Gauge invariance in loop quantum cosmology: Hamilton-Jacobi and Mukhanov-Sasaki equations for scalar perturbations

Thomas Cailleteau and Aurelien Barrau
Phys. Rev. D 85, 123534 – Published 20 June 2012

Abstract

Gauge invariance of scalar perturbations is studied together with the associated equations of motion. Extending the methods developed in Hamiltonian general relativity, the Hamilton-Jacobi equation is investigated into the details in the framework of loop quantum gravity. The gauge-invariant observables are built, and their equations of motions are reviewed both in the Hamiltonian and Lagrangian approaches. This method is applied to scalar perturbations with either holonomy or inverse-volume corrections.

  • Received 30 January 2012

DOI:https://doi.org/10.1103/PhysRevD.85.123534

© 2012 American Physical Society

Authors & Affiliations

Thomas Cailleteau and Aurelien Barrau

  • Laboratoire de Physique Subatomique et de Cosmologie, UJF, CNRS/IN2P3, INPG 53, av. des Martyrs, 38026 Grenoble cedex, France

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Issue

Vol. 85, Iss. 12 — 15 June 2012

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