The evolution of a closed Friedmann universe filled by a tachyon scalar field with a trigonometric potential and cold dark matter (CDM) is investigated. A subset of the evolutions consistent to 1σ confidence level with the Union 2.1 supernova data set is identified. The evolutions of the tachyon field are classified. Some of them evolve into a de Sitter attractor, while others proceed through a pseudo-tachyonic regime into a sudden future singularity. Critical evolutions leading to Big Brake singularities in the presence of CDM are found and a new type of cosmological evolution characterized by singularity avoidance in the pseudo-tachyon regime is presented.

Z. Horvath, Z. Keresztes, A. Kamenchtchik, L. Gergely (2015). Criticality and Big Brake singularities in the tachyonic evolutions of closed Friedmann universes with cold dark matter. PHYSICAL REVIEW D, PARTICLES, FIELDS, GRAVITATION, AND COSMOLOGY, 91, 103513-103513 [10.1103/PhysRevD.91.103513].

Criticality and Big Brake singularities in the tachyonic evolutions of closed Friedmann universes with cold dark matter

KAMENCHTCHIK, ALEXANDR;
2015

Abstract

The evolution of a closed Friedmann universe filled by a tachyon scalar field with a trigonometric potential and cold dark matter (CDM) is investigated. A subset of the evolutions consistent to 1σ confidence level with the Union 2.1 supernova data set is identified. The evolutions of the tachyon field are classified. Some of them evolve into a de Sitter attractor, while others proceed through a pseudo-tachyonic regime into a sudden future singularity. Critical evolutions leading to Big Brake singularities in the presence of CDM are found and a new type of cosmological evolution characterized by singularity avoidance in the pseudo-tachyon regime is presented.
2015
Z. Horvath, Z. Keresztes, A. Kamenchtchik, L. Gergely (2015). Criticality and Big Brake singularities in the tachyonic evolutions of closed Friedmann universes with cold dark matter. PHYSICAL REVIEW D, PARTICLES, FIELDS, GRAVITATION, AND COSMOLOGY, 91, 103513-103513 [10.1103/PhysRevD.91.103513].
Z. Horvath; Z. Keresztes; A. Kamenchtchik; L. Gergely
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Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/11585/485773
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