
- •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
338 |
8 Supergravity: A Bestiary in Diverse Dimensions |
to obtain a parameterization of the section X in terms of coordinates σ, φ of the manifold SO(1, 1) × SO(1, n)/SO(2) × SO(n). This achieves the desired proof that the group Giso has a transitive action on the special manifold and consequently that the cubic norm (8.6.37), (8.6.38) is admissible as a definition of a very special manifold.
8.6.3 Quaternionic Geometry
Next we turn our attention to the hypermultiplet sector of an N = 2 supergravity. For these multiplets no distinction arises between the D = 4 and D = 5. Each hypermultiplet contains 4 real scalar fields and, at least locally, they can be regarded as the four components of a quaternion. The locality caveat is, in this case, very substantial because global quaternionic coordinates can be constructed only occasionally even on those manifolds that are denominated quaternionic in the mathematical literature [6, 17]. Anyhow, what is important is that, in the hypermultiplet sector, the scalar manifold QM has dimension multiple of four:
dimR QM = 4m ≡ 4 # of hypermultiplets |
(8.6.48) |
and, in some appropriate sense, it has a quaternionic structure.
We name Hypergeometry that pertaining to the hypermultiplet sector, irrespectively whether we deal with global or local N = 2 theories. Yet there are two kinds of hypergeometries. Supersymmetry requires the existence of a principal SU(2)- bundle
S U −→ QM |
(8.6.49) |
The bundle S U is flat in the rigid supersymmetry case while its curvature is proportional to the Kähler forms in the local case.
These two versions of hypergeometry were already known in mathematics prior to their use [14, 18–20, 22, 23] in the context of N = 2 supersymmetry and are identified as:
rigid hypergeometry ≡ HyperKähler geometry
(8.6.50)
local hypergeometry ≡ quaternionic geometry
8.6.4 Quaternionic, Versus HyperKähler Manifolds
Both a quaternionic or a HyperKähler manifold QM is a 4m-dimensional real manifold endowed with a metric h:
ds2 = huv (q) dqu dqv ; u, v = 1, . . . , 4m |
(8.6.51) |
and three complex structures
J x : T (QM ) −→ T (QM ) (x = 1, 2, 3) |
(8.6.52) |
8.6 Supergravities in Five Dimension and More Scalar Geometries |
339 |
that satisfy the quaternionic algebra
J x J y = −δxy 1 + εxyzJ z |
(8.6.53) |
and respect to which the metric is Hermitian:
X, Y T QM : h J x X, J x Y = h(X, Y) (x = 1, 2, 3) |
(8.6.54) |
From (8.6.54) it follows that one can introduce a triplet of 2-forms
Kx = Kuvx dqu dqv ; Kuvx = huw(J x )vw |
(8.6.55) |
that provides the generalization of the concept of Kähler form occurring in the complex case. The triplet Kx is named the HyperKähler form. It is an SU(2) Lie-algebra valued 2-form in the same way as the Kähler form is a U(1) Lie-algebra valued 2- form. In the complex case the definition of Kähler manifold involves the statement that the Kähler 2-form is closed. At the same time in Hodge-Kähler manifolds (those appropriate to local supersymmetry in D = 4) the Kähler 2-form can be identified with the curvature of a line-bundle which in the case of rigid supersymmetry is flat. Similar steps can be taken also here and lead to two possibilities: either HyperKähler or quaternionic manifolds.
Let us introduce a principal SU(2)-bundle S U as defined in (8.6.49). Let ωx denote a connection on such a bundle. To obtain either a HyperKähler or a quaternionic manifold we must impose the condition that the HyperKähler 2-form is covariantly closed with respect to the connection ωx :
Kx ≡ dKx + εxyzωy Kz = 0 |
(8.6.56) |
The only difference between the two kinds of geometries resides in the structure of the S U -bundle.
Definition 8.6.1 A HyperKähler manifold structure described above and such that the
is a 4m-dimensional manifold with the S U -bundle is flat.
Defining the S U -curvature by: |
|
|
|
Ωx ≡ dωx + |
1 |
εxyzωy ωz |
(8.6.57) |
|
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2 |
|||
in the HyperKähler case we have: |
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|
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Ωx = 0 |
(8.6.58) |
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Vice-versa |
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Definition 8.6.2 A quaternionic manifold is a 4m-dimensional manifold with the structure described above and such that the curvature of the S U -bundle is proportional to the HyperKähler 2-form.
340 |
8 Supergravity: A Bestiary in Diverse Dimensions |
Hence, in the quaternionic case we can write:
Ωx = λKx |
(8.6.59) |
where λ is a non-vanishing real number.
