- •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
246 |
6 Supergravity: The Principles |
supersymmetry algebra. The answer is easily obtained arguing in terms of highest vectors. Consider the highest helicity state of the graviton:
|Ω! = |2, 0, 0, 0! |
(6.5.15) |
and let us assume that it is the highest state of the entire supermultiplet. This means that it is annihilated by all supercharges that are creation operators, namely:
q( 21 ,± 21 ,± 12 ,± 12 )|2, 0, 0, 0! = 0 |
(6.5.16) |
A non-vanishing result is obtained applying to |2, 0, 0, 0! products of the operators
q(− 21 ,± 12 ,± 12 ,± 21 ), where all factors in the product are different. So we find: |
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2 1 |
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Applying the destruction operators to all other positive weights of the spin two representation we find that the set of weights we can construct is just the union of the weights belonging to the three mentioned irreducible representations. Hence the D = 11 supermultiplet is indeed constituted by the fields mentioned in Table 6.2.
6.6 Summary of Supergravities
Having clarified the construction principles of supergravities and their fundamental algebraic basis, rooted in the Free Differential Algebra structure we pass to a scan of the available theories.
In D = 11 there is just a unique supergravity, M-theory, whose structure we have thoroughly discussed.
In D = 10 we have just five different supergravities, displayed in Fig. 6.12 which are in one-to-one correspondence with the available consistent superstring theories. Actually, from the supergravity viewpoint there are only three possible theories in D = 10. The type II theories that have two Majorana-Weyl supercharges (A and B, according to the choice of their chirality, as we explain below) and the type I theory that has only one Majorana-Weyl supercharge and can be coupled to a vector multiplet. The different choice of the gauge group is the only distinction among type
6.6 Summary of Supergravities |
247 |
Fig. 6.12 The field content of the five D = 10 supergravities. The fields of each of these theories are the massless modes of the corresponding superstring theory. The bosonic fields are organized according to their string origin in the NS-NS or R-R sector, while the fermionic fields are organized according to their chirality
I theories. However a very complex mechanism displayed by these latter resides in the possibility of introducing their coupling to gauge and Lorentz Chern-Simons three-forms: this provides the cancellation of anomalies and selects the three models that complete the list of consistent superstring theories. In this book we do not dwell on D = 10, N = 1 supergravities and on their Lorentz Chern-Simons coupling for which we refer the reader to the book [28]. We rather focus on type II theories of which we give a complete account.
The key point in D = 10 is the existence of Majorana-Weyl spinors satisfying the double condition:
ψL/R = C |
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L/RT ; |
Γ11ψL/R = ±ψL/R |
(6.6.1) |
ψ |
where C is the charge conjugation matrix and Γ11 is the chirality matrix (see Appendix A.4 for details). The type IIA theory is based on the super-Poincaré Lie algebra containing two Majorana-Weyl supercharges, one QL which is left-handed, the other QR which is right-handed. The type IIB theory is instead based on the superPoincaré Lie algebra that contains two Majorana-Weyl supercharges, QAL (A = 1, 2) of the same chirality, say left-handed. The presence of this doublet of chiral supercharges introduces an SL(2, R) symmetry which is an essential item in the construction of the whole theory.
In dimensions D < 10 the number of available supergravity theories starts growing because we can reduce the number of supercharges and introduce an increasing available choice of matter supermultiplets. As soon as scalar fields appear in the
248 |
6 Supergravity: The Principles |
spectrum they introduce a new quality: the scalars can be regarded as the coordinates of a differentiable target manifold for whose geometry supersymmetry selects a variety of special structures. Chapter 8 presents a bird-eye review of supergravity geometries and couplings.
Chapter 7 is instead devoted to enlighten the vital dualism between the bulk and the brane world-volume perspectives. For that we shall need the explicit structure of the type II theories which we present in the next two sections.
6.7 Type IIA Supergravity in D = 10
The full-fledged rheonomic construction of type IIA supergravity was obtained only recently in [29] which we follow in the present section. The field content of the theory is given in Table 6.3.
This field content corresponds to the basic forms of a specific Free Differential Algebra including the 0-form items entering the rheonomic parameterizations of its curvatures.
The starting point is, as usual, the super-Poincaré algebra. In D = 10 we have two super-Poincaré algebras with 32 supercharges, the type IIA and the type IIB. If we also include the dilaton, as we will do, there are various equivalent definitions of curvatures that are named frames and differ by dilaton pre-factors. The Einstein frame is that which leads to an action where the Einstein kinetic term is canonical without any dilaton pre-factors. The string frame, which has distinguished advantages when writing the string action in its background, corresponds instead to non-canonical Einstein terms in the action. The two frames are just related by a suitable Weyl transformation depending on the dilaton. For type IIA supergravity we use the string frames for two reasons. The first is that in this frame the FDA has a simpler and more elegant form. The second is pedagogical. We want to emphasize the freedom of using different but equivalent frames. For type IIB supergravity we will rather use the Einstein frame in which the SL(2, R) symmetry of that theory is manifest.
The Maurer Cartan description of the type IIA superalgebra is obtained by setting to zero the following curvatures:
Table 6.3 Structure of the graviton multiplet in Type IIA supergravity
SO(1, 9) rep. |
# of states |
Name |
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(2, 0, 0, 0, 0) |
35 |
graviton |
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( 32 |
, 21 , |
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, 21 )L |
56 |
left gravitino |
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1 )R |
56 |
right gravitino |
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28 |
NS B-field |
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RR 1-form |
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(1, 1, 1, 0, 0) |
56 |
RR 3-form |
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( 12 |
, 21 , |
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, 21 )L |
8 |
left dilatino |
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right dilatino |
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dilaton |
6.7 Type IIA Supergravity in D = 10 |
249 |
Type IIA Super-Poicaré Algebra in the String Frame
Rab ≡ dωab − ωac ωcb |
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where the 0-form dilaton ϕ appearing in (6.7.4) introduces a mobile coupling constant. Furthermore, V a , ωab denote the vielbein and the spin connection 1-forms, respectively, while the two fermionic 1-forms ψL/R are Majorana-Weyl spinors of opposite chirality:
Γ11ψL/R = ±ψL/R |
(6.7.7) |
The flat metric ηab = diag(+, −, . . . , −) is the mostly minus one and Γ11 is Hermitian and squares to the identity Γ112 = 1.
Setting Rab = T a = G[2] = f[1] = 0 one obtains the Maurer Cartan equations of a superalgebra where the spinor charges, QL,R dual to the spinor 1-forms ψL,R not only anticommute to the translations Pa but also to a central charge Z dual to the (Ramond Ramond) 1-form C[1].
According to Sullivan’s second theorem the FDA extension of the above superalgebra is dictated by its cohomology. In a first step one finds that there exists a cohomology class of degree three which motivates the introduction of a new 2-form generator B[2] which in the superstring interpretation is just the Kalb-Ramond field. Considering then the cohomology of the FDA-extended algebra one finds a degree four cohomology class which motivates the introduction of a 3-form generator C[3]. In the superstring interpretation, this is just the second R-R field, the first being the gauge field C[1]. Altogether the complete type IIA FDA is obtained by adjoining the following curvatures to those already introduced:
The FDA Extension of the Type IIA Superalgebra in the String Frame |
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Equations (6.7.1)–(6.7.5) together with (6.7.8)–(6.7.9) provide the complete definition of the type IIA Free Differential Algebra.