three lectures on super gravity
TRANSCRIPT
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Three Lectures on Supergravity
Joaquim GomisBased on the SUGRA book of Dan Freedman
and Antoine Van Proeyen to appear in Cambridge University Press
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Public Material
Lectures on supergravity, Amsterdam-Brussels-Paris doctoral school, Paris 2009, October-November 2009
http://itf.fys.kuleuven.be/~toine/SUGRA_DoctSchool.pdfA. Van Proeyen, Tools for supersymmetry, hep-th 9910030
Lectures on Supergravity. Universidad Catolica. Santiago de Chile.Novmber-December 2009. Joaquim Gomis, web page Jorge Alfaro
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Overview of Supersymmetry andSupergravity
• Super Poincare
Translations
Spinor supercharge (odd)
Lorentz transformations
Massless multiplets contains spins (s, s-1/2), for s=1/2, 1, 2,
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Overview of Supersymmetry andSupergravity
Supergravity
Gauged supersymmetry was expected to be an extension of generalRelativity with a superpartner of the gravito call gravitino
Multiplet (2,3/2)
S. Ferrara, D. Freedman, P. Van Nieuwenhuizen (1976)S. Deser, B. Zumino (1976)D. Volkov, V. Soroka (1973),
Extensions with more supersymmetries and extension has beenconsidered, N=2 supergravity, special geometry. N=1 Supergravity in 11d
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Motivation for Supergravity
Supergravity (SUGRA) is an extension of Einstein's general relativity to include supersymmetry (SUSY). General relativity demands extensions since it has shortcomings including at least the following:
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Motivation for Supergravity• Space time singularities. The singularity theorems of Penrose,
Hawking and Geroch shows that general relativity is incomplete.
• Failure to unify gravity with the strong and electro weak forces.
• Einstein gravity is not power counting renormalizable. It is renormalizable as an effective theory. It is not a fundamental theory
• If we include supersymmetry in a theory of gravity. The simple example of divergences: zero point energy of the vacuum, can potentially be cancelled by super partners of ordinary particles
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The current status of supergravity
• A reliable approximation to M-theory.• An essential ingrediente for supersymmetric
phenomenology ( minimal supersymmetricestándar model coupled to N=1 supergravity).
• Applications in cosmology• An crucial part for the AdS/CFT correspondence
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Index
Clifford algebras ans spinorsFree Rarita-Schwinger fieldDifferential geometryFirst and second order formulation of gravityN=1 Global Supersymmetry in D=4
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Index
N=1 pure supergravity in 4 dimensionsD=11 supergravityKilling spinors equations and BPS solutions
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Clifford algebras and spinors
• Clifford algebras in general dimensions
Euclidean Clifford algebras
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Clifford algebras and spinors
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Clifford algebras and spinors
,
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Clifford algebras and spinors
The antysymmetrization indicated with […] is always with total weight 1
distinc indexes choices
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Basis of the algebra for even dimensions
Other possible basis
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The highest rank Clifford algebra element
Provides the link bewteen even and odd dimensions
Properties
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Weyl spinors
No explicity Weyl representation will be used in these lectures
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Odd space dimension D=2m+1
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Symmetries of gamma matrices
implies
Explicit forms conjugation matrix
The possible sign factors depend on the spacetime dimension D modulo 8And on r modulo 4
For odd dimension C is unique (up to phase factor)
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Symmetries of gamma matrices
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Symmetries of gamma matrices• Since we use hermitian representations, the symmetry
properties of gamma matrices determines also itscomplex conjugation
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Adjoint spinor• We have defined the Dirac adjoint, which involves the complex
conjugate. Here we define the conjugate of “any” spinor using thetranspose and the charge conjugation matrix
Symmetry properties for bilinears
Majorana flip
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Spinor indexes
Note
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Spinor indexesThe gamma matrices have components
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Fierz rearrangement• In supergravity we will need changing the pairing of
spinors in products of bilinears, which is called Fierzrearrangement
Basic Fierz identity from
Expanding any A as
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Fierz rearrangement
We get
Where
Completeness relation
Is the rank of
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Charge conjugate spinorComplex conjugation is necessary to verify that the lagrangian involvingspinor bilinears is hermitian.
