FDA of M-Theory and Cohomology
- •6.4.2 FDA Equivalence with Larger (Super) Lie Algebras
- •6.5 The Principle of Rheonomy
- •6.5.1 The Flow Chart for the Construction of a Supergravity Theory
- •6.6 Summary of Supergravities
- •Type IIA Super-Poicaré Algebra in the String Frame
- •The FDA Extension of the Type IIA Superalgebra in the String Frame
- •The Bianchi Identities
- •6.7.1 Rheonomic Parameterizations of the Type IIA Curvatures in the String Frame
- •Bosonic Curvatures
- •Fermionic Curvatures
- •6.7.2 Field Equations of Type IIA Supergravity in the String Frame
- •6.8 Type IIB Supergravity
- •SL(2, R) Lie Algebra
- •Coset Representative of SL(2, R)/O(2) in the Solvable Parameterization
- •The SU(1, 1)/U(1) Vielbein and Connection
- •6.8.2 The Free Differential Algebra, the Supergravity Fields and the Curvatures
- •The Curvatures of the Free Differential Algebra in the Complex Basis
- •The Curvatures of the Free Differential Algebra in the Real Basis
- •6.8.3 The Bosonic Field Equations and the Standard Form of the Bosonic Action
- •6.9 About Solutions
- •References
- •7.1 Introduction and Conceptual Outline
- •7.2 p-Branes as World Volume Gauge-Theories
- •7.4 The New First Order Formalism
- •7.4.1 An Alternative to the Polyakov Action for p-Branes
- •7.6 The D3-Brane: Summary
- •7.9 Domain Walls in Diverse Space-Time Dimensions
- •7.9.1 The Randall Sundrum Mechanism
- •7.9.2 The Conformal Gauge for Domain Walls
- •7.10 Conclusion on This Brane Bestiary
- •References
- •8.1 Introduction
- •8.2 Supergravity and Homogeneous Scalar Manifolds G/H
- •8.2.3 Scalar Manifolds of Maximal Supergravities in Diverse Dimensions
- •8.3 Duality Symmetries in Even Dimensions
- •8.3.1 The Kinetic Matrix N and Symplectic Embeddings
- •8.3.2 Symplectic Embeddings in General
- •8.5 Summary of Special Kähler Geometry
- •8.5.1 Hodge-Kähler Manifolds
- •8.5.2 Connection on the Line Bundle
- •8.5.3 Special Kähler Manifolds
- •8.6 Supergravities in Five Dimension and More Scalar Geometries
- •8.6.1 Very Special Geometry
- •8.6.3 Quaternionic Geometry
- •8.6.4 Quaternionic, Versus HyperKähler Manifolds
- •References
- •9.1 Introduction
- •9.2 Black Holes Once Again
- •9.2.2 The Oxidation Rules
- •Orbit of Solutions
- •The Schwarzschild Case
- •The Extremal Reissner Nordström Case
- •Curvature of the Extremal Spaces
- •9.2.4 Attractor Mechanism, the Entropy and Other Special Geometry Invariants
- •9.2.5 Critical Points of the Geodesic Potential and Attractors
- •At BPS Attractor Points
- •At Non-BPS Attractor Points of Type I
- •At Non-BPS Attractor Points of Type II
- •9.2.6.2 The Quartic Invariant
- •9.2.7.1 An Explicit Example of Exact Regular BPS Solution
- •The Metric
- •The Scalar Field
- •The Electromagnetic Fields
- •The Fixed Scalars at Horizon and the Entropy
- •The Metric
- •The Scalar Field
- •The Electromagnetic Fields
- •The Fixed Scalars at Horizon and the Entropy
- •9.2.9 Resuming the Discussion of Critical Points
- •Non-BPS Case
- •BPS Case
- •9.2.10 An Example of a Small Black Hole
- •The Metric
- •The Complex Scalar Field
- •The Electromagnetic Fields
- •The Charges
- •Structure of the Charges and Attractor Mechanism
- •9.2.11 Behavior of the Riemann Tensor in Regular Solutions
- •9.3.4 The SO(8) Spinor Bundle and the Holonomy Tensor
- •9.3.5 The Well Adapted Basis of Gamma Matrices
- •9.3.6 The so(8)-Connection and the Holonomy Tensor
- •9.3.7 The Holonomy Tensor and Superspace
- •9.3.8 Gauged Maurer Cartan 1-Forms of OSp(8|4)
- •9.3.9 Killing Spinors of the AdS4 Manifold
- •9.3.10 Supergauge Completion in Mini Superspace
- •9.3.11 The 3-Form
- •9.4.1 Maurer Cartan Forms of OSp(6|4)
- •9.4.2 Explicit Construction of the P3 Geometry
- •9.4.3 The Compactification Ansatz
- •9.4.4 Killing Spinors on P3
- •9.4.5 Gauge Completion in Mini Superspace
- •9.4.6 Gauge Completion of the B[2] Form
- •9.5 Conclusions
- •References
- •10.1 The Legacy of Volume 1
- •10.2 The Story Told in Volume 2
- •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: Auxiliary Tools for p-Brane Actions
- •B.1 Notations and Conventions
- •Appendix C: Auxiliary Information About Some Superalgebras
- •C.1.1 The Superalgebra
- •C.2 The Relevant Supercosets and Their Relation
- •C.2.1 Finite Supergroup Elements
- •C.4 An so(6) Inversion Formula
- •Appendix D: MATHEMATICA Package NOVAMANIFOLDA
- •Coset Manifolds (Euclidian Signature)
- •Instructions for the Use
- •Description of the Main Commands of RUNCOSET
- •Structure Constants for CP2
- •Spheres
- •N010 Coset
- •RUNCOSET Package (Euclidian Signature)
- •Main
- •Spin Connection and Curvature Routines
- •Routine Curvapack
- •Routine Curvapackgen
- •Contorsion Routine for Mixed Vielbeins
