
- •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

310 |
|
8 Supergravity: A Bestiary in Diverse Dimensions |
|
Table 8.2 Scalar geometries in maximal supergravities |
|
||
|
|
|
|
D = 9 |
E2(2) ≡ SL(2, R) O(1, 1) |
H = O(2) |
dimR(G/H) = 3 |
D = 8 |
E3(3) ≡ SL(3, R) SL(2, R) |
H = O(2) O(3) |
dimR(G/H) = 7 |
D = 7 |
E4(4) ≡ SL(5, R) |
H = O(5) |
dimR(G/H) = 14 |
D = 6 |
E5(5) ≡ O(5, 5) |
H = O(5) O(5) |
dimR(G/H) = 25 |
D = 5 |
E6(6) |
H = Usp(8) |
dimR(G/H) = 42 |
D = 4 |
E7(7) |
H = SU(8) |
dimR(G/H) = 70 |
D = 3 |
E8(8) |
H = O(16) |
dimR(G/H) = 128 |
persymmetry allows for unique maximal theories in D ≤ 9 and there is just one scalar coset manifold, that listed in Table 8.2. Yet this result can be interpreted in two ways depending on whether we look at it from the type IIA or from the type IIB viewpoint. There is indeed a challenging problem that corresponds to retrieving the steps of the two possible chains of sequential toroidal compactifications within the algebraic structure of the isometry groups Gx and identifying which scalar field appears at which step of the sequential chain. Such a problem has a very elegant and instructive solution in terms of a rather simple and classical mathematical theory, namely the solvable Lie algebra parameterization of non-compact cosets. This mathematical theory that makes a perfect match with the string theory origin of supergravities plays an important role in the discussion of p-brane solutions. In the Solvable Lie algebra parameterizations the scalar fields are divided into two groups, those that are associated with Cartan generators of the solvable algebra and those that are associated with nilpotent generators. The Cartan scalars are those that play the role of generalized dilatons and couple to the field strength (p + 2)-forms as in (7.7.1). Within the algebraic approach, the a parameters appearing in the couplings of type exp[−aφ]|F [p+2]|2 have an interpretation in terms of roots and weights of the Gx Lie algebras which provides a very important insight into the whole matter. The solvable Lie algebra approach, that in maximal supergravities helps so clearly to master the string theory origin of the cosets G/H, can be extended also to the scalar manifolds of theories with a lesser number of supercharges. Indeed, from a mathematical point of view it works for all non-compact cosets.
8.3 Duality Symmetries in Even Dimensions
Generically a p-brane in D-dimensions either carries an electric charge with respect to a (p + 1)-form gauge field A[p+1] or a magnetic charge with respect to the dual
|
|
|
|
[D−p−3] |
. In the general case it cannot be dyonic with respect to |
|||
(D − p − 3)-form Adual |
||||||||
the same gauge field since |
|
|
|
|
||||
|
|
|
|
|
|
p + 1 = D − p − 3 |
(8.3.1) |
|
However, in |
even dimension D |
= |
2r, the Diophantine equation (8.3.1) admits one |
|||||
D 4 |
|
|
|
|
||||
|
= |
2 |
|
|
|
|
|
|
solution p |
|
− |
, so that we always have, in this case, a special instance of branes |

8.3 Duality Symmetries in Even Dimensions |
311 |
which can be dyonic: they are particles or 0-branes in D = 4, strings or 1-branes in D = 6 and 2-branes in D = 8. The possible presence of such dyonic objects has profound implications on the structure of the even dimensional supergravity Lagrangians. Indeed most of the dualities, T , S and U that relate the five perturbative superstrings have a non-trivial action on p-branes and generically transform them as electric-magnetic duality rotations. Hence, when self-dual (r − 1)-forms are available, string dualities reflect into duality symmetries of the supergravity Lagrangians which constitute an essential ingredient in their construction. By duality symmetry we mean the following: a certain group of transformations Gdual acts on the set of field equations of supergravity plus the Bianchi identities of the (r − 1)-forms mapping this set into itself. Clearly Gdual acts also on the scalar fields φI and in order to be a symmetry it must respect their kinetic term gI J (φ)∂μφI ∂μφJ . This happens if and only if Gdual is a group of isometries for the scalar metric gI J (φ). In other words string dualities are encoded in the isometry group of the scalar manifold of supergravity which is lifted to act as a group of electric-magnetic duality rotations on the (r − 1)-forms.
