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Photon propagation in quantum gravity

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Title: Photon propagation in quantum gravity


1
Photon propagation in quantum gravity
  • A tool to test Lorentz Invariance
  • R. Gleiser, C. Kozameh, F. Parisi

2
Physics at the end of the XIX century
  • Lord Kelvin reflecting on the status of physics.
  • I am lucky to have seen all the major
    accomplishments in Physics!
  • Maxwells theory to explain the ondulatory
    nature of light.
  • Newtons theory to explain celestial motion.
  • Thermodynamics to explain the behavior of
    systems.
  • All that is left is to solve specific problems.
  • Small problem lack of invariance of Maxwell
    theory under the Galilean group. It was thought
    the equations were valid on a reference frame at
    rest with respect to the ether. The Michelson
    Morley experiment was designed to measure the
    speed of the earth with respect to the ether.

3
Einsteins five papers of 1905
  • "On a heuristic viewpoint concerning the
    production and transformation of light."
  • (light quantum/photoelectric effect) (17 March
    1905)Annalen der Physik, 17(1905), pp. 132-148.
  • "A New Determination of Molecular Dimensions"
    (Doctoral dissertation) (30 April 1905).
  • Annalen der Physik, 19 (1906), pp. 289-305.
  • "On the motion of small particles suspended in
    liquids at rest required by the molecular-kinetic
    theory of heat." (Brownian motion paper) (11 May
    1905)Annalen der Physik, 17 (1905), pp. 549-560.

4
Einsteins five papers of 1905
  • " On the electrodynamics of moving bodies"
  • (Special relativity) (30 June 1905) Annalen der
    Physik, 17 (1905), pp. 891-921.
  • " Does the inertia of a body depend on its energy
    content?"
  • (Emc2) (27 September 1905).
  • Annalen der Physik, 18 (1905), pp. 639-641.

5
Einsteins fourth miraculous paper
  • Lorentz invariance is arguably the most
    fundamental principle in Physics.
  • In 1905, Albert Einstein, inspired by the
    Michelson and Morley's experiment, presented his
    theory of special relativity and redefined our
    notion of space, time and gravity.

6
Einsteins fourth miraculous paper
  • Today physicists are doing reruns of old
    experiments with extraordinary precision testing
    the constancy of the speed of light. NatureĀ 427,
    482 - 484 (2004)
  • Recent claims coming from the two leading
    candidates for a quantum theory of gravity
    challenge this basic symmetry.
  • Their predictions could be observed with present
    level of technology.
  • If true, there would have to be a mayor revision
    of our understanding of the physical processes.
  • In this talk we review these claims and show that
    Lorentz invariance is preserved.

7
Possible Lorentz violating effects
  • Superstrings. Very energetic photons interact
    with the quantum structure of the space-time.
    Consequence their speed is lower than that of
    less energetic photons. G. Amelio-Camelia, et al,
    Nature 393, 793 (1998).
  • Loop Quantum Gravity. Left and right helicity
    photons travel at different speeds.
  • R. Gambini, J. Pullin, Phys. Rev. D 59, 124021
    (1999).

8
Possible Lorentz violating effects
  • Photons emitted simultaneously will separate as
    they travel through space. Time delay seen by
    observer
  • Physical processes
  • will mask this effect.
  • Unlikely to be observed

9
Another Lorentz violating effect.
  • For linearly polarized photons the polarization
    direction depends on the energy of the photon.
  • R. Gleiser, C. Kozameh, Phys. Rev. D 59, 124021
    (2001).
  • This effect has been used to set an upper bound
    for visible light and for
    gamma rays.

10
Is Lorentz invariance violated?
  • None of these predicted effects have been
    observed. Is Lorentz invariance really violated
    at the order of approximation of these
    calculations?
  • Superstring model difficult to follow.
    Nevertheless the dispersion relation arises from
    the equation
  • where vi is the speed of the receding string.
  • This equation says that any photon follows the
    same null geodesic regardless of its energy.

11
Coupling radiation fields with gravity
  • The loop quantum gravity model has a more
    standard approach. It is thus worth reviewing the
    relevant fields involved in this interaction
  • Classical theory Lagrangian and Hamiltonian
    formulation
  • Quantum theory the quantum operators.
  • Semiclassical approximation
  • - Effective interaction Hamiltonian.
  • - Field equations

12
Classical source-free Maxwell fields
  • Maxwell field
  • Lagrangian density
  • Euler-Lagrange equation
  • Local (t, xa) coords.

13
Hamiltonian formulation
  • Conjugate momentum to Aa
  • Hamiltonian density
  • Hamilton equations

14
The quantum operators and states
  • The quantum operators are
  • where the canonical pairs satisfy the c.c.r.
  • The Hamiltonian density operator reads
  • The semiclassical states

15
The effective Hamiltonian
  • Taking expectation values of H with semiclassical
    states
  • Or, using vectorial notation
  • with

16
The field equations
  • The Hamilton equations of motion yield
  • which means that either satisfy the
    wave equation
  • C. Kozameh, F. Parisi, Class. Quantum Grav.
    (2004).

17
Summary of results
  • Lorentz invariance is preserved by the
    interaction between photons and quantum gravity
    states at a semiclassical approximation.
  • Results extend to any gravitational state with
    rotational invariance.
  • Any violation must appear at a higher order, i.e.
    when we consider the back reaction to the metric.
  • Preliminary results indicate that this non
    lorentzian term oscilates around a Lorentz
    preserving dispersion relation.
  • Details will be presented at the next
    commemoration conference.
  • .
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