
- •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
422 |
10 Conclusion of Volume 2 |
As it is always the case, the Maurer Cartan equations are just a property of the (super) Lie algebra and hold true independently of the (super) manifold on which the 1-forms are realized: on the supergroup manifold or on different supercosets of the same supergroup.
C.2 The Relevant Supercosets and Their Relation
Let us also consider the following pure fermionic coset:
M 0|4N |
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Osp(N |4) |
(C.2.1) |
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osp |
= SO( |
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× |
Sp(4, R) |
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N |
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There is an obvious relation between these two supercosets that can be formulated in the following way:
Mosp4|4N AdS4 × Mosp0|4N |
(C.2.2) |
In order to explain the actual meaning of (C.2.2) we proceed as follows. Let the graded matrix L Osp(N |4) be the coset representative of the coset Mosp4|4N , such that the Maurer Cartan form Λ of (C.1.5) can be identified as:
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Λ = L−1 dL |
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(C.2.3) |
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Let us now factorize L as follows: |
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L = LF LB |
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(C.2.4) |
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where LF is a coset representative for the coset: |
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Osp(N |4) |
# |
L |
F |
(C.2.5) |
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SO( |
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× |
Sp(4, R) |
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N |
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and LB is the Osp(N |4) embedding of a coset representative of AdS4, namely:
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LB |
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Sp(4, R) |
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LB = |
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0 |
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# LB |
(C.2.6) |
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1N |
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SO(1, 3) |
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In this way we find: |
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Λ |
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L−1 |
Λ |
F |
L |
B + |
L−1 dL |
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(C.2.7) |
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B |
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B |
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Let us now write the explicit form of ΛF in analogy to (C.1.5):
ΛF = |
2 |
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ΘA |
3 |
(C.2.8) |
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−eAAB |
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4ieΘAγ5 |
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C Auxiliary Information About Some Superalgebras |
423 |
where ΘA is a Majorana-spinor valued fermionic 1-form and where |
F is an |
sp(4, R) Lie algebra valued 1-form presented as a 4 × 4 matrix. Both ΘA as F and AAB depend only on the fermionic θ coordinates and differentials.
On the other hand we have: |
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LB−1 dLB = |
0B |
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(C.2.9) |
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where the ΩB is also an sp(4, R) Lie algebra valued 1-form presented as a 4 × 4 matrix, but it depends only on the bosonic coordinates xμ of the anti de Sitter space AdS4. Indeed, according to (C.1.5) we can write:
B = − |
1 |
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4 Babγab − 2eγa γ5Ba |
(C.2.10) |
where {Bab, Ba } are respectively the spin-connection and the vielbein of AdS4, just as {Bαβ , Bα } are the connection and vielbein of the internal coset manifold M7.
Inserting now these results into (C.2.7) and comparing with (C.1.5) we obtain:
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ψA = LB−1ΘA |
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AAB = AAB |
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(C.2.11) |
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− |
ωabγ |
ab − |
2eγ |
γ |
Ea |
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Babγ |
ab − |
2eγ |
γ |
Ba |
+ |
L−1 |
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The above formulae encode an important information. They show how the supervielbein and the superconnection of the supermanifold (C.1.9) can be constructed starting from the vielbein and connection of AdS4 space plus the Maurer Cartan forms of the purely fermionic supercoset (C.2.1). In other words formulae (C.2.11) provide the concrete interpretation of the direct product (C.2.2). This will also be our starting point for the actual construction of the supergauge completion in the case of maximal supersymmetry and for its generalization to the cases of less supersymmetry.
C.2.1 Finite Supergroup Elements
We studied the osp(N |4) superalgebra but for our purposes we cannot confine ourselves to the superalgebra, we need also to consider finite elements of the corresponding supergroup. In particular the supercoset representative. Elements of the supergroup are described by graded matrices of the form:
M = |
A |
Θ |
(C.2.12) |
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Π |
D |
where A, D are submatrices made out of even elements of a Grassmann algebra while Θ, Π are submatrices made out of odd elements of the same Grassmann algebra. It is important to recall, that the operations of transposition and Hermitian

424 |
10 Conclusion of Volume 2 |
conjugation are defined as follows on graded matrices:
MT = |
2 |
ATT |
ΠT |
3 |
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T |
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−Θ |
D |
(C.2.13) |
2 3
M† =
A† Π †
Θ† D†
This is done in order that the supertrace should preserve the same formal properties enjoyed by the trace of ordinary matrices:
Str(M) = Tr(A) − Tr(D)
(C.2.14)
Str(M1M2) = Str(M2M1)
Equations (C.2.13) and (C.2.14) have an important consequence. The consistency of the equation:
M† = MT |
(C.2.15) |
implies that the complex conjugate operation on a super matrix must be defined as follows:
M |
= |
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A |
−Θ |
(C.2.16) |
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Π |
D |
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Let us now observe that in the Majorana basis which we have adopted we have:
C |
= |
i |
2 |
ε |
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iε |
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7 |
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iε |
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where the 4 × 4 matrix ε is given by (C.3.7). Therefore in this basis an orthosymplectic group element L OSp(N |4) which satisfies:
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LT CL = C |
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7 |
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7 |
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L†H L |
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H |
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(C.2.19) |
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has the following structure: |
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= 7 |
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= |
2 |
S |
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exp[−i π4 ]Θ |
3 |
(C.2.20) |
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exp[−i π4 ]Π |
O |
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where the bosonic sub-blocks S , O are respectively 4 × 4 and N × N and real, while the fermionic ones Θ, Π are respectively 4 × N and N × 4 and also real.
