- •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
386 |
9 Supergravity: An Anthology of Solutions |
9.3.8 Gauged Maurer Cartan 1-Forms of OSp(8|4)
A fundamental ingredient in the construction of gauged supergravities is constituted by the gauging of Maurer Cartan forms of the scalar coset manifold G /H (see for instance [42] for a survey of the subject). The vector fields present in the supermultiplet, which are 1-forms defined over the space-time manifold M4, are used to deform the Maurer Cartan 1-forms of the scalar manifold G /H that are instead sections of T (G /H ). Mutatis mutandis, a similar construction turns out to be quite essential in the problem of gauge completion under consideration. In our case what will be gauged are the Maurer Cartan 1-forms of the supercoset
M 0|4N |
|
Osp(N | 4) |
(9.3.78) |
|||
|
|
|||||
osp |
= SO( |
) |
× |
Sp(4, R) |
|
|
|
|
N |
|
|
|
which contains the fermionic coordinates of the final superspace we desire to construct (for a thorough discussion of the orthosymplectic supergroups and of their cosets we refer the reader to Appendix C). The role of the space-time gauge fields is instead played by the U-connection (9.3.66) of the so(8) spinor bundle constructed over the internal 7-manifold (G /H )7.
Accordingly we define:
Λ ≡ L−1 |
L = L−1 dL + [U, L] |
(9.3.79) |
7 |
7 |
|
where 7U is the supermatrix defined by the canonical immersion of the so(8) Lie algebra into the orthosymplectic superalgebra:
7U = |
0 |
0 |
= I (U) |
0 |
U |
(9.3.80)
I : so(8) → osp(8|4)
As a result of their definition, the gauged Maurer Cartan forms satisfy the following deformed Maurer Cartan equations:
Λ + Λ Λ = L− |
1 |
|
(9.3.81) |
||||||||
|
(Θ) F |
[U], L(Θ) |
|||||||||
7 |
7 |
7 |
|
|
|
|
|
|
|
|
|
where |
|
|
|
|
|
|
|
|
|
|
|
|
|
|
0 |
|
|
0 |
|
|
|
||
|
|
|
|
||||||||
|
F [U] = |
0 |
|
|
F U |
] |
(9.3.82) |
||||
|
|
|
|
|
|
|
|
[ |
|
|
By explicit evaluation, from (9.3.81) we obtain the following deformation of the Maurer Cartan equations (9.4.3):
|
d xy + |
xz |
|
ty εzt + 4ieΦAx |
ΦAy , = −iΘAx FAB [U]ΘBy |
|
|||||||||
|
7 |
|
|
7 |
|
|
7 |
|
7 |
7 |
|
|
|
|
|
|
AAB |
|
eAAC |
|
|
ACB |
|
4iΦx |
Φy |
εxy |
|
OAP (Θ)FP Q |
U OQB (Θ) |
|
|
|
7 |
− |
|
7 |
|
7 |
− |
7A |
7B |
|
= |
− FAB [U] [ |
] |
(9.3.83) |
|
|
|
x |
|
xy |
|
|
z |
− eA7AB |
x |
= |
x |
|
|
||
|
dΦ7A |
+ 7 |
|
εyzΦ7A |
Φ7B |
ΘP FP Q[U]OQA(Θ) |
|
9.3 Flux Vacua of M-Theory and Manifolds of Restricted Holonomy |
387 |
The above equations are our main starting point to construct a supergauge completion for compactifications with less preserved supersymmetry.
9.3.9 Killing Spinors of the AdS4 Manifold
The next main item for the construction of the supergauge completion is given by the Killing spinors of anti de Sitter space. Indeed, in analogy with the Killing spinors of the internal 7-manifold, defined by (9.3.43) with m = 1, we can now introduce the notion of Killing spinors of the AdS4 space and recognize how they can be constructed in terms of the coset representative, namely in terms of the fundamental harmonic of the coset.
