first order gravity on the light front

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First order gravity on the light front Sergei Alexandrov Laboratoire Charles Coulomb Montpellier work in progress with Simone Speziale

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Page 1: First order gravity on the light front

First order gravity

on the light front

Sergei Alexandrov

Laboratoire Charles Coulomb Montpellier

work in progress with Simone Speziale

Page 2: First order gravity on the light front

Light Front Light cone coordinates:

Page 3: First order gravity on the light front

Light Front Light cone coordinates:

Main features:

• Triviality of the vacuum

– energy

– momentum

Page 4: First order gravity on the light front

Light Front Light cone coordinates:

Main features:

• Triviality of the vacuum

– energy

– momentum

• Non-trivial physics of zero modes

Page 5: First order gravity on the light front

Light Front Light cone coordinates:

Main features:

• Triviality of the vacuum

– energy

– momentum

• Non-trivial physics of zero modes

• Importance of boundary conditions at

Page 6: First order gravity on the light front

Light Front Light cone coordinates:

Main features:

• Triviality of the vacuum

– energy

– momentum

linear in velocities

• Presence of second class constraints

• Non-trivial physics of zero modes

• Importance of boundary conditions at

Page 7: First order gravity on the light front

Null surfaces are natural in gravity (Penrose,…)

Gravity on the light front

null vectors

• Sachs(1962) – constraint free formulation

• conformal metrics on

• intrinsic geometry of

• extrinsic curvature of

• Reisenberger – symplectic structure on

the constraint free data

null foliation

Page 8: First order gravity on the light front

Null surfaces are natural in gravity (Penrose,…)

Gravity on the light front

null vectors

• Torre(1986) – canonical formulation in the metric formalism

• Goldberg,Robinson,Soteriou(1991) – canonical formulation in the complex Ashtekar variables

• Inverno,Vickers(1991) – canonical formulation in the complex Ashtekar variables adapted to the double null foliation

Constraint algebra

becomes a Lie algebra

• Sachs(1962) – constraint free formulation

• conformal metrics on

• intrinsic geometry of

• extrinsic curvature of

• Reisenberger – symplectic structure on

the constraint free data

null foliation

Page 9: First order gravity on the light front

Null surfaces are natural in gravity (Penrose,…)

Gravity on the light front

null vectors

• Torre(1986) – canonical formulation in the metric formalism

• Goldberg,Robinson,Soteriou(1991) – canonical formulation in the complex Ashtekar variables

• Inverno,Vickers(1991) – canonical formulation in the complex Ashtekar variables adapted to the double null foliation

Constraint algebra

becomes a Lie algebra

• Veneziano et al. (recent) – light-cone averaging in cosmology

• Sachs(1962) – constraint free formulation

• conformal metrics on

• intrinsic geometry of

• extrinsic curvature of

• Reisenberger – symplectic structure on

the constraint free data

null foliation

Page 10: First order gravity on the light front

Motivation

Can the light front formulation be useful in quantum gravity (black holes, spin foams…)?

Page 11: First order gravity on the light front

Motivation

– was not analyzed yet • One needs the real first order formulation on the light front

Can the light front formulation be useful in quantum gravity (black holes, spin foams…)?

Page 12: First order gravity on the light front

Motivation

Exact path integral (still to be defined)

– was not analyzed yet • One needs the real first order formulation on the light front

Can the light front formulation be useful in quantum gravity (black holes, spin foams…)?

• Can one find constraint free data in the first order formulation? (preferably without using double null foliation)

Page 13: First order gravity on the light front

Motivation

Exact path integral (still to be defined)

– was not analyzed yet • One needs the real first order formulation on the light front

• The issue of zero modes in gravity was not studied yet

Can the light front formulation be useful in quantum gravity (black holes, spin foams…)?

• Can one find constraint free data in the first order formulation? (preferably without using double null foliation)

Page 14: First order gravity on the light front

Motivation

Exact path integral (still to be defined)

– was not analyzed yet • One needs the real first order formulation on the light front

• The issue of zero modes in gravity was not studied yet

Can the light front formulation be useful in quantum gravity (black holes, spin foams…)?

• Can one find constraint free data in the first order formulation? (preferably without using double null foliation)

• In the first order formalism the null condition can be controlled

by fields in the tangent space

Page 15: First order gravity on the light front

Technical motivation

3+1 decomposition of the tetrad

Used in various approaches to quantum gravity (covariant LQG, spin foams…)

Page 16: First order gravity on the light front

Technical motivation

3+1 decomposition of the tetrad

Used in various approaches to quantum gravity (covariant LQG, spin foams…)

lapse

shift

spatial metric

Page 17: First order gravity on the light front

Technical motivation

3+1 decomposition of the tetrad

determines the nature of the foliation

spacelike spacelike lightlike timelike

Used in various approaches to quantum gravity (covariant LQG, spin foams…)

lapse

shift

spatial metric

Page 18: First order gravity on the light front

Technical motivation

3+1 decomposition of the tetrad

determines the nature of the foliation

spacelike spacelike lightlike timelike

light front formulation

Used in various approaches to quantum gravity (covariant LQG, spin foams…)