The request that these duality symmetries do exist determines the general form of the supergravity Lagrangian and is a key ingredient in its construction. For this reason in the present section we consider the case of even dimensions D = 2r and we review the general structure of an Abelian theory containing n differential (r −
1)-forms: |
|
AΛ ≡ AμΛ1...μr−1 dxμ1 · · · dxμr−1 ; (Λ = 1, . . . , n) |
(8.3.2) |
and m real scalar fields φI . The field strengths of the (r − 1)-forms and their Hodge duals are defined as follows:
|
|
|
|
|
1 |
|
|
|
|
|
F Λ ≡ dAΛ ≡ |
|
FμΛ1...μr dxμ1 · · · dxμr |
|
|||||
|
r! |
|
|||||||
|
|
1 |
FμΛ1...μr |
dxμ1 · · · dxμr |
|
||||
F Λ ≡ |
|
|
|||||||
r! |
(8.3.3) |
||||||||
FμΛ1 |
...μr |
≡ ∂μ1 AμΛ2...μr |
+ r − 2 terms |
|
|||||
|
|
1 |
εμ1...μr ν1...νr F Λ|ν1...νr |
|
|||||
FμΛ1 |
...μr |
≡ |
|
|
|
||||
r |
! |
|
|||||||
|
|
|
|
|
|
|
|
|
Defining the space-time integration volume as:
|
dD x ≡ |
1 |
εμ1...μD dxμ1 |
· · · dxμD |
(8.3.4) |
||||||
we obtain: |
D! |
||||||||||
|
|
|
|
|
|
|
|
|
|
|
|
F Λ F Σ |
|
1 |
εμ1...μr ν1...νr FμΛ1...μr FνΣ1...νr |
|
|||||||
= |
|
|
|||||||||
(r )2 |
(8.3.5) |
||||||||||
|
|
|
|
! |
1 |
|
|
|
|||
F Λ |
|
F Σ |
|
( )r |
|
F Λ |
F Σ|μ1...μr |
|
|||
|
|
|
= − |
(r |
) |
μ1...μr |
|
||||
|
|
|
|
|
|
|
! |
|
|
|
|

312 |
8 Supergravity: A Bestiary in Diverse Dimensions |
The real scalar fields φI span an m-dimensional manifold Mscalar7 endowed with a metric gI J (φ). Utilizing the above field content we can write the following action functional:
S = Stens + Sscal |
|
|
|
|
|
|
|
|
|
|
|
|
||||
Stens = |
(−)r |
γ |
|
(φ)F Λ |
|
F |
Σ |
+ |
1 |
θ |
|
(φ)F Λ |
|
F Σ |
||
|
|
|
|
|
|
|||||||||||
2 |
|
|
2 |
|
||||||||||||
|
ΛΣ |
|
|
|
|
ΛΣ |
|
|
||||||||
Sscal = |
2 gI J (φ)∂μφI ∂μ |
φJ dD x |
|
|
|
|
|
|
(8.3.6) |
|||||||
|
1 |
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
where the scalar field dependent n × n matrix γΛΣ (φ) generalizes the inverse of the squared coupling constant g12 appearing in ordinary 4D-gauge theories. The field dependent matrix θΛΣ (φ) is instead a generalization of the θ -angle of quantum chromodynamics. The matrix γ is symmetric in every space-time dimension, while θ is symmetric or antisymmetric depending on whether r = D/2 is an even or odd number. In view of this fact it is convenient to distinguish the two cases, setting:
D |
4ν |
|
ν Z | r = 2ν |
(8.3.7) |
||
|
= |
+ 2 |
ν |
Z |
| r = 2ν |
+ 1 |
|
4ν |
|
Introducing a formal operator j that maps a field strength into its Hodge dual:
j F Λ μ1 μr ≡... |
1 |
εμ1 μr ν1 νr F Λ|ν1... ... ... |
νr |
||||
(r!) |
|||||||
and a formal scalar product: |
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
1 |
|
|
n |
|
||
(G, K) ≡ GT K ≡ |
|
GμΛ1...μr KΛ|μ1 |
...μr |
||||
|
|
||||||
|
(r ) |
||||||
|
! |
|
Λ 1 |
|
|||
|
|
|
|
= |
|
