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Full Integrability of Supergravity Billiards: the arrow of time, asymptotic states and trapped surfaces in the cosmic evolution Lecture by Pietro Frè and Alexander S. Sorin In connection with the nomination for the JINR prize 2008

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Page 1: Full Integrability of Supergravity Billiards: the arrow of time, asymptotic states and trapped surfaces in the cosmic evolution Lecture by Pietro Frè and

Full Integrability of Supergravity Billiards:

the arrow of time, asymptotic states and trapped surfaces in the cosmic evolution

Lecture by Pietro Frè andAlexander S. Sorin

In connection with the nomination for the JINR prize 2008

Page 2: Full Integrability of Supergravity Billiards: the arrow of time, asymptotic states and trapped surfaces in the cosmic evolution Lecture by Pietro Frè and

Standard Cosmology

Standard cosmology is based on the cosmological principle.

Homogeneity Isotropy

Page 3: Full Integrability of Supergravity Billiards: the arrow of time, asymptotic states and trapped surfaces in the cosmic evolution Lecture by Pietro Frè and

Evolution of the scale factorwithout cosmological

constant

Page 4: Full Integrability of Supergravity Billiards: the arrow of time, asymptotic states and trapped surfaces in the cosmic evolution Lecture by Pietro Frè and

From 2001 we know that the Universe is spatially flat (k=0) and

that it is dominated by dark energy.

Most probably there has been inflation

Page 5: Full Integrability of Supergravity Billiards: the arrow of time, asymptotic states and trapped surfaces in the cosmic evolution Lecture by Pietro Frè and

The scalar fields drive inflation while rolling down from a maximum to a minimum

• Exponential expansion during slow rolling

• Fast rolling and exit from inflation

• Oscillations and reheating of the Universe

Page 6: Full Integrability of Supergravity Billiards: the arrow of time, asymptotic states and trapped surfaces in the cosmic evolution Lecture by Pietro Frè and

The isotropy and homogeneity are proved by

the CMB spectrum

Page 7: Full Integrability of Supergravity Billiards: the arrow of time, asymptotic states and trapped surfaces in the cosmic evolution Lecture by Pietro Frè and

WMAP measured anisotropies of CMB

The milliKelvin angular variations of CMB temperature are the inflation blown upimage of Quantum fluctuations of the gravitational potential and the seeds of large scale cosmological structures

Page 8: Full Integrability of Supergravity Billiards: the arrow of time, asymptotic states and trapped surfaces in the cosmic evolution Lecture by Pietro Frè and

Accelerating Universe dominated by Dark Energy

Equation of State

Page 9: Full Integrability of Supergravity Billiards: the arrow of time, asymptotic states and trapped surfaces in the cosmic evolution Lecture by Pietro Frè and

Non isotropic Universes

This is what happens if there is isotropy !

Relaxing isotropy an entire new world of phenomena opens up

In a multidimensional world, as string theory predicts, there is no isotropy among all dimensions!

Page 10: Full Integrability of Supergravity Billiards: the arrow of time, asymptotic states and trapped surfaces in the cosmic evolution Lecture by Pietro Frè and

Cosmic Billiards before 2003A challenging phenomenon, was proposed, at the beginning of this millenium, by a number of authors under the name of cosmic billiards. This proposal was a development of the pioneering ideas of Belinskij, Lifshits and Khalatnikov, based on the Kasner solution of Einstein equations. The Kasner solution corresponds to a regime, where the scale factors of a D-dimensional universe have an exponential behaviour . Einstein equations are simply solved by imposing quadratic algebraic constraints on the coefficients . An inspiring mechanical analogy is at the root of the name billiards.

Page 11: Full Integrability of Supergravity Billiards: the arrow of time, asymptotic states and trapped surfaces in the cosmic evolution Lecture by Pietro Frè and

Some general considerations on roots and gravity.......

String Theory implies D=10 space-time dimensions.

Hence a generalization of the standard cosmological metric is of the type:

In the absence of matter the conditions for this metric to be Einstein are:

Now comes an idea at first sight extravagant.... Let us imagine that

are the coordinates of a ball moving linearly with constant velocity

What is the space where this fictitious ball moves

Page 12: Full Integrability of Supergravity Billiards: the arrow of time, asymptotic states and trapped surfaces in the cosmic evolution Lecture by Pietro Frè and

ANSWER:The Cartan subalgebra of a rank 9 Lie algebra.

h1

h2

h9

What is this rank 9 Lie algebra?

