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Phys. Rev. D 79, 083504 (2009) [8 pages]

Tachyon cosmology, supernovae data, and the big brake singularity

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Z. Keresztes
Department of Theoretical Physics, University of Szeged, Tisza Lajos krt 84-86, Szeged 6720, Hungary
Department of Experimental Physics, University of Szeged, Dóm Tér 9, Szeged 6720, Hungary

L. Á. Gergely
Department of Theoretical Physics, University of Szeged, Tisza Lajos krt 84-86, Szeged 6720, Hungary
Department of Experimental Physics, University of Szeged, Dóm Tér 9, Szeged 6720, Hungary
Department of Applied Science, London South Bank University, 103 Borough Road, London SE1 OAA, United Kingdom

V. Gorini and U. Moschella
Dipartimento di Scienze Fisiche e Mathematiche, Università dell’Insubria, Via Valleggio 11, 22100 Como, Italy
INFN, sezione di Milano, Via Celoria 16, 20133 Milano, Italy

A. Yu. Kamenshchik
Dipartimento di Fisica and INFN, via Irnerio 46, 40126 Bologna, Italy
L. D. Landau Institute for Theoretical Physics, Russian Academy of Sciences, Kosygin street 2, 119334 Moscow, Russia

Received 15 January 2009; published 6 April 2009

We compare the existing observational data on type Ia supernovae with the evolutions of the Universe predicted by a one-parameter family of tachyon models which we have introduced recently [ Phys. Rev. D 69 123512 (2004)]. Among the set of the trajectories of the model which are compatible with the data there is a consistent subset for which the Universe ends up in a new type of soft cosmological singularity dubbed big brake. This opens up yet another scenario for the future history of the Universe besides the one predicted by the standard ΛCDM model.

© 2009 The American Physical Society

URL:
http://link.aps.org/doi/10.1103/PhysRevD.79.083504
DOI:
10.1103/PhysRevD.79.083504
PACS:
98.80.Cq, 98.80.Jk, 98.80.Es, 95.36.+x

See Also

See Also: Zoltán Keresztes, László Á. Gergely, Alexander Yu. Kamenshchik, Vittorio Gorini, and David Polarski, Will the tachyonic universe survive the big brake?, Phys. Rev. D 82, 123534 (2010).