the total Lagrangian of (8.3.6) can be rewritten as
L (tot) = F T (γ 1 + θ j )F + 1 gI J (φ)∂μφI ∂μφJ
2
(8.3.8)
(8.3.9)
(8.3.10)
and the essential distinction between the two cases of (8.3.7) is given, besides the symmetry of θ , by the involutive property of j , namely we have:
D = 4ν | θ = θ T |
j 2 = −1 |
(8.3.11) |
D = 4ν + 2 | θ = −θ T |
j 2 = 1 |
|
7Whether the φI can be arranged into complex fields is not relevant at this level of the discussion.

8.3 Duality Symmetries in Even Dimensions |
313 |
Introducing dual and antiself-dual combinations:
D = 4ν
D = 4ν + 2
and the field-dependent matrices:
D = 4ν
D = 4ν + 2
F ± = F ij F j F ± = ±iF ±
(8.3.12)
F ± = F ± j F j F ± = ±F ±
N= θ − iγ
N= θ + iγ
(8.3.13)
N = θ + γ −N T = θ − γ
the tensor part of the Lagrangian (8.3.10) can be rewritten in the following way in the two cases:
|
|
|
|
i |
|
|
|
|
|
|
|
|
|
D = 4ν : |
Ltens = |
F |
+T N F |
+ − F −T N F − |
|||||||||
8 |
|||||||||||||
D = 4ν + 2 : |
Ltens = |
1 |
F |
+T N F |
+ + F −T N T F − |
||||||||
|
|||||||||||||
8 |
|||||||||||||
Introducing the new tensor: |
|
|
|
|
|
|
|
|
|
|
|
|
|
GμΛ1...μr |
≡ −(r!) |
∂L |
D = 4ν |
||||||||||
|
|
|
|||||||||||
∂F Λ |
|||||||||||||
|
|
|
|
|
|
|
μ1...μr |
|
|
|
|||
GμΛ1...μr |
|
|
|
|
∂L |
|
|
|
|||||
≡ (r!) |
|
|
|
D = 4ν + 2 |
|||||||||
∂F Λ |
|
|
|||||||||||
|
|
|
|
|
|
μ1...μr |
|
|
|
which, in matrix notation, corresponds to:
(8.3.14)
(8.3.15)
j G ≡ a |
∂L |
|
a |
|
|
|
|
= |
|
(γ 1 |
+ θ j )F |
(8.3.16) |
|
∂F T |
r! |
where a = depending on whether D = 4ν or D = 4ν + 2, the Bianchi identities and field equations associated with the Lagrangian (8.3.6) can be written as follows:
∂μ1 FμΛ1...μr = 0; |
∂μ1 GμΛ1...μr = 0 |
(8.3.17) |
This suggests that we introduce the 2n column vector:
V ≡ |
j F |
(8.3.18) |
j G |

314 |
8 Supergravity: A Bestiary in Diverse Dimensions |
and that we consider general linear transformations on such a vector:
|
|
j F |
|
|
A |
B j F |
|
||||
|
|
j G |
|
= C |
D j G |
|
(8.3.19) |
||||
|
A B |
|
|
|
|
|
|
|
|
|
|
For any matrix |
GL(2n, R) the new vector V |
of magnetic and electric field- |
|||||||||
C D |
strengths satisfies the same equations (8.3.17) as the old one. In a condensed nota- |
||||||||||||
|
|
|
|
|
|
|
|
|
|
|
|
|
tion we can write: |
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
∂V = 0 |
|
∂V = 0 |
|
|
(8.3.20) |
||||
Separating the self-dual and antiself-dual parts |
|
|
|
|||||||||
|
1 |
F + + F |
− ; |
1 |
|
|
+ + G |
− |
|
|||
|
F = |
|
G = |
|
|
G |
(8.3.21) |
|||||
|
2 |
2 |
||||||||||
and taking into account that for D = 4ν we have: |
|
|
|
|||||||||
|
|
G + = N F +; |
G − = |
|
F − |
|
(8.3.22) |
|||||
|
|
N |
|
|||||||||
while for D = 4ν + 2 the same equation reads: |
|
|
|
G + = N F +; G − = −N T F −
the duality rotation of (8.3.19) can be rewritten as:
D = 4ν : |
F + |
|
|
A |
B |
F + |
||
G + |