The analogue of (9.3.43) is given by:
Sp(4)χx ≡ d − |
4 Babγab − 2eγa γ5Ba χx = 0 |
(9.3.84) |
|
|
1 |
|
|
and states that the Killing spinor is a covariantly constant section of the sp(4, R) bundle defined over AdS4. This bundle is flat since the vanishing of the sp(4, R) curvature is nothing else but the Maurer Cartan equation of sp(4, R) and hence corresponds to the structural equations of the AdS4 manifold. We are therefore guaranteed that there exists a basis of four linearly independent sections of such a bundle, namely four linearly independent solutions of (9.3.84) which we can normalize as follows:
|
|
|
|
x γ5χy = i(C γ5)xy = εxy |
|
(9.3.85) |
|||||||
|
|
|
χ |
|
|||||||||
Let LB the coset representative mentioned in (C.2.6) and satisfying: |
|
||||||||||||
|
1 |
Babγ |
ab − |
2eγ |
|
γ |
Ba |
= B = |
L−1 dL |
|
(9.3.86) |
||
|
|
|
|
||||||||||
− 4 |
|
a |
5 |
|
B |
B |
|
||||||
It follows that the inverse matrix LB−1 satisfies the equation: |
|
|
|||||||||||
|
|
|
|
|
(d + |
|
B )LB−1 = 0 |
|
|
(9.3.87) |
Regarding the first index y of the matrix (L−B 1)y x as the spinor index acted on by the connection B and the second index x as the labeling enumerating the Killing spinors, (9.3.87) is identical with (9.3.84) and hence we have explicitly constructed its four independent solutions. In order to achieve the desired normalization (9.3.85) it suffices to multiply by a phase factor exp[−i 14 π ], namely it suffices to set:
χ(x)y |
= exp −i |
1 |
π |
LB−1 y x |
(9.3.88) |
4 |
388 |
9 Supergravity: An Anthology of Solutions |
In this way the four Killing spinors fulfill the Majorana condition. Furthermore since L−B 1 is symplectic it satisfies the defining relation
LB−1C γ5LB = C γ5 |
(9.3.89) |
which implies (9.3.85).
9.3.10 Supergauge Completion in Mini Superspace
As it was observed many years ago in [26, 41] and it is reviewed at length in the book [44], given a bosonic Freund Rubin compactification of M-theory on an internal coset manifold M7 = HG which admits N Killing spinors it is fairly easy to extend it consistently to a mini-superspace M 11|4×N which contains all of the eleven bosonic coordinates but only 4 × N θ s, namely those which are associated with unbroken supersymmetries. We review this extension reformulating it in a more inspiring way that treats the two bosonic manifolds in a symmetric way.
In the original formulation, the mini superspace is viewed as the following tensor
product |
|
|
M 11|4×N ≡ Mosp4|4N × |
G |
(9.3.90) |
|
||
H |
and in order to construct the FDA p-forms, in addition to the Maurer Cartan forms of the above coset, we just need to introduce the Killing spinors of the bosonic internal manifold. Let ηA be an orthonormal basis of N eight component Killing spinors satisfying the Killing spinor condition (9.3.44) and the normalization:
ηA T ηB = δAB |
(9.3.91) |
Next, following [44] and [60], we can now write the complete solution for the background fields in the case of AdS4 × HG Freund-Rubin backgrounds:
|
|
|
V a |
|
Ea |
|
|
|
|
|
|
|
|
|
|
|||
V a |
= |
V α |
= Bα |
|
1 |
η |
A |
τ α ηB AAB |
||||||||||
7 |
|
|
7 |
|
|
|
|
− 8 |
|
|
|
|
|
|
||||
|
|
|
ωab= |
ω |
ab |
|
|
|
|
|
|
|
|
|
||||
ωab |
|
|
|
7 |
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
ωαb = |
0 |
|
|
|
|
|
|
|
|
|
|
(9.3.92) |
|||||
|
|
|
|
ˆ |
|
|
|
|
|
|
|
|
|
|
|
|
|
|
ˆ |
= ˆ αβ = |
|
|
αβ |
+ |
e |
|
|
|
αβ |
ηB AAB |
|||||||
|
|
ηAτ |
||||||||||||||||
Ψ |
= |
|
ωˆ |
= B |
|
4 |
|
|||||||||||
|
ψ |
A |
|
|
|
|
|
|
|
|
|
|
|
|
||||
7 |
η |
A |
|
|
|
|
|
|
|
|
|
|
|
|
|
|||
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
where {Bαβ , Bα } are the spin connection and the vielbein, respectively, of the bosonic seven dimensional coset manifold HG .
