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Phys. Rev. D 79, 044034 (2009) [10 pages]

Cosmological wormholes

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Hideki Maeda1,*, Tomohiro Harada2,†, and B. J. Carr3,4,‡
1Centro de Estudios Científicos (CECS), Arturo Prat 514, Valdivia, Chile
2Department of Physics, Rikkyo University, Toshima, Tokyo 171-8501, Japan
3Astronomy Unit, Queen Mary, University of London, Mile End Road, London E1 4NS, United Kingdom
4Research Center for the Early Universe, Graduate School of Science, University of Tokyo, Tokyo 113-0033, Japan

Received 12 January 2009; published 26 February 2009

Motivated by the cosmological wormhole solutions obtained from our recent numerical investigations, we provide a definition of a wormhole which applies to dynamical situations. Our numerical solutions do not have timelike trapping horizons but they are wormholes in the sense that they connect two or more asymptotic regions. Although the null energy condition must be violated for static wormholes, we find that it can still be satisfied in the dynamical context. Two analytic solutions for a cosmological wormhole connecting two Friedmann universes without trapping horizons are presented.

© 2009 The American Physical Society

URL:
http://link.aps.org/doi/10.1103/PhysRevD.79.044034
DOI:
10.1103/PhysRevD.79.044034
PACS:
04.20.Gz, 04.20.Jb, 04.40.Nr

*hideki@cecs.cl

harada@rikkyo.ac.jp

B.J.Carr@qmul.ac.uk