The orthosymplectic conditions (C.2.18) translate into the following conditions on the sub-blocks:

C Auxiliary Information About Some Superalgebras |
425 |
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1 |
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S T εS = ε − i 4e Π T Π |
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OT O = 1 + i4eΘT εΘ |
(C.2.21) |
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1 |
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S T εΘ = − |
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Π T O |
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4e |
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As we see, when the fermionic off-diagonal sub-blocks are zero the diagonal ones are respectively a symplectic and an orthogonal matrix.
If the graded matrix L is regarded as the coset representative of either one of the two supercosets (C.1.9), (C.2.1), we can evaluate the explicit structure of the left-invariant one form Λ. Using the M 0|4×N style of the Maurer Cartan equations (C.1.10) we obtain:
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− |
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= |
−4e exp[−i π4 ]ΦT ε |
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−eA |
]Φ |
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Λ |
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L |
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1 dL |
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exp[−i π4 |
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(C.2.22) |
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where the 1-forms |
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of the inverse coset representative: |
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− |
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π |
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[− |
T |
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3 |
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1 |
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−εS T ε |
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exp i π4 |
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1 |
εΠ T |
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L |
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4e |
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(C.2.23) |
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− exp[−i 4 ]4eΘ |
ε |
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eA = −OT dO − i4eΘT ε dΘ |
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Ω = −εS T ε dS − i |
1 |
Π T dΠ |
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(C.2.24) |
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4e |
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Φ = −εST ε dΘ + |
1 |
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C.2.2 The Coset Representative of OSp(N |4)/SO(N ) × Sp(4)
It is fairly simple to write an explicit form for the coset representative of the fermionic supermanifold
M 0|4×N |
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OSp(N |4) |
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(C.2.25) |
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N |
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= Sp(4, R) |
× |
SO( |
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by adopting the upper left block components Θ of the supermatrix (C.2.20) as coordinates. It suffices to solve (C.2.21) for the sub blocks S , O , Π . Such an explicit solution is provided by setting:
O(Θ) = 1 + 4ieΘT εΘ 1/2
S (Θ) = 1 + 4ieΘΘT ε 1/2
(C.2.26)
Π= 4e 1 + 4ieΘT εΘ −1/2ΘT ε 1 + 4ieΘΘT ε 1/2
= 4eΘT ε
426 |
10 Conclusion of Volume 2 |
In this way we conclude that the coset representative of the fermionic supermanifold (C.2.25) can be chosen to be the following supermatrix:
L(Θ) = |
2 |
(1 + 4i |
π |
|
T |
|
exp[−iT4 |
]Θ |
1/2 |
3 |
(C.2.27) |
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eΘΘT ε)1/2 |
π |
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− exp[−i 4 |
]4eΘ |
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ε |
(1 + 4ieΘ εΘ) |
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By straightforward steps from (C.2.23) we obtain the inverse of the supercoset element (C.2.27) in the form:
|
− |
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(Θ) |
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( Θ) |
2 |
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+ |
π |
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T |
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− |
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T |
1/2 |
3 |
(C.2.28) |
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L |
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1 |
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= |
L |
− |
= |
(1 |
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4ieΘΘT ε)1/2 |
|
exp[−i π4 |
]Θ |
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− exp[−i 4 |
]4eΘ |
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ε |
(1 + 4ieΘ |
εΘ) |
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Correspondingly we work out the explicit expression of the Maurer Cartan forms:
eA = 1 + 4ieΘT εΘ 1/2 d 1 + 4ieΘT εΘ 1/2 − i4eΘT ε dΘ |
|
Φ = 1 + 4ieΘΘT ε 1/2 dΘ + Θ d 1 + 4ieΘT εΘ 1/2 |
(C.2.29) |
= 1 + 4ieΘΘT ε 1/2 d 1 + 4ieΘΘT ε 1/2 − i4eΘ dΘT ε |
|
C.3 D = 6 and D = 4 Gamma Matrix Bases
In the discussion of the AdS4 × P3 compactification we need to consider the decomposition of the D = 10 gamma matrix algebra into the tensor product of the so(6) Clifford algebra times that of so(1, 3). In this section we discuss an explicit basis for the so(6) gamma matrix algebra using that of so(7). Conventionally we identify the 7-matrix τ7 with the chirality matrix in d = 6.