It is E9 , namely an affine extension of the Lie algebra E8

Page 13: Full Integrability of Supergravity Billiards: the arrow of time, asymptotic states and trapped surfaces in the cosmic evolution Lecture by Pietro Frè and

Lie algebras and root systems

Page 14: Full Integrability of Supergravity Billiards: the arrow of time, asymptotic states and trapped surfaces in the cosmic evolution Lecture by Pietro Frè and

Lie algebras are classified.......

by the properties of simple roots. For instance for A3 we have 1, 2 , 3

such that...........

1

2

3

2+3

1+2

1+2 +3

It suffices to specify the scalar products of simple roots

And all the roots are given

For instance for A3

There is a simple way of representing these scalar

products:Dynkin diagrams

1 2 3

Page 15: Full Integrability of Supergravity Billiards: the arrow of time, asymptotic states and trapped surfaces in the cosmic evolution Lecture by Pietro Frè and

Algebras of the type

4

1 6 5 3 2 1

1 2 1

exist for any

Algebras of the type exist only for

E series (exceptional)

In an euclidean space we cannot fit more than 8 linear independent vectors with angles of 120 degrees !!The group Er is the duality group of String

Theory in dimension D = 10 – r + 1

In D=3 we have E8

Then what do we have for D=2 ?

Page 16: Full Integrability of Supergravity Billiards: the arrow of time, asymptotic states and trapped surfaces in the cosmic evolution Lecture by Pietro Frè and

We have E9 !

How come? More than 8 vectors cannot be fitted in an euclidean space at the prescribed angles !

Yes! Euclidean!! Yet in a non euclidean space we can do that !!

Do you remember the condition on the exponent pi = (velocity of the little ball)

where

If we diagonalize the matrix Kij we find the eigenvalues

Here is the non-euclidean signature in the Cartan subalgebra of E9. It is an

infinite dimensional algebra ( = infinite number of roots!!)

Page 17: Full Integrability of Supergravity Billiards: the arrow of time, asymptotic states and trapped surfaces in the cosmic evolution Lecture by Pietro Frè and

Now let us introduce also the roots......

h1

h2

h9

There are infinitely many, but the time-like ones are in finite number. There are 120 of them as in E8. All the others are light-like

Time like roots, correspond to the light fields of Superstring Theory different from the diagonal metric: off-diagonal components of the metric and p-form fields

When we switch on the roots, the fictitious cosmic ball no longer goes on straight lines. It bounces!!

Page 18: Full Integrability of Supergravity Billiards: the arrow of time, asymptotic states and trapped surfaces in the cosmic evolution Lecture by Pietro Frè and

The cosmic Billiard

The Lie algebra roots correspond to off-diagonal elements of the metric, or to matter fields (the p+1 forms which couple to p-branes)

Switching a root we raise a wall on which the cosmic ball bounces

Or, in frontal view

Page 19: Full Integrability of Supergravity Billiards: the arrow of time, asymptotic states and trapped surfaces in the cosmic evolution Lecture by Pietro Frè and

Before 2003: Rigid Billiards

h-space CSA of the U algebra

walls hyperplanes orthogonalto positive roots (hi)

bounces Weyl reflections

billiard region Weyl chamber

The Supergravity billiard is completely determined by U-duality group

Smooth billiards:

Asymptotically any time—dependent solution defines a zigzag in ln ai space

Damour, Henneaux, Nicolai 2002 --

Exact cosmological solutions can be constructed using U-duality (in fact billiards are exactly integrable)

bounces Smooth Weyl reflections

walls Dynamical hyperplanes

Frè, Sorin,

and collaborators,

2003-2008

series of papers

Page 20: Full Integrability of Supergravity Billiards: the arrow of time, asymptotic states and trapped surfaces in the cosmic evolution Lecture by Pietro Frè and

What is the meaning of the smooth cosmic billiard ?

• The number of effective dimensions varies dynamically in time!

• Some dimensions are suppressed for some cosmic time and then enflate, while others contract.

• The walls are also dynamical. First they do not exist then they raise for a certain time and finally decay once again.

• The walls are euclidean p-branes! (Space-branes)

• When there is the brane its parallel dimensions are big and dominant, while the transverse ones contract.

• When the brane decays the opposite occurs

Page 21: Full Integrability of Supergravity Billiards: the arrow of time, asymptotic states and trapped surfaces in the cosmic evolution Lecture by Pietro Frè and

Cosmic Billiards in 2008

The billiard phenomenon is the generic feature of all exact solutions of supergravity restricted to time dependence.

We know all solutions where two scale factors are equal. In this case one-dimensional -model on the coset U/H. We proved complete integrability.

We established an integration algorithm which provides the general integral.