- •Calculation of the Contorsion for General Manifolds
- •Calculation for Cartan Maurer Equations and Vielbein Differentials (Euclidian Signature)
- •Routine Thoft
- •AdS Space in Four Dimensions (Minkowski Signature)
- •Lie Algebra of SO(2, 3) and Killing Metric
- •Solvable Subalgebra Generating the Coset and Construction of the Vielbein
- •Killing Vectors
- •Trigonometric Coordinates
- •Test of Killing Vectors
- •MANIFOLDPROVA
- •The 4-Dimensional Coset CP2
- •Calculation of the (Pseudo-)Riemannian Geometry of a Kasner Metric in Vielbein Formalism
- •References
- •Index
382 |
9 Supergravity: An Anthology of Solutions |
and the spectrum of fluctuations of the background arranges into Osp(N | 4) supermultiplets furthermore assigned to suitable representations of the bosonic flavor group.
9.3.4 The SO(8) Spinor Bundle and the Holonomy Tensor
We come next to discuss a very important property of 7-manifolds with a spin structure which plays a crucial role in understanding the supergauge completion. This is the existence of an SO(8) vector bundle whose non-trivial connection is defined by the Riemannian structure of the manifold. To introduce this point and in order to illustrate its relevance to our problem we begin by considering a basis of D = 11 gamma matrices well adapted to the compactification on AdS4 × M7.
9.3.5 The Well Adapted Basis of Gamma Matrices
According to the tensor product representation well adapted to the compactification, the D = 11 gamma matrices can be written as follows:
Γa = γa |
18×8 |
(a = 0, 1, 2, 3) |
(9.3.62) |
Γ3+α = γ5 τα |
(α = 1, . . . , 7) |
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where, following the old Kaluza Klein supergravity literature [26, 30, 41] the matrices τα are the real antisymmetric realization of the SO(7) Clifford algebra with negative metric:
{τα , τβ } = −2δαβ ; |
τα = −(τα )T |
(9.3.63) |
In this basis the charge conjugation matrix is given by: |
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C = C 18×8 |
(9.3.64) |
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where C is the charge conjugation matrix in d = 4: |
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C γa C −1 = −γaT ; |
C T = −C |
(9.3.65) |
9.3.6 The so(8)-Connection and the Holonomy Tensor
Next we observe that using these matrices the covariant derivative introduced in (9.3.48) defines a universal so(8)-connection on the spinor bundle which is given once the Riemannian structure is given, namely once the vielbein and the spin con-
9.3 Flux Vacua of M-Theory and Manifolds of Restricted Holonomy |
383 |
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More precisely, let ζA7 be an orthonormal basis: |
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of sections of the spinor bundle over the Einstein manifold M7. Any spinor can be written as a linear combination of these sections that are real. Furthermore the bar operation in this case is simply the transposition. Hence, if we consider the so(8) covariant derivative of any of these sections, this is a spinor and, as such, it can be expressed as a linear combinations of the same:
so(8) ζA |
≡ d + Uso(8) ζA |
= UAB ζB |
(9.3.68) |
7 |
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77 7 |
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According to standard lore the one-form valued, antisymmetric 8 × 8 matrix UAB
77
defined by (9.3.68) is the so(8)-connection in the chosen basis of sections. If the manifold M7 admits N Killing spinors, then it follows that we can choose an orthonormal basis where the first N sections are Killing spinors:
ζA = ηA; so(8) ηA = 0, A = 1, . . . , N |
(9.3.69) |
and the remaining 8 − N elements of the basis, whose covariant derivative does not vanish are orthogonal to the Killing spinors:
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so(8) ξ |
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It is then evident from (9.3.69) and (9.3.70) that the so(8)-connection UAB takes
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values only in a subalgebra so(8−N ) so(8) and has the following block diagonal form:
UAB = |
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U |
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AB |
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Squaring the SO(8)-covariant derivative, we find
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UCB ) ζB |
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FAB [ ] |
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Rγ δ αβ − 4e2δγ δ αβ |
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where C γ δ αβ is the so called holonomy tensor, essentially identical with the Weyl tensor of the considered Einstein 7-manifold.