As a consequence of the above structure the manifold QM has a holonomy group of the following type:
Hol(QM ) = SU(2) H |
(quaternionic) |
Hol(QM ) = 1 H (HyperKähler) |
|
H Sp(2m, R) |
(8.6.60) |
In both cases, introducing flat indices {A, B, C = 1, 2}{α, β, γ = 1, . . . , 2m} that run, respectively, in the fundamental representation of SU(2) and of Sp(2m, R), we can find a vielbein 1-form
U Aα = UuAα (q) dqu |
(8.6.61) |
such that |
|
huv = UuAα UvBβ Cαβ εAB |
(8.6.62) |
where Cαβ = −Cβα and εAB = −εBA are, respectively, the flat Sp(2m) and Sp(2) SU(2) invariant metrics. The vielbein U Aα is covariantly closed with respect to
the SU(2)-connection ωz and to some Sp(2m, R)-Lie Algebra valued connection
αβ = βα :
U Aα ≡ dU Aα + |
|
i |
ωx εσx ε−1 AB U Bα + αβ U Aγ Cβγ = 0 |
(8.6.63) |
|
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|
||||
2 |
|||||
where (σ x ) |
B are the standard Pauli matrices. Furthermore U Aα satisfies the reality |
||||
condition: |
A |
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|
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UAα ≡ U Aα = εAB Cαβ U Bβ |
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(8.6.64) |
Equation (8.6.64) defines the rule to lower the symplectic indices by means of the flat symplectic metrics εAB and Cαβ . More specifically we can write a stronger version of (8.6.62) [24]:
UuAα UvBβ + UvAα UuBβ Cαβ = huv εAB
We have also the inverse vielbein UAαu defined by the equation
UAαu UvAα = δvu
Flattening a pair of indices of the Riemann tensor Ruvts we obtain
|
uv |
αA |
βB |
|
i |
x |
|
AC |
B |
|
αβ |
αβ |
|
AB |
R |
ts |
Uu |
Uv |
= − |
|
Ωts |
ε |
|
(σx )C |
C |
|
+ Rts |
ε |
|
2 |
|
|
|
(8.6.65)
(8.6.66)
(8.6.67)

8.6 Supergravities in Five Dimension and More Scalar Geometries |
|
341 |
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Table 8.3 Homogeneous |
m |
G/H |
m |
G/H |
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symmetric quaternionic |
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manifolds |
m |
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Sp(2m+2) |
2 |
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G2 |
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Sp(2)×Sp(2m) |
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SO(4) |
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m |
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SU(m,2) |
|
7 |
|
F4 |
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SU(m)×SU(2)×U(1) |
Sp(6)×Sp(2) |
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m |
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SO(4,m) |
|
10 |
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E6 |
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SO(4)×SO(m) |
SU(6)×U(1) |
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16 |
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E7 |
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SO(12)×SU(2) |
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28 |
|
E8 |
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E7×SU(2) |
|||||||
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|
where Rαβ |
is the field strength of the Sp(2m) connection: |
|
ts |
|
|
|
dΔαβ + αγ δβ Cγ δ ≡ Rαβ = Rtαβs dqt dqs |
(8.6.68) |
Equation (8.6.67) is the explicit statement that the Levi Civita connection associated with the metric h has a holonomy group contained in SU(2) Sp(2m). Consider now (8.6.53), (8.6.55) and (8.6.59). We easily deduce the following relation:
hst Kusx Ktyw = −δxy huw + εxyzKuwz |
(8.6.69) |
that holds true both in the HyperKähler and in the quaternionic case. In the latter case, using (8.6.59), (8.6.69) can be rewritten as follows:
hst Ωusx Ωtyw = −λ2δxy huw + λεxyzΩuwz |
(8.6.70) |
Equation (8.6.70) implies that the intrinsic components of the curvature 2-form Ωx yield a representation of the quaternion algebra. In the HyperKähler case such a representation is provided only by the HyperKähler form. In the quaternionic case we can write:
ΩAα,Bβx ≡ Ωuvx UAαu UBβv = −iλCαβ (σx )AC εCB |
(8.6.71) |
||
Alternatively (8.6.71) can be rewritten in an intrinsic form as |
|
||
Ωx = −iλCαβ (σx )AC εCB U αA U βB |
(8.6.72) |
||
whence we also get: |
|
|
|
|
i |
Ωx (σx )AB = λUAα U Bα |
(8.6.73) |
|
|
||
2 |
The quaternionic manifolds are not requested to be homogeneous spaces, however there exists a subclass of quaternionic homogeneous spaces that are displayed in Table 8.3.