We discovered new properties of the moduli space of the general integral. This is the compact coset H/Gpaint , further modded by the relevant Weyl group. This is the Weyl group WTS of the Tits Satake subalgebra UTS ½ U.

There exist both trapped and (super)critical surfaces. Asymptotic states of the universe are in one-to-one correspondence with elements of WTS.

Classification of integrable supergravity billiards into a short list of universality classes.

Arrow of time. The time flow is in the direction of increasing the disorder:

Disorder is measured by the number of elementary transpositions in a Weyl group element.

Glimpses of a new cosmological entropy to be possibly interpreted in terms of superstring microstates, as it happens for the Bekenstein-Hawking entropy of black holes.

Results established by P.Frè and A.Sorin

Page 22: Full Integrability of Supergravity Billiards: the arrow of time, asymptotic states and trapped surfaces in the cosmic evolution Lecture by Pietro Frè and

Main PointsDefinition

Statement

Because t-dependentsupergravity field equationsare equivalent to thegeodesic equations fora manifold

U/H

Because U/H is alwaysmetrically equivalent toa solvable group manifold exp[Solv(U/H)]and this defines acanonical embedding

Page 23: Full Integrability of Supergravity Billiards: the arrow of time, asymptotic states and trapped surfaces in the cosmic evolution Lecture by Pietro Frè and

What is a - model ?It is a theory of maps from one manifold to another one:

World manifold W:coordinates

Target manifold M:

coordinates I

Page 24: Full Integrability of Supergravity Billiards: the arrow of time, asymptotic states and trapped surfaces in the cosmic evolution Lecture by Pietro Frè and

Starting from D=3 (D=2 and D=1, also) all the (bosonic) degrees of freedom are scalars

The bosonic Lagrangian of both Type IIA and Type IIB reduces, upon toroidal dimensional reduction from D=10 to D=3, to the gravity coupled sigma model

)16()8(8

SO

E

targetM With the target manifold being the maximally non-compact coset space

8

5

1 2 3 4 6 7

Page 25: Full Integrability of Supergravity Billiards: the arrow of time, asymptotic states and trapped surfaces in the cosmic evolution Lecture by Pietro Frè and

The discovered PrincipleThe relevant

Weyl group is that

of the Tits Satake

projection. It is

a property of a universality class

of theories.

There is an interesting topology of parameter space for the LAX EQUATION

Page 26: Full Integrability of Supergravity Billiards: the arrow of time, asymptotic states and trapped surfaces in the cosmic evolution Lecture by Pietro Frè and

The Weyl group of a Lie algebra• Is the discrete group generated by all

reflections with respect to all roots• Weyl(L) is a discrete subgroup of the

orthogonal group O(r) where r is the rank of L.

Page 27: Full Integrability of Supergravity Billiards: the arrow of time, asymptotic states and trapped surfaces in the cosmic evolution Lecture by Pietro Frè and

The mathematical ingredients Dimensional reduction to D=3 realizes the

identification SUGRA = -model on U/H The mechanism of Kac Moody extensions The solvable parametrization of non-

compact U/H The Tits Satake projection The Lax representation of geodesic

equations and the Toda flow integration algorithm

Page 28: Full Integrability of Supergravity Billiards: the arrow of time, asymptotic states and trapped surfaces in the cosmic evolution Lecture by Pietro Frè and

Full Integrability

Lax pair representation

and the integration algorithm

Page 29: Full Integrability of Supergravity Billiards: the arrow of time, asymptotic states and trapped surfaces in the cosmic evolution Lecture by Pietro Frè and

Lax Representation andIntegration Algorithm

Solvable coset

representative

Lax operator (symm.)

Connection (antisymm.)

Lax Equation

Page 30: Full Integrability of Supergravity Billiards: the arrow of time, asymptotic states and trapped surfaces in the cosmic evolution Lecture by Pietro Frè and

Parameters of the time flows

From initial data we obtain the time flow (complete integral)

Initial data are specified by a pair: an element of the non-compact CartanSubalgebra and an element of maximal compact group:

Page 31: Full Integrability of Supergravity Billiards: the arrow of time, asymptotic states and trapped surfaces in the cosmic evolution Lecture by Pietro Frè and

Properties of the flowsThe flow is isospectral

The asymptotic values of the Lax operator are diagonal (Kasner epochs)

Page 32: Full Integrability of Supergravity Billiards: the arrow of time, asymptotic states and trapped surfaces in the cosmic evolution Lecture by Pietro Frè and

Proposition

Trapped

submanifolds

ARROW OF

TIME

Parameter space

Page 33: Full Integrability of Supergravity Billiards: the arrow of time, asymptotic states and trapped surfaces in the cosmic evolution Lecture by Pietro Frè and

Example. The Weyl group of

Sp(4)» SO(2,3)

Available flows

on 3-dimensional

critical surfaces

Available flows on edges, i.e. 1-dimensional critical surfaces

Page 34: Full Integrability of Supergravity Billiards: the arrow of time, asymptotic states and trapped surfaces in the cosmic evolution Lecture by Pietro Frè and

An example of flow on a critical surface for SO(2,4).

