corner
corner

Phys. Rev. Lett. 92, 061301 (2004) [4 pages]

On the “Causality Argument” in Bouncing Cosmologies

Download: PDF (108 kB) Buy this article Export: BibTeX or EndNote (RIS)

Jérôme Martin* and Patrick Peter
Institut d’Astrophysique de Paris, GReCO, FRE 2435-CNRS, 98bis Boulevard Arago, 75014 Paris, France

Received 8 July 2003; published 10 February 2004

We exhibit a situation in which cosmological perturbations of astrophysical relevance propagating through a bounce are affected in a scale-dependent way. Involving only the evolution of a scalar field in a closed universe described by general relativity, the model is consistent with causality. Such a specific counterexample leads to the conclusion that imposing causality is not sufficient to determine the spectrum of perturbations after a bounce provided it is known before. We discuss consequences of this result for string motivated scenarios.

© 2004 The American Physical Society

URL:
http://link.aps.org/doi/10.1103/PhysRevLett.92.061301
DOI:
10.1103/PhysRevLett.92.061301
PACS:
98.80.Cq

*Electronic address: jmartin@iap.fr

Electronic address: peter@iap.fr