Charge conjugate of any spinor
It coincides withe Dirac conjugate except for the numerical factor
Barred charge conjugate spinor
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Majorana spinors• Majorana fields are Dirac fields that satisfy and addtional
“reality” condition, whic reduces the number degrees offreedom by two. More fundamental like Weyl fields
Particles described by a Majorana field are such that particles andantiparticles are identical
Majorana field
We have which implies
Recall
which implies
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Majorana spinors
In this case we have Majorana spinors. We have that the barred conjugatedspinor and Dirac adjoint spinor coincide
In the Majorana case we can have real representations for the gammaMatrices . For D=4
Two cases
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Majorana spinors
We have B=1, then Implies
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Majorana spinors in physical theories
for D=2,3, 4 mod 8 . Majorana and Dirac fields transform in the same way underLorentz transformations, but half degrees of freedom
For commuting spinors vanishes
Is a total derivative, we need anticommuting Majoranaspinors
The Majorana field satisfies the conventional Dirac equation
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Majorana spinors in physical theories
Majorna action in terms of “Weyl” fields, D=4
equations of motion
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The free Rarita-Schwinger field
Consider now a free spinor abelian gauge fieldwe omit the spinor indexes
Gauge transformation
This is fine for a free theory, but interacting supergravity theories are more restrictive .We will need to use Majorana and/or Weyl spinors
Field strenght gauge invariant
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The free Rarita-Schwinger field
• ActionProperties: a) Lorentz invariant, b) first order in space-time derivativesc) gauge invariant, d) hermitean
The lagrangian is invariant up to a total derivative
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The free Rarita-Schwinger field
• Equation of motion
Noether identities
Using
We can write the equations of motion as
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Differential geometry
• The metric and the frame fieldLine element Non-degenerate metric
Frame field
Inverse frame field
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Differential geometry
• Frame field
Vector under Lorentz transformations
Vector field
Dual form
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Volume forms and integrationcan be integrated
Canonical volume form depends of the metric or frame field
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Hodge duality of forms
Lorentzian signature
Euclidean signature
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p-forms gauge fields
Bianchi identity
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p-forms gauge fieldsequations of motion, useful relation
Bianchi identity
A p-form and D-p-2 form are dual
Algebraic equation of motion
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First structure equation
• Spin connection
same transformation properties that YM potential for the group O(D-1,1)
it is not a Lorentz vector. Introduce thespin connection connection one form
The quantity
transforms as a vector
Let us consider the differential of the vielbvein
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First structure equation
• Lorentz Covariant derivatives
The metric has vanishing covarint derivative.
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First structure equation
The geometrical effect of torsion is seen in the properties of an infinitesimalparallelogram constructed by the parallel transport of two vector fields.
For the Levi-Civita connection the torsion vanishes
Non-vanishing torsion appears in supergravity
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First structure equation
• Covariant derivatives
The structure equationimplies
is called contorsion
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First structure equation
• The affine connectionOur next task is to transform Lorentz covariant derivatives to covariantderivatives with respect to general conformal transformations
,Affine connectionrelates affine connection with spin connection
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First structure equation
• The affine connection
For mixed quantities with both coordinate ans frame indexes, it isuseful to distinguish among local Lorentz and coordinate covariantderivatives
Vielbein postulate equivalent to
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First structure equation
• Partial integration
The second term shows the violation of the manipulations of the integration byParts in the case of torsion
We have
from which
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Second structure equation
• Curvature tensorYM gauge potential for the
Group O(D-1,1)
YM field strength. We define the curvature two form
Second structure equation
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Bianchi identities
we have
First Bianchi identity, it has no analogue in YM
usual Bianchi identity for YM
useful relation
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Ricci identities and curvature tensorCommutator of covariant derivatives
Curvature tensor
Second Bianchi identity
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Ricci tensorRicci tensor
Scalar curvature R=
If there is no torsion
Useful relation
Hilbert action
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Dimensional analysis and Planck units
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General relativity
• Einstein-Hilbert action in first order formalism
GR can be view as a “gauge” theory of the Poincare group?
are the components of the Lorentz curvature and torsion
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General relativityThe Poincare gauge transformations are
Local translations
Local Lorentz
Up to a total derivate we EH action is not invariant
If we impose by hand the vanishing of the torsion we have invariance. Notice the vanishing is the equation of motion of EH action with respectto the spin connection. In this way we get the second order formulation
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The first order formalism for gravityand fermions
Field content
Fermion field Action
The total covariant derivative and the Lorentz covariant derivativecoincide for spinor field but not for the gravitino
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The first and second orderformulations of general relativity
Constant gamma matrices verify
The curved gamma matrices transforms a vector under coordinate transformationsBut they have also spinor indexes
holds for any affine connection with or without torsion
• Curved space gamma matrices
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The first and second orderformulations of general relativity
• Fermion equation of motion
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The first and second orderformulations of general relativity
• The first order formalism for gravity and fermions
Variation of the gravitational action
We have used
Euation of motion of the spin connection
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The first and second orderformulations of general relativity
• The first order formalism for gravity and fermionsIntegration by parts
Form the fermion action
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The first and second orderformulations of general relativity
• The first order formalism for gravity and fermionsThe equations of motion of the spin connection gives
If we substitute
the right hand side is traceless therefore also the torsion is traceless
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The first and second orderformulations of general relativity
• The first order formalism for gravity and fermions
The physical equivalent second order action is
Physical effects in the fermion theories with torsion and without torsionDiffer only in the presence of quartic fermion term.This term generates 4-point contact diagrams .