384 |
9 Supergravity: An Anthology of Solutions |
9.3.7 The Holonomy Tensor and Superspace
As a further preparation to our subsequent discussion of the gauge completion let us now consider the form taken on the AdS4 × G /H backgrounds by the operator Kab introduced in (9.3.9) and governing the mechanism of supersymmetry breaking. We will see that it is just simply related to the holonomy tensor discussed in the previous section, namely to the field strength of the SO(8)-connection on the spinor bundle. To begin with, we calculate the operator Fa introduced in (9.3.3), (9.3.5). Explicitly using the well adapted basis (9.3.62) for gamma matrices we find:
Fa = Fa = −2eγa γ5 18
Fα = −e14 τα
Using this input we obtain:
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Kaβ |
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γ δ |
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ab |
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αβ = − |
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R |
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4e |
αβ |
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(9.3.73)
(9.3.74)
Where the tensor Cγ δ αβ defined by the above equation is named the holonomy tensor and it is an intrinsic geometric property of the compact internal manifold M7. As we see the holonomy tensor vanishes only in the case of M7 = S7 when the Riemann tensor is proportional to an antisymmetrized Kronecker delta, namely, when the internal Einstein 7-manifold is maximally symmetric. The holonomy tensor is a 21 × 21 matrix which projects the SO(7) Lie algebra to a subalgebra:
Hhol SO(7) |
(9.3.75) |
with respect to which the 8-component spinor representation should contain singlets in order for unbroken supersymmetries to survive. Indeed the holonomy tensor appears in the integrability condition for Killing spinors. Indeed squaring the defining equation of Killing spinors with m = 1 we get the consistency condition:
Cγ δ αβ τγ δ η = 0 |
(9.3.76) |
which states that the Killing spinor directions are in the kernel of the operators Cγ δ αβ τγ δ , namely are singlets of the subalgebra Hhol generated by them.
In view of this we conclude that the gravitino field strength has the following structure:
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ab |
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ρab = 0 |
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= 0 |
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ρaβ |
(9.3.77) |
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ραβ |
0 |
zero at θ = 0 |
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= ; |
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depends only on the broken θ s |
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9.3 Flux Vacua of M-Theory and Manifolds of Restricted Holonomy |
385 |
Table 9.1 The homogeneous 7-manifolds that admit at least 2 Killing spinors are all Sasakian or tri-Sasakian. This is evident from the fibration structure of the 7-manifold, which is either a fibra-
tion in circles S1 for the N = 2 cases or a fibration in S3 for the unique N = 3 case corresponding to the N 010 manifold
N Name Coset |
Holon. so(8) Fibration |
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bundle |
8 |
S7 |
SO(8) |
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SO(7) |
2 M111 SU(3)×SU(2)×U(1)
SU(2)×U(1)×U(1)
2 Q111 SU(2)×SU(2)×SU(2)×U(1)
U(1)×U(1)×U(1)
2 |
V 5,2 |
SO(5) |
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SO(2) |
3 N 010 SU(3)×SU(2) SU(2)×U(1)
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S7 =3P3 |
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111 |
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Table 9.2 The homogeneous 7-manifolds that admit just one Killing spinors are the squashed 7-sphere and the infinite family of N pqr manifolds for pqr = 010.
N |
Name |
Coset |
Holon. so(8) |
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bundle |
1 |
S7 |
SO(5)×SO(3) |
SO(7)+ |
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squashed |
SO(3)×SO(3) |
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1 |
N pqr |
SU(3)×U(1) |
SO(7)+ |
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U(1)×U(1) |
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As a preparation for our next coming discussion it is now useful to remind the reader that the list of homogeneous 7-manifolds G /H of Englert type which preserve at least two supersymmetries (N ≥ 2) is extremely short. It consists of the Sasakian or tri-Sasakian homogeneous manifolds7 which are displayed in Table 9.1. For these cases our strategy in order to obtain the supergauge completion will be based on a superextension of the Sasakian fibration. The cases with N = 1 are somewhat more involved since such a weapon is not in our stoke. These cases are also ultra-few and they are displayed in Table 9.2.
7The theory of Sasakian manifolds, as applied to supergravity compactifications was discussed in [39]. In short an odd dimensional manifold is named Sasakian if the even dimensional cone constructed over it has vanishing first Chern class. After several manipulations this implies that the Sasakian manifold is an S1-fibre bundle over a suitable complex base manifold.