C.3.1 D = 6 Clifford Algebra
In this section, the indices α, β, . . . run on six values and denote the vector indices of so(6). In order to discuss the gamma matrix basis we introduce so(7) indices
|
= α, 7 |
(C.3.1) |
α |
which run on seven values and we define the Clifford algebra with negative metric:
{τ |
|
, τ |
|
} = −δ |
|
(C.3.2) |
α |
β |
αβ |
C Auxiliary Information About Some Superalgebras |
427 |
This algebra is satisfied by the following, real, antisymmetric matrices:
τ1
τ3
τ5
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0 0 |
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0 |
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−1 0 |
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1 |
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τ2
τ4
τ6
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0 0 0 0 −1 0 |
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(C.3.3) |
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0 0 |
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0 0 0 0 |
−1 |
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0 |
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0 |
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1 |
0 |
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τ7 |
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− |
1 |
0 |
0 |
0 |
0 |
0 |
0 |
0 |
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1 |
0 |
0 |
0 |
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C.3.2 D = 4 γ -Matrix Basis and Spinor Identities
In this section we construct a basis of so(1, 3) realizes the isomorphism so(2, 3) sp(4, R) text. Naming σi the standard Pauli matrices:
gamma matrices such that it explicitly with the conventions used in the main
|
= |
1 |
0 |
; |
|
= |
i |
0 |
; |
|
= |
0 |
|
1 |
|
σ1 |
|
0 |
1 |
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σ2 |
|
0 |
−i |
|
σ3 |
|
1 |
0 |
(C.3.4) |
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− |
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428 |
10 Conclusion of Volume 2 |
|
we realize the so(1, 3) Clifford algebra: |
|
|
{γa , γb} = 2ηab; |
ηab = diag(+, −, −, −) |
(C.3.5) |
by setting: |
|
|
γ0 = σ2 1; |
γ1 = iσ3 σ1 |
|
γ2 = iσ1 1; |
γ3 = iσ3 σ3 |
(C.3.6) |
γ5 = σ3 σ2; C = iσ2 1
where γ5 is the chirality matrix and C is the charge conjugation matrix. Making now reference to (C.1.2) and (C.1.3) of the main text we see that the antisymmetric matrix entering the definition of the orthosymplectic algebra, namely C γ5 is the following one:
C |
i |
0 |
0 |
0 |
1 |
, |
C γ5 ε |
i |
0 |
0 |
−1 |
0 |
(C.3.7) |
||
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0 |
0 |
1 |
0 |
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0 |
0 |
0 |
1 |
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= |
−1 |
0 |
0 |
0 |
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= = |
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0 |
1 |
0 |
0 |
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0 |
− |
1 0 |
0 |
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1 0 |
0 |
0 |
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− |
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namely it is proportional, through an overall i-factor, to a real completely offdiagonal matrix. On the other hand all the generators of the so(2, 3) Lie algebra, i.e. γab and γa γ5 are real, symplectic 4 × 4 matrices. Indeed we have
γ01 |
0 |
|
0 |
−1 |
|
0 |
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γ02 |
0 1 |
0 |
0 |
|||||||
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0 |
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0 |
0 |
−1 |
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1 |
0 |
0 |
0 |
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|||||
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= |
0 |
− |
1 |
0 |
|
0 |
|
; |
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= 0 0 −1 |
0 |
|||||||
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1 |
0 |
0 |
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0 |
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0 0 |
0 |
1 |
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− |
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− |
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γ12 |
0 |
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0 |
0 |
1 |
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γ13 |
0 0 −1 |
0 |
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||||||||
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0 |
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0 |
−1 |
0 |
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0 |
0 |
0 |
−1 |
||||||
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= −1 |
|
0 |
0 |
0 |
; |
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= 0 1 |
0 |
0 |
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0 |
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1 |
0 |
0 |
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1 0 |
0 |
0 |
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γ23 |
−1 |
|
0 |
0 |
0 |
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γ34 |
|
0 |
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0 |
0 |
−1 (C.3.8) |
|||||
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0 |
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1 |
0 |
0 |
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0 |
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0 |
1 |
0 |
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= |
0 |
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0 |
0 |
1 |
; |
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= −1 |
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0 0 |
0 |
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0 |
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0 |
− |
1 |
0 |
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1 0 |
0 |
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γ0γ5 |
0 |
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0 |
−1 |
0 |
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γ1γ5 |
0 |
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1 |
0 |
0 |
||||||
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= |
0 |
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0 |
0 |
1 |
; |
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= |
−1 |
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0 |
0 |
0 |
||||
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0 |
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1 |
0 |
0 |
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0 |
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0 −1 |
0 |
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1 0 |
0 |
0 |
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1 |
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1 0 0 0 |
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0 |
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−1 |
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0 |
1 |
0 |
0 |
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γ2γ5 |
= |
0 |
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1 |
0 |
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0 |
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; |
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γ3γ5 |
= 0 0 0 1 |
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1 0 |
0 |
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0 |
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0 0 1 0 |
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