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Inflation and dark energy from the Brans-Dicke theory

2014/12/27 by Michal Artymowski, Artymowski, Michal, Zygmunt Lalak +3
Physics and Astronomy · #FOS: Physical sciences #General Relativity and Quantum Cosmology (gr-qc) #High Energy Physics - Theory (hep-th) #gr-qc #hep-th

paper · pdf · doi:10.48550/arxiv.1412.8075

14 pages, 5 figures. arXiv admin note: substantial text overlap with arXiv:1405.7818

arxiv created 2014/12/27 · arxiv updated 2014/12/30

Abstract

We consider the Brans-Dicke theory motivated by the f(R) = R + αRn - βR2-n model to obtain a stable minimum of the Einstein frame scalar potential of the Brans-Dicke field. As a result we have obtained an inflationary scalar potential with non-zero value of residual vacuum energy, which may be a source of Dark Energy. In addition we discuss the probability of quantum tunnelling from the minimum of the potential. Our results can be easily consistent with PLANCK or BICEP2 data for appropriate choices of the value of n and ω.

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