What happens at ?

lapse

shift

spatial metric

Page 19: First order gravity on the light front

Technical motivation

3+1 decomposition of the tetrad

Perform canonical analysis for the real first order

formulation of general relativity on a lightlike foliation

determines the nature of the foliation

spacelike spacelike lightlike timelike

light front formulation

Used in various approaches to quantum gravity (covariant LQG, spin foams…)

What happens at ?

lapse

shift

spatial metric

Page 20: First order gravity on the light front

1. Canonical formulation of field theories on the light front

2. A review of the canonical structure of first order gravity

3. Canonical analysis of first order gravity on the light front

4. The issue of zero modes

Plan of the talk

Page 21: First order gravity on the light front

Massless scalar field in 2d

Solution:

Page 22: First order gravity on the light front

Massless scalar field in 2d

Solution:

Primary constraint Hamiltonian

Light front formulation

Page 23: First order gravity on the light front

Massless scalar field in 2d

Solution:

Primary constraint Hamiltonian

Stability condition:

is of second class

Light front formulation

Page 24: First order gravity on the light front

Massless scalar field in 2d

Solution:

Primary constraint Hamiltonian

Stability condition:

is of second class

zero mode

first class

Identification:

Light front formulation

Page 25: First order gravity on the light front

Massless scalar field in 2d

Solution:

Primary constraint Hamiltonian

Stability condition:

is of second class

zero mode

first class

Identification:

• the phase space is one-dimensional • the lost dimension is encoded in the Lagrange multiplier

Conclusions:

Light front formulation

Page 26: First order gravity on the light front

Massive theories

One generates the same constraint but different Hamiltonian

Page 27: First order gravity on the light front

Massive theories

One generates the same constraint but different Hamiltonian

inhomogeneous equation

Stability condition:

Page 28: First order gravity on the light front

Massive theories

One generates the same constraint but different Hamiltonian

inhomogeneous equation

Stability condition:

The existence of the zero mode contradicts to the natural boundary

conditions

Page 29: First order gravity on the light front

Massive theories

One generates the same constraint but different Hamiltonian

In massive theories the light front constraints do not have first class zero modes

inhomogeneous equation

Stability condition:

The existence of the zero mode contradicts to the natural boundary

conditions

Page 30: First order gravity on the light front

Massive theories

One generates the same constraint but different Hamiltonian

In massive theories the light front constraints do not have first class zero modes

inhomogeneous equation

Stability condition:

The existence of the zero mode contradicts to the natural boundary

conditions

In higher dimensions:

behave like massive 2d case

Page 31: First order gravity on the light front

Dimensionality of the phase space

On the light front

dim. phase space = num. of deg. of freedom

Page 32: First order gravity on the light front

Dimensionality of the phase space

On the light front

dim. phase space = num. of deg. of freedom

Fourier decompositions

Page 33: First order gravity on the light front

Dimensionality of the phase space

On the light front

dim. phase space = num. of deg. of freedom

Second class constraint

Symplectic structure is non-degenerate

Dirac bracket

Fourier decompositions

Page 34: First order gravity on the light front

First order gravity (spacelike case)

Fix – normal to the foliation

Canonical variables:

Page 35: First order gravity on the light front

First order gravity (spacelike case)

Fix – normal to the foliation

Canonical variables:

Linear simplicity constraints

Page 36: First order gravity on the light front

First order gravity (spacelike case)

Fix – normal to the foliation

Canonical variables:

Linear simplicity constraints

Hamiltonian is a linear combination of constraints

Page 37: First order gravity on the light front

First order gravity (spacelike case)

Fix – normal to the foliation

Canonical variables:

Linear simplicity constraints

Hamiltonian is a linear combination of constraints

3 6

Page 38: First order gravity on the light front

First order gravity (spacelike case)

Fix – normal to the foliation

Canonical variables:

Linear simplicity constraints

Hamiltonian is a linear combination of constraints

3 6

secondary constraints

Page 39: First order gravity on the light front

First order gravity (spacelike case)

Fix – normal to the foliation

Canonical variables:

Linear simplicity constraints

Hamiltonian is a linear combination of constraints

3 6

secondary constraints

1st class

2d class

Page 40: First order gravity on the light front

First order gravity (spacelike case)

Fix – normal to the foliation

Canonical variables:

Linear simplicity constraints

Hamiltonian is a linear combination of constraints

3 6

secondary constraints

dim. of phase space = 2×18 – 2(3+3+1)-(3+9+6)=4

1st class

2d class

Page 41: First order gravity on the light front

Cartan equations

Cartan equations

Page 42: First order gravity on the light front

Cartan equations

Cartan equations

do not contain time

derivatives and Lagrange multipliers

12 constraints

Page 43: First order gravity on the light front

Cartan equations

Cartan equations

do not contain time

derivatives and Lagrange multipliers

12 constraints

for fixed do not contain

time derivatives

Page 44: First order gravity on the light front

Cartan equations

Cartan equations

do not contain time

derivatives and Lagrange multipliers

12 constraints

for fixed do not contain

time derivatives

fix 3 components of

( – 2d class)