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N=1 Global Supersymmetry in D=4
• Susy algebra
equivalently
at quantum level
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N=1 Global Supersymmetry in D=4
• Susy algebraIn Weyl basis
In this form it is obvious the U(1) R symmetry
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N=1 Global Supersymmetry in D=4
• Basic multiplets
or
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N=1 Global Supersymmetry in D=4
• Susy field theories of the chiral multiplet
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N=1 Global Supersymmetry in D=4
• Transformations rules of the antichiral multiplet
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N=1 Global Supersymmetry in D=4
• Susy algebra
has beenused
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N=1 Global Supersymmetry in D=4
• Action
W(Z) superpotential, arbitrary holomorphic function of Z
Complete action
Are not a dynamical field, their equations of motion are algebraicwe can eliminate them
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N=1 Global Supersymmetry in D=4
• Wess-Zumino model
Eliminating the auxiliary field F
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N=1 Global Supersymmetry in D=4
• Susy algebraNote that the anticommutator is realized as the commutator of two
variations with parameters
for Majorana spinorsIf we compute the left hand side, this dones not the anticommutator of thefermionic charges because any bosonic charge that commutes with fieldwill not contribute
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N=1 Global Supersymmetry in D=4
Now the symmetry algebra only closes on-shell
the extra factor apart from translation is a symmetric combination of the equationof the fermion field
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• Basics
Therefore we have diffeomorphism. Thus local susy requires gravity
fields
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1) If there is some sort of broken global symmetry. N=1 D=4 supergravity coupledto chiral and gauge multiplets of global Susy could describe the physics ofelementary particles
2) D=10 supergravity is the low energy limit of superstring theory. Solutions ofSUGRA exhibit spacetime compactification
3) Role of D=11 supergravity for M-theory
4) AdS/CFT in the limit in which string theory is approximated by supergravity.correlations of the boundary gauge theory at strong coupling are available fromweak coupling classical calculations in five and ten dimensional supergravity
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• Transformation rules for gauge theory point of view
Gauge prameters
gauge transformations
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First order formalism
We regard the spin connection as an independent variable from the frame field.The action is
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• First order formalism
valid for D=2,3,4,10, 11 where Majorana spinors exist
,therefore we have
Let us compute the equations of the spin connection
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The spin connection equation ofmotion is
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• First order formalism
The fifth rank tensor vanishes for D=4. For dimensions D>4 this term is notVanishing and is one the complications of supergravity
The equivalent second order action of gravity is
With
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• Local supersymmetry transformationsThe second order action for N=1 D=4 is supergravity is complete and it islocal supersymmetry
which includes the gravitino torsionThe variation of the action contains terms which are first, third and fifth orderin the gravitino field. The terms are independent and must cancel separately
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• The universal part of supergravity. Second orderformalism
Is the torsion-free spin connection
We not need to include the connectiondue to symmetry properties
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• Transformation rules
Variation of the gravitational action
The variation of the action consists of terms linear in From the frame field
variation and the gravitino variation and cubic terms from the field variation
of the gravitino action
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In the second order formalism, partial integrationis valid, so we compute by two
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Finaly we have
Therefore the linear terms cancel
First Bianchi identity without torsin
,
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Infinitesimal transformation of the frame field
covariant form
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the susy parameter
the dots means a symmetric combination of the equations of motion
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• Generalizations
Supergravity in dimensions different from four
D=10 supergravities Type IIA and IIB are the low energy limits of superstringtheories of the same name
Type II A and gauged supergravities appear in ADS/CFT correspondence
D=11 low energy limit of M theory that it is not perturbative
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Field content
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Gauge transformation of 3-form
Ansatz action
Initially we use second order formalism with torsion-free spin connection
Bianchi dentity
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• Ansatz transformations
useful relationsUseful relations
To determine the constants we consider the free action (global susy)
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• transformations
and Bianchi identity we get
To determine c we compute the commutator of two susy transformations
If With gauge transformation given theparameter
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• transformationsthe conserved Noether current is (coefficient of
Ansatz for the action and transformations in the interacting case. We introducethe frame field and a gauge susy parameter
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• Action
We need to find the dots
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• Action
Full action
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The spinor bilinears have a special role. They are non-vanishing fot the classicalBPS M2 and M5 solutions .
