approximation methods for the dynamics in deparametrized lqg

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Mehdi Assanioussi Faculty of Physics, University of Warsaw work in collaboration with J. Lewandowski & I. Mäkinen [arXiv:1702.01688] Fifth Tux workshop on QG Tux, Feb 2017 Approximation methods for the dynamics in Deparametrized LQG

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Mehdi Assanioussi

Faculty of Physics, University of Warsaw

work in collaboration with J. Lewandowski & I. Mäkinen

[arXiv:1702.01688]

Fifth Tux workshop on QG

Tux, Feb 2017

Approximation methods for the

dynamics in Deparametrized LQG

Plan of the talk

I. LQG deparametrized models

II. Physical Hamiltonian operators

III. Approximation methods for the dynamics

i. Expansion: Hamiltonian op. / Evolution op.

ii. Examples

IV. Summary & outlook

LQG deparametrized models

LQG deparametrized models

Motivation

1

• Test-ground for LQG quantization methods

• Insights on the continuum limit of LQG

• Insights on the dynamics of Matter fields in presence of QG

LQG deparametrized models

• Complete quantum gravity models:

* Physical Hilbert space

* Admissible Hamiltonian operator

• Computable dynamics (time evolution)

Motivation

1

• Test-ground for LQG quantization methods

• Insights on the continuum limit of LQG

• Insights on the dynamics of Matter fields in presence of QG

First steps…

LQG deparametrized models

Deparametrization Matter fields as coordinates

2

LQG deparametrized models

Massless K.G. scalar field Non-rotational dust

Deparametrization Matter fields as coordinates

e.g: time ref. mod.

2

Deparametrization

LQG deparametrized models

Time ref. models

Spacetime ref.

models

3

Deparametrization

LQG deparametrized models

Time ref. models

Spacetime ref.

models

Successful

Unsuccessful

3

Deparametrization

LQG deparametrized models

Time ref. models

Spacetime ref.

models

Successful

Unsuccessful

Depends…

Successful

3

Deparametrization

LQG deparametrized models

Time ref. models

Spacetime ref.

models

Successful

Unsuccessful

Depends…

Successful

3

LQG deparametrized models

Massless K.G. scalar field Non-rotational dust

e.g: time ref. mod.

4

LQG deparametrized models

Massless K.G. scalar field Non-rotational dust

e.g: time ref. mod.

4

Physical Hilbert space:

LQG deparametrized models

Massless K.G. scalar field Non-rotational dust

e.g: time ref. mod.

4

Proper implementation of the functional C

* Self-adjoint Hamiltonian operator

* Spatial diffeomorphism invariant

* Computable dynamics

Physical Hilbert space:

Physical Hamiltonian operators

Physical Hamiltonian operators

Scalar constraint functional

5

Immirzi-Barbero

parameter

Physical Hamiltonian operators

Scalar constraint functional

Lorentzian part

(Curvature operator)

Euclidean part

(Euclidean operator)

5

Immirzi-Barbero

parameter

Physical Hamiltonian operators

Scalar constraint functional

Lorentzian part

(Curvature operator)

Euclidean part

(Euclidean operator)

Constructing the operator on

5

Immirzi-Barbero

parameter

Physical Hamiltonian operators

Curvature operator

(Regge calculus)

6

Physical Hamiltonian operators

Curvature operator

(Regge calculus)

6

Physical Hamiltonian operators

Euclidean operator

7

Physical Hamiltonian operators

Euclidean operator

Regularization

7

Physical Hamiltonian operators

Euclidean operator

Regularization

Moving to :

7

Physical Hamiltonian operators

8

Physical Hamiltonian operators

Properties

• The curvature op. preserves the graphs;

• The Euclidean op. removes loops from the graphs;

• SU(2) gauge inv. & spatial diff. covariant ;

• Anomaly-free;

8

Physical Hamiltonian operators

Properties

• The curvature op. preserves the graphs;

• The Euclidean op. removes loops from the graphs;

• SU(2) gauge inv. & spatial diff. covariant ;

• Anomaly-free;

8

Physical Hamiltonian operators

Properties

• The curvature op. preserves the graphs;

• The Euclidean op. removes loops from the graphs;

• SU(2) gauge inv. & spatial diff. covariant ;

• Anomaly-free;

• Existence of symmetric extensions (self-adjoint?);

• Domain decomposes into stable separable sub-spaces;

8

Approximation methods for the dynamics

Approximation methods for the dynamics

Dynamics

9

Approximation methods for the dynamics

Dynamics

• Transition amplitudes:

• Quantum observables:

9

Approximation methods for the dynamics

Dynamics

• Transition amplitudes:

• Quantum observables:

• Expansion of the evolution operator:

9

Approximation methods for the dynamics

10

Dynamics

Approximation methods for the dynamics

• Perturbation theory for the Hamiltonian op.:

10

Dynamics

Approximation methods for the dynamics

• Perturbation theory for the Hamiltonian op.:

10

Dynamics Self-adjointSymmetric

Approximation methods for the dynamics

• Perturbation theory for the Hamiltonian op.:

10

Dynamics Self-adjointSymmetric

Approximation methods for the dynamics

Concretely? For what range of β?

11

Approximation methods for the dynamics

Concretely? For what range of β?

Examples:

11

Evolution of volume & curvature expectation values

Approximation methods for the dynamics

Concretely? For what range of β?

Examples:

11

• initial states = eigenvectors of volume (4-valent vertex)

Evolution of volume & curvature expectation values

Approximation methods for the dynamics

Concretely? For what range of β?

Examples:

11

• initial states = eigenvectors of volume (4-valent vertex)

• β-expansion is taken up to 2nd

order:

Evolution of volume & curvature expectation values

Approximation methods for the dynamics

Concretely? For what range of β?

Examples:

11

• initial states = eigenvectors of volume (4-valent vertex)

• β-expansion is taken up to 2nd

order:

• time-expansion is taken up to 4th

order:

Evolution of volume & curvature expectation values

Approximation methods for the dynamics

Scalar field model in examples

12

j=2 j=10

Approximation methods for the dynamics

Scalar field model in examples

12

Periodic evolution at 0th

order

j=2 j=10

Approximation methods for the dynamics

Dust field model in examples

13

j=10j=10

Approximation methods for the dynamics

Dust field model in examples

14

j=10j=2

Summary & outlook

Summary & outlook

Deparametrized models:

Symmetric Hamiltonian operators

Approximation method (pert. th.) for the Hamiltonian op.:

* treatment of the square root in the SF model

* explicit computation of dynamics

Self-adjointness proofs

Identification & interpretation of relevant physical states

Include Standard Model

Summary & outlook

Deparametrized models:

Symmetric Hamiltonian operators

Approximation method (pert. th.) for the Hamiltonian op.:

* treatment of the square root in the SF model

* explicit computation of dynamics

Self-adjointness proofs

Identification & interpretation of relevant physical states

Include Standard Model