2 , i.e. O2,1 = 0

Future

PAST

Plot of 1 ¢ h

Plot of 1 ¢ h

Future infinity is 8 (the highest Weyl group element), but at past infinitywe have 1 (not the highest) = criticality

Zoom on this region

Trajectory of the cosmic ball

Page 35: Full Integrability of Supergravity Billiards: the arrow of time, asymptotic states and trapped surfaces in the cosmic evolution Lecture by Pietro Frè and

Future

PAST

Plot of 1 ¢ h

Plot of 1 ¢ h

O2,1 ' 0.01 (Perturbation of

critical surface)

There is an extra primordial

bounce and we have the lowest Weyl group element 5 at

t = -1

Page 36: Full Integrability of Supergravity Billiards: the arrow of time, asymptotic states and trapped surfaces in the cosmic evolution Lecture by Pietro Frè and

END of this RECITALThank you for your

attention

In case of request of request…..there is encore…..

Page 37: Full Integrability of Supergravity Billiards: the arrow of time, asymptotic states and trapped surfaces in the cosmic evolution Lecture by Pietro Frè and

For subject lovers

More details on the underlying

Mathematical Structure

Page 38: Full Integrability of Supergravity Billiards: the arrow of time, asymptotic states and trapped surfaces in the cosmic evolution Lecture by Pietro Frè and

Duality Algebras

The algebraic structure of duality algebras in D<4

dimensions

Page 39: Full Integrability of Supergravity Billiards: the arrow of time, asymptotic states and trapped surfaces in the cosmic evolution Lecture by Pietro Frè and

Structure of the Duality Algebra in D=3

Universal,

comes

from Gravity

Comes from

vectors in D=4

Symplectic metric in d=2 Symplectic metric in 2n dim

Page 40: Full Integrability of Supergravity Billiards: the arrow of time, asymptotic states and trapped surfaces in the cosmic evolution Lecture by Pietro Frè and

Affine and Hyperbolic algebrasand the cosmic billiard

We do not have to stop to D=3 if we are just interested in time dependent backgrounds

We can step down to D=2 and also D=1 In D=2 the duality algebra becomes an

affine Kac-Moody algebra In D=1 the duality algebra becomes an

hyperbolic Kac Moody algebra Affine and hyperbolic symmetries are

intrinsic to Einstein gravity

(Julia, Henneaux, Nicolai, Damour)

Page 41: Full Integrability of Supergravity Billiards: the arrow of time, asymptotic states and trapped surfaces in the cosmic evolution Lecture by Pietro Frè and

N=8 E8(8)

N=6 E7(-5)

N=5 E6(-14)

N=4

SO(8,n+2)

N=3

SU(4,n+1)

Duality algebras for diverse N(Q) from D=4 to D=3

E7(7)

SO*(12)

SU(1,5)

SL(2,R)£SO(6,n)

SU(3,n) £ U(1)Z

Page 42: Full Integrability of Supergravity Billiards: the arrow of time, asymptotic states and trapped surfaces in the cosmic evolution Lecture by Pietro Frè and

What happens for D<3?

7

9

5

6

8

4

7

3

6

2

5

1

4

8

3 D

Exceptional E11- D series for N=8 give a hint

E8

Julia 1981

2

E9 = E8Æ

UD

GL(2,R)SL(2) + SL(3)

SL(5)

E4E3

SO(5,5)

E5E6E7

0

Page 43: Full Integrability of Supergravity Billiards: the arrow of time, asymptotic states and trapped surfaces in the cosmic evolution Lecture by Pietro Frè and

This extensions is affine!

