Effective constraints of loop quantum gravity

Martin Bojowald, Mikhail Kagan, Hector H. Hernández, and Aureliano Skirzewski
Phys. Rev. D 75, 064022 – Published 19 March 2007

Abstract

Within a perturbative cosmological regime of loop quantum gravity corrections to effective constraints are computed. This takes into account all inhomogeneous degrees of freedom relevant for scalar metric modes around flat space and results in explicit expressions for modified coefficients and of higher order terms. It also illustrates the role of different scales determining the relative magnitude of corrections. Our results demonstrate that loop quantum gravity has the correct classical limit, at least in its sector of cosmological perturbations around flat space, in the sense of perturbative effective theory.

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  • Received 5 December 2006

DOI:https://doi.org/10.1103/PhysRevD.75.064022

©2007 American Physical Society

Authors & Affiliations

Martin Bojowald* and Mikhail Kagan

  • Institute for Gravitational Physics and Geometry, The Pennsylvania State University, 104 Davey Lab, University Park, Pennsylvania 16802, USA

Hector H. Hernández and Aureliano Skirzewski§

  • Max-Planck-Institut für Gravitationsphysik, Albert-Einstein-Institut, Am Mühlenberg 1, D-14476 Potsdam, Germany

  • *Electronic address: bojowald@gravity.psu.edu
  • Electronic address: mak411@psu.edu
  • Electronic address: hehe@aei.mpg.de
  • §Electronic address: skirz@aei.mpg.de

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Issue

Vol. 75, Iss. 6 — 15 March 2007

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