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IIA SUGRA bosonic fields
Fermionic fields, non-chiral gravitino, non-chiral dilatino
5,6
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Bogomol’ny bound• Consider an scalar field theory in 4d flat space time
There are two vacua at
We expect a domain wall separating the region of two vacua
We look for an static configuration connecting the two vacua
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Bogomol’ny bound
• BPS procedureThe potential V can be wriiten in terms of superpotential W
Energy density in terms energy momentum tensor
Total energy
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Bogomol’ny bound
where
We have an energy bound
which is saturated if the first order equation, BPS equation is verified
In this case the energy is
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Domain wall as a BPS solution
One can prove that this BPS solution is also a solution of the second orderequations of motion
Notice that the domain wall is non-perturbative solution of the equations of motion
If the theory can be embbed in a supersymmetric theory, the solutions of theBPS equations will preserve some supersymmetry
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Effective Dynamics of the domain wallThe width of the domanin wall is If we consider fluctuations of
the scalar filed with wave length >>L the dynamics of the will be Independent of of the details of the wall.
The lagrangian up to quadratic fluctuations is
Let us do the separation of variables
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Effective Dynamics of the domain wallTo study the small perturbations we we should study the eigenvalueproblem
Exits a zero mode
This zero mode corresponds to a massless excitation and it is associatedwith the broken translation invariance
The action for these fluctuations given by
It describe the accion of a membrane, 2-brane, at low energies
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Effective Dynamics of the domain wallThe membrane action to all orders is given by
where is teh determinat of the induced metric
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Supersymmetric domain wall
• WZ Action
W(Z) superpotential, arbitrary holomorphic function of Z
Complete action
Are not a dynamical field, their equations of motion are algebraicwe can eliminate them
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Domain wall ½ BPS The susy transformations for the WZ model are
For the domain wall ansatz the transformation of the should be
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Domain wall ½ BPS
This condition implies
and
Note that this supersymmetric calculation recovers the result of the bosonic BPSCalculation. Therefore the domain wall is ½ BPS
This result can be deduced from the anticommutator of spinorial charges
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Classical Solutions of Supergravity
• The solutions of supergravity give the metric, vector fields and scalar fields.
• The preserved supersymmetry means some rigidsupersymmetry
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Killing Spinors and BPS Solutions
• N=1 D=4 supergravityFlat metric with fermions equal to zero is a solution of supergravity with
The residual global transformations are determined by the conditions
The Killing spinors of the Minkowski background are the set of 4 independentconstant Majorana spinors. We have D=4 Poincare Susy algebra
Vacuum solution
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Killing vectors and Killing spinors
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Killing Spinors and BPS Solutions
• The integrability condition for Killing spinors
A spacetime with Killing spinors satisfies
Integrability condition
only if
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Killing spinors for pp-wavesAnsatz for the metric
For H=0 reduces to Minkowski spacetime in light-cone coordinates
Flat metric in these coordinates
Note that is a covariant constant null vector
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Killing spinors for pp-wavesThe frame 1-forms are
From the first Cartan structure equation we get the torsion free spinconnection one forms
and from the second one
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Killing spinors for pp-wavesThe Killing spinor conditions are
explicitely
All conditions are verified if we take constant spinors with constraint
Since there are two Killing spinors.
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Killing spinors for pp-wavesNotice
To complete the analysis we need the Ricci tensor. The non-trvial component is
Therefore the pp-wave is Ricic flat if and only if H is harmonic in the variables x,y
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pp-waves in D=11 supergravityEleven dimensional supergravity with bosonic fileds the metric and thefour-form field strength has pp-wave solutions
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pp-waves in D=11 supergravity
If we choose
They have at least 16 Killing spinors. If one choose
The number of Killing spinors is 32!, like
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Spheres
The metric of the sphere is obtained as induced metric of the flat
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SpheresFrame one forms
Spin connection. First structure equation
Curvature. Second curvature equation
Constant positive curvature
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SpheresRecursive proocedure for higher dimensional sphres
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Anti-de Sitter spacesimple solutions of supergravity
with negative constant solution
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Anti-de Sitter space
Ads as a coset space
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Anti-de Sitter space
• MC 1-form
Ads metric
Ads can be embedded in pseuo-Euclidean space
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Anti-de Sitter space
metric
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Anti-de Sitter space
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Anti-de Sitter spaceNote that varies in (-R.R)
Local parametrization
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Global parametrization
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Anti-de Sitter space
Different embeddings
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Anti-de Sitter space, covers the whole hyperbolid for
the algunlar variables the whole
New radial coordinate
Another possibility
It is conformalto the direct product of the real line, time coordinate, times theSphere in D-1 dimensions
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Anti-de Sitter space
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Anti-de Sitter space
The metric is conformal to the positive region of D dimensional Minlowski space with coordinates
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Killing spinor are solutions of
Integrability condition
If we insert vanishes identically
IIt is a hint that AdS is a maximally supersymmetric space
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Frame fields
Spin connection
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The last term includes transverse indexes.