UD=4

W0

The new triplet is connected to the vector root with a single line,since the SL(2)MM commutes with UD=4

2 exceptions: pure D=4 gravity and N=3 SUGRA

UD=4

W1

0

W2

0 1

The new affine triplet: (LMM0, LMM

+, LMM-)

Page 44: Full Integrability of Supergravity Billiards: the arrow of time, asymptotic states and trapped surfaces in the cosmic evolution Lecture by Pietro Frè and

N=8 E8(8)

N=6 E7(-5)

N=5 E6(-14)

N=4

SO(8,n+2)

N=3

SU(4,n+1)

D=4

E7(7)

SO*(12)

SU(1,5)

SL(2,R)£SO(6,n)

SU(3,n) £ U(1)Z

E9(9)

E7

E6

SO(8,n+2)

D=3 D=2

Page 45: Full Integrability of Supergravity Billiards: the arrow of time, asymptotic states and trapped surfaces in the cosmic evolution Lecture by Pietro Frè and

The Tits Satake projection

A fondamental ingredient

to single out the universality

classes and the relevant Weyl group

Page 46: Full Integrability of Supergravity Billiards: the arrow of time, asymptotic states and trapped surfaces in the cosmic evolution Lecture by Pietro Frè and

root system

of rank r1

ProjectionSeveral roots of the higher system have the same projection.

These are painted copies of the same wall.

The Billiard dynamics occurs in the rank r2 system

Page 47: Full Integrability of Supergravity Billiards: the arrow of time, asymptotic states and trapped surfaces in the cosmic evolution Lecture by Pietro Frè and

Two type of roots

1

2

3

Page 48: Full Integrability of Supergravity Billiards: the arrow of time, asymptotic states and trapped surfaces in the cosmic evolution Lecture by Pietro Frè and

To say it in a more detailed way:

Non split algebras arise as duality algebras in non maximal supergravities N< 8

r – split rank

Under the involutive automorphism that defines the non split real section

compact roots

non compact roots

root pairs

Non split real algebras are represented by Satake diagrams

For example, for N=6 SUGRAwe have E7(-5)

Compact simple rootsdefine a sugalgebraHpaint

Page 49: Full Integrability of Supergravity Billiards: the arrow of time, asymptotic states and trapped surfaces in the cosmic evolution Lecture by Pietro Frè and

The paint group

The subalgebra of external automorphisms:

is compact and it is the Lie algebra of the paint group

Page 50: Full Integrability of Supergravity Billiards: the arrow of time, asymptotic states and trapped surfaces in the cosmic evolution Lecture by Pietro Frè and

Paint group in diverse dimensions

The paint group survives under dimensional reduction, that adds only non-compact directions to the scalar manifold

D=3D=4

It means that the Tits Satake projection commutes with the dimensional reduction

Page 51: Full Integrability of Supergravity Billiards: the arrow of time, asymptotic states and trapped surfaces in the cosmic evolution Lecture by Pietro Frè and

The SolvableParametrization

Crucial for integrability is the remarkable relation between

non-compact cosets U/H and

Solvable Group Manifolds exp[Solv]

Page 52: Full Integrability of Supergravity Billiards: the arrow of time, asymptotic states and trapped surfaces in the cosmic evolution Lecture by Pietro Frè and

Solvable Lie Algebras: i.e. triangular matrices• What is a solvable Lie algebra A ?• It is an algebra where the derivative series ends after some steps• i.e. D[A] = [A , A] , Dk[A] = [Dk-1[A] , Dk-1[A] ]• Dn[A] = 0 for some n > 0 then A = solvable

THEOREM: All linear representations of a solvable Lie algebra admit a basis where

every element T 2 A is given by an upper triangular matrixFor instance the upper triangular matrices of this

type form a solvable subalgebra

SolvN ½ sl(N,R)

Page 53: Full Integrability of Supergravity Billiards: the arrow of time, asymptotic states and trapped surfaces in the cosmic evolution Lecture by Pietro Frè and

The solvable parametrizationThere is a fascinating theorem which provides an identification of the geometry

of moduli spaces with Lie algebras for (almost) all supergravity theories.

THEOREM: All non compact (symmetric) coset manifolds are metrically equivalent to a solvable group manifold

• There are precise rules to construct Solv(U/H)• Essentially Solv(U/H) is made by

• the non-compact Cartan generators Hi 2 CSA K and

• those positive root step operators E which are not orthogonal to the non compact Cartan subalgebra CSA K

Splitting the Lie algebra U into the maximal compact subalgebra H plus the orthogonal complement K

Page 54: Full Integrability of Supergravity Billiards: the arrow of time, asymptotic states and trapped surfaces in the cosmic evolution Lecture by Pietro Frè and

Maximally split cosets U/H U/H is maximally split if CSA = CSA K is

completelly non-compact Maximally split U/H occur if and only if SUSY

is maximal # Q =32. In the case of maximal susy we have (in D-

dimensions the E11-D series of Lie algebras

For lower supersymmetry we always have non-maximally split algebras U