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JOURNALS // Teoreticheskaya i Matematicheskaya Fizika // Archive

TMF, 2012 Volume 173, Number 3, Pages 441–452 (Mi tmf8333)

This article is cited in 2 papers

Phantom dark energy with tachyonic instability: Metric perturbations

A. V. Serghienkoabc, V. A. Rubakovcb

a Demidov Yaroslavl State University, Yaroslavl, Russia
b Lomonosov Moscow State University, Moscow, Russia
c Institute for Nuclear Research, RAS, Moscow, Russia

Abstract: We study the evolution of metric perturbations in a model of UV-stable phantom dark energy. The model has tachyon instabilities at long wavelengths. We find that like the tachyon modes themselves, metric perturbations grow exponentially in time, starting from very small values determined by vacuum fluctuations, and may become sizeable at late times. We derive a constraint on the model parameters that follows from requiring that the metric perturbation amplitudes not be exceedingly large today.

Keywords: phantom, tachyon, metric perturbation.

Received: 12.03.2012

DOI: 10.4213/tmf8333


 English version:
Theoretical and Mathematical Physics, 2012, 173:3, 1709–1719

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