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Phys. Rev. Lett. 102, 081301 (2009) [4 pages]

Cosmological Footprints of Loop Quantum Gravity

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J. Grain*
AstroParticule et Cosmologie, Université Paris 7, CNRS, IN2P3 10, rue Alice Domon et Léonie Duquet, 75205 Paris cedex 13, France
Institut d’Astrophysique Spatiale, Université Paris-Sud 11, CNRS, Bâtiments 120–121, 91405 Orsay cedex, France

A. Barrau
Laboratoire de Physique Subatomique et de Cosmologie, UJF, INPG, CNRS, IN2P3 53, avenue des Martyrs, 38026 Grenoble cedex, France
Institut des Hautes Etudes Scientifiques, 35, route de Chartres, 91440 Bures-sur-Yvette, France

Received 1 September 2008; published 26 February 2009

The primordial spectrum of cosmological tensor perturbations is considered as a possible probe of quantum gravity effects. Together with string theory, loop quantum gravity is one of the most promising frameworks to study quantum effects in the early universe. We show that the associated corrections should modify the potential seen by gravitational waves during the inflationary amplification. The resulting power spectrum should exhibit a characteristic tilt. This opens a new window for cosmological tests of quantum gravity.

© 2009 The American Physical Society

URL:
http://link.aps.org/doi/10.1103/PhysRevLett.102.081301
DOI:
10.1103/PhysRevLett.102.081301
PACS:
04.60.Bc, 04.60.Pp, 98.80.Cq, 98.80.Qc

*grain@apc.univ-paris7.fr

aurelien.barrau@cern.ch