Quantum cosmology with a big-brake singularity

Alexander Y. Kamenshchik, Claus Kiefer, and Barbara Sandhöfer
Phys. Rev. D 76, 064032 – Published 27 September 2007

Abstract

We investigate a cosmological model with a big-brake singularity in the future: while the first time derivative of the scale factor goes to zero, its second time derivative tends to minus infinity. Although we also discuss the classical version of the model in some detail, our main interest lies in its quantization. We formulate the Wheeler-DeWitt equation and derive solutions describing wave packets. We show that all such solutions vanish in the region of the classical singularity, a behavior which we interpret as singularity avoidance. We then discuss the same situation in loop quantum cosmology. While this leads to a different factor ordering, the singularity is avoided there, too.

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  • Received 14 May 2007

DOI:https://doi.org/10.1103/PhysRevD.76.064032

©2007 American Physical Society

Authors & Affiliations

Alexander Y. Kamenshchik

  • Dipartimento di Fisica and INFN, Via Irnerio 46, 40126 Bologna, Italy
  • L. D. Landau Institute for Theoretical Physics of the Russian Academy of Sciences, Kosygin Street 2, 119334 Moscow, Russia

Claus Kiefer and Barbara Sandhöfer

  • Institut für Theoretische Physik, Universität zu Köln, Zülpicher Strasse 77, 50937 Köln, Germany

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Issue

Vol. 76, Iss. 6 — 15 September 2007

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