|
= C D N F + |
||||||
|
F − |
|
|
A |
B |
F − |
||
|
G − |
|
|
= C D |
|
F − |
||
|
|
N |
||||||
D = 4ν + 2 : |
F + |
|
|
A |
B |
F + |
||
G + |
|
= C D N F + |
||||||
|
F − |
|
|
A |
B |
|
|
F − |
|
G − |
|
= C D |
− |
N T F − |
|||
|
|
|
|
|
|
|
|
(8.3.23)
(8.3.24)
In both cases the problem is that the transformation rule of G ± must be consistent with the definition of the latter as variation of the Lagrangian with respect to F ± (see (8.3.15)). This request restricts the form of the matrix Λ = CA DB . As we are just going to show, in the D = 4ν case Λ must belong to the symplectic subgroup Sp(2n, R) of the special linear group, while in the D = 4ν + 2 case it must be in the pseudo-orthogonal subgroup SO(n, n):
|
A |
B |
|
|
|
|||
D = 4ν : |
C D Sp(2n, R) GL(2 |
n, R) |
||||||
|
|
(8.3.25) |
||||||
|
A |
B |
|
|
|
|
||
D = 4ν + 2 : |
C |
D SO(n, |
n) GL(2n, R) |

8.3 Duality Symmetries in Even Dimensions |
315 |
the above subgroups being defined as the set of 2n × 2n matrices satisfying, respectively, the following conditions:
Λ Sp(2n, R) → ΛT |
|
|
1 0 |
Λ = |
|
1 |
0 |
|||||||
|
|
|
|
|
|
0 |
1 |
|
|
|
0 |
1 |
||
Λ SO(n, n) → ΛT |
|
− |
|
0 |
Λ = |
1 |
− |
|
(8.3.26) |
|||||
1 |
|
|
0 |
|||||||||||
|
|
|
|
|
|
0 |
|
1 |
|
|
0 |
|
1 |
|
To prove the statement we just made, we calculate the transformed Lagrangian L
and then we compare its variation |
∂L |
with G ± as it follows from the postulated |
∂F T |
transformation rule (8.3.24). To perform such a calculation we rely on the following basic idea. While the duality rotation (8.3.24) is performed on the field strengths and on their duals, also the scalar fields are transformed by the action of some diffeomorphism ξ Diff(Mscalar) of the scalar manifold and, as a consequence of that, also the matrix N changes. In other words given the scalar manifold Mscalar we assume that in the two cases of interest there exists a surjective homomorphism of the following form:
ιδ : Diff(Mscalar) −→ GL(2 |
|
|
(8.3.27) |
n, R) |
|||
so that: |
|
||
|
ξ |
|
|
ξ Diff(Mscalar) : φI −→ φI |
(8.3.28) |
|
Aξ |
Bξ |
|
|
|
|
ιδ (ξ ) = |
GL(2n, R) |
|||||
Cξ |
Dξ |
Using such a homomorphism we can define the simultaneous action of ξ on all the fields of our theory by setting:
|
: |
φ −→ ξ(φ) |
|
||
ξ |
|
−→ |
ιδ (ξ )V |
(8.3.29) |
|
|
V |
|
N (φ) −→ N (ξ(φ))
where the notation (8.3.18) has been utilized. In the tensor sector the transformed Lagrangian, is
|
|
|
|
|
i |
|
|||||||
Ltens |
= |
|
|
F +T (A + BN )T N (A + BN )F + |
|
||||||||
|
8 |
|
|||||||||||
|
|
|
|
|
− F −T (A + B |
|
)T |
|
(A + B |
|
)F − |
(8.3.30) |
|
|
|
|
|
|
N |
N |
N |
||||||
for the D = 4ν case and |
|
|
|
|
|
|
|
|
|
|
|||
Ltens = |
|
i |
|
F +T (A + BN )T N (A + BN )F + |
|
||||||||
8 |
|
|
|||||||||||
|
|
− F −T A − BN T T N T A − BN T F − |
(8.3.31) |
for the D = 4ν + 2 case.