Page 45: First order gravity on the light front

Cartan equations

Cartan equations

do not contain time

derivatives and Lagrange multipliers

12 constraints

for fixed do not contain

time derivatives

fix 3 components of

( – 2d class)

fix 2 components of and the lapse

Page 46: First order gravity on the light front

Cartan equations

Cartan equations

do not contain time

derivatives and Lagrange multipliers

12 constraints

for fixed do not contain

time derivatives

We expect that the Hamiltonian constraint becomes second class

fix 3 components of

( – 2d class)

fix 2 components of and the lapse

Page 47: First order gravity on the light front

Hamiltonian analysis on the light front

Light front condition

Canonical variables:

Linear simplicity constraints

Page 48: First order gravity on the light front

Hamiltonian analysis on the light front

Light front condition

Canonical variables:

Linear simplicity constraints

Page 49: First order gravity on the light front

Hamiltonian analysis on the light front

Light front condition

Canonical variables:

Linear simplicity constraints

Hamiltonian is a linear combination of constraints

where

Page 50: First order gravity on the light front

Hamiltonian analysis on the light front

Light front condition

Canonical variables:

Linear simplicity constraints

2 7

Hamiltonian is a linear combination of constraints

where

Page 51: First order gravity on the light front

Hamiltonian analysis on the light front

Light front condition

Canonical variables:

Linear simplicity constraints

2 7

Hamiltonian is a linear combination of constraints

where

secondary constraints

equation fixing the lapse +

Page 52: First order gravity on the light front

Tertiary constraints The crucial observation:

has 2 null eigenvectors

induced metric

on the foliation

and

Page 53: First order gravity on the light front

Tertiary constraints The crucial observation:

has 2 null eigenvectors

induced metric

on the foliation

and

There are two

tertiary constraints

Projector on the

null eigenvectors

Page 54: First order gravity on the light front

Tertiary constraints The crucial observation:

has 2 null eigenvectors

induced metric

on the foliation

and

Stabilization procedure stops due to

There are two

tertiary constraints

Projector on the

null eigenvectors

Page 55: First order gravity on the light front

Summary

List of constraints:

Gauss

preserving

Gauss

rotating

spatial

diffeos Hamiltonian

primary

simplicity secondary simplicity

tertiary

Page 56: First order gravity on the light front

Summary

List of constraints:

Gauss

preserving

4

Gauss

rotating

spatial

diffeos Hamiltonian

primary

simplicity secondary simplicity

tertiary

First class Second class

3 2 1 9 6 2

Page 57: First order gravity on the light front

2 1 4 2

2 4

Summary

List of constraints:

Gauss

preserving

4

Gauss

rotating

spatial

diffeos Hamiltonian

primary

simplicity secondary simplicity

tertiary

First class Second class

3 2 1 2

Lie algebra

Page 58: First order gravity on the light front

2 1 4 2

2 4

Summary

List of constraints:

Gauss

preserving

4

Gauss

rotating

spatial

diffeos Hamiltonian

primary

simplicity secondary simplicity

tertiary

First class Second class

3 2 1 2

dim. of phase space = 2×18 – 2(4+3)-(2+1+9+6+2)=2

as it should be on the light front

Lie algebra

Page 59: First order gravity on the light front

Zero modes

The zero modes of constraints are

determined by equations fixing Lagrange multipliers

Page 60: First order gravity on the light front

Zero modes

The zero modes of constraints are

determined by equations fixing Lagrange multipliers

Potential first class constraints:

Page 61: First order gravity on the light front

Zero modes

The zero modes of constraints are

determined by equations fixing Lagrange multipliers

Potential first class constraints:

homogeneous equations

Page 62: First order gravity on the light front

Zero modes

The zero modes of constraints are

determined by equations fixing Lagrange multipliers

Potential first class constraints:

homogeneous equations

Page 63: First order gravity on the light front

Conjecture

A zero mode can exist only if the corresponding Lagrange multiplier satisfies

a homogeneous equation

One may expect only two zero modes

In our case there are two homogenous equations for and

Page 64: First order gravity on the light front

Conjecture

A zero mode can exist only if the corresponding Lagrange multiplier satisfies

a homogeneous equation

One may expect only two zero modes

In our case there are two homogenous equations for and

Gravity behaves like

2d massless theory

exist

Page 65: First order gravity on the light front

Conjecture

A zero mode can exist only if the corresponding Lagrange multiplier satisfies

a homogeneous equation

One may expect only two zero modes

In our case there are two homogenous equations for and

Gravity behaves like

2d massless theory

exist

Initial data on one null hypersurface fix

the solution

do not exist

Page 66: First order gravity on the light front

Open problems

• Do the zero modes in gravity really exist? If yes, what is the geometric meaning of the zero modes? • What are the appropriate boundary conditions along ? • How do singularities appear in this formalism?

• Can one solve (at least formally) all constraints?

• What is the right symplectic structure (Dirac bracket)?

• Can this formulation be applied to quantum gravity problems?