9.3 Flux Vacua of M-Theory and Manifolds of Restricted Holonomy |
389 |
Let us now observe that in this formulation of the superextension, the fermionic coordinates are actually attached to the space-time manifold AdS4, which is superextended to a supercoset manifold:
AdS |
superextension |
Osp(N | 4) |
|
M 4|4×N |
(9.3.93) |
||||
= |
|
≡ |
|||||||
4 |
SO( |
N |
) |
× |
SO(1, 3) |
|
|
||
|
|
|
|
|
|
|
|
At the same time the internal manifold M7 = HG is regarded as purely bosonic and it is twisted into the fabric of the Free Differential Algebra through the notion of the Killing spinors ηA, defined as covariantly constant sections of the SO(8) spinor bundle over M7.
Yet whether supersymmetries are preserved or broken precisely depends on the structure of the SO(8) spinor bundle on M7. Henceforth it is suggestive to think that the fermionic coordinates should not be attached to either the internal or to external manifold, rather they should live as a fibre over the bosonic manifolds. The first step in order to realize such a programme consists of a reformulation of the superextension in minisuperspace that treats the space-time manifold AdS4 and the internal manifold M7 in a symmetric way and in both instances relies on the notion of Killing spinors of the bosonic submanifold as a way of including the fermionic one. This can be easily done in view of (C.2.2) whose precise meaning we have explained in Sect. C.2. Indeed in view of (C.2.2) we can look at (9.3.90) in the following equivalent, but more challenging fashion:
M 11|4×N = AdS4 × M 0|4×N × M7 |
|
|
|
|
|
|
|
|||||||||||
|
Sp(4, R) |
|
|
|
Osp(N | 4) |
|
|
|
|
G |
|
(9.3.94) |
||||||
≡ SO(1, 3) |
× SO(N ) × Sp(4, R) |
× |
|
H |
||||||||||||||
|
|
|||||||||||||||||
|
|
|
|
|
|
|
|
|
|
|
|
M7 |
|
|||||
|
|
AdS4 |
4×N fermionic manifold |
|
|
|
||||||||||||
|
|
|
|
|
The above equation simply corresponds to the rewriting of (9.3.92) in the following way
|
|
|
|
V a |
= |
Ba |
|
|
1 |
|
|
|
γ a χ |
|
xy |
|
||||||
|
|
|
|
|
|
χ |
|
|
||||||||||||||
V a = V α |
|
|
α− |
|
81 |
η τ α η |
y |
F |
|
|||||||||||||
|
|
|
|
7 |
|
B |
|
|
|
e |
|
|
|
x |
|
|||||||
7 |
|
|
= |
|
− |
8 |
|
|
A |
B AAB |
|
|||||||||||
|
|
|
|
7ab |
|
|
|
ab |
|
|
1 |
|
|
|
|
|
ab |
xy |
|
|||
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
||||||||
ω |
ab |
|
ωˆ αb = B |
|
+ |
2 |
χ x γ5 |
γ |
|
χy F |
(9.3.95) |
|||||||||||
|
|
|
ω |
|
|
0 |
|
|
|
|
|
|
|
|
|
|
|
|
|
|
||
ˆ |
|
= |
|
ˆ |
= |
|
|
|
|
|
|
e |
|
|
|
|
|
|
|
|||
|
|
|
|
|
|
|
|
|
ηAτ αβ ηB AAB |
|
||||||||||||
|
|
|
|
ωˆ αβ = Bαβ + |
4 |
|
||||||||||||||||
|
7 |
= |
|
|
|
|
|
x A |
|
|
|
|
|
|
|
|
|
|
|
|
||
|
ηA |
χx Φ | |
|
|
|
|
|
|
|
|
|
|
|
|
||||||||
|
Ψ |
|
|
|
|
|
|
|
|
|
|
|
|
|
|
The next step is that of replacing the Maurer Cartan forms of the fermionic manifold with their gauged counterparts. This should be the order zero solution of the supergauge completion involving also the broken θ s. Next order contributions in the broken θ s however are necessary. For M-theory this problem was not yet solved while it was solved in the case of the type IIA compactification that we discuss next.