316 |
8 Supergravity: A Bestiary in Diverse Dimensions |
|
In both cases consistency with the definition of G + requires, that |
|
|
|
N ≡ N ξ(φ) = (Cξ + Dξ N )(Aξ + Bξ N )−1 |
(8.3.32) |
while consistency with the definition of G − imposes, in the D = 4ν case the transformation rule:
|
≡ |
|
ξ(φ) = (Cξ + Dξ |
|
)(Aξ + Bξ |
|
)−1 |
(8.3.33) |
N |
N |
N |
N |
and in the case D = 4ν + 2 the other transformation rule:
−N T ≡ −N T ξ(φ) = Cξ − Dξ N T Aξ − Bξ N T −1 (8.3.34)
It is from the transformation rules (8.3.32), (8.3.33) and (8.3.34) that we derive a restriction on the form of the duality rotation matrix Λξ ≡ ιδ (ξ ). Indeed, in the D = 4ν case we have that by means of the fractional linear transformation (8.3.32) Λξ must map an arbitrary complex symmetric matrix into another matrix of the same sort. It is straightforward to verify that this condition is the same as the first of conditions (8.3.26), namely the definition of the symplectic group Sp(2n, R). Similarly in the D = 4ν + 2 case the matrix Λξ must obey the property that taking the negative of the transpose of an arbitrary real matrix N before or after the fractional linear transformation induced by Λξ is immaterial. Once again, it is easy to verify that this condition is the same as the second property in (C.1.3), namely the definition of the pseudo-orthogonal group SO(n, n). Consequently the surjective homomorphism of (8.3.27) specializes as follows in the two relevant cases
ιδ : Diff(Mscalar) −→ Sp(2 |
|
|
|
|
|
|
|
n, R) |
(8.3.35) |
||||||
|
|
|
|
|
|
||
Diff(Mscalar) −→ SO(n, n) |
|
Clearly, since both Sp(2n, R) and SO(n, n) are finite dimensional Lie groups, while Diff(Mscalar) is infinite-dimensional, the homomorphism ιδ can never be an isomorphism and actually we always have:
dim ker ιδ = ∞ |
(8.3.36) |
What should be clear from the above discussion is that a family of Lagrangians as in (8.3.6) will admit a group of duality-rotations/field-redefinitions that will map one into the other member of the family, as long as a kinetic matrix NΛΣ can be constructed that transforms as in (8.3.32). A way to obtain such an object is to identify it with the period matrix occurring in problems of algebraic geometry. At the level of the present discussion, however, this identification is by no means essential: any construction of NΛΣ with the appropriate transformation properties is acceptable.
Note also that so far we have used the words duality-rotations/field-redefinitions and not the word duality symmetry. Indeed the diffeomorphisms of the scalar manifold we have considered were quite general and, as such had no claim to be symmetries of the action, or of the theory. Indeed the question we have answered is the