Gauss–Bonnet dark energy on Hořava–Lifshitz cosmology

Abstract We investigate the Gauss–Bonnet dark energy model and its deformed version on Hořava–Lifshitz cosmology, which belongs to the class of cosmologies obtained from the so-called projectable version of Hořava–Lifshitz gravity. In particular, we investigate the bulk/boundary interaction in this...

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Main Authors: Samuel Lepe, Giovanni Otalora
Format: Article
Language:English
Published: SpringerOpen 2018-04-01
Series:European Physical Journal C: Particles and Fields
Online Access:http://link.springer.com/article/10.1140/epjc/s10052-018-5822-0
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author Samuel Lepe
Giovanni Otalora
author_facet Samuel Lepe
Giovanni Otalora
author_sort Samuel Lepe
collection DOAJ
description Abstract We investigate the Gauss–Bonnet dark energy model and its deformed version on Hořava–Lifshitz cosmology, which belongs to the class of cosmologies obtained from the so-called projectable version of Hořava–Lifshitz gravity. In particular, we investigate the bulk/boundary interaction in this scenario through the Q function, which we interpret as a measure of the energy transference between the bulk and the spacetime boundary. Then we discuss whether the thermal equilibrium will be stable or not, once it is reached, and the validity of the generalized second law. We show that the Q function can exhibit sign changes along the cosmic evolution and the Universe reaches the thermal equilibrium as a transient phenomenon.
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spelling doaj.art-8408165d9a2f480b84e13d4df738503f2022-12-22T01:59:31ZengSpringerOpenEuropean Physical Journal C: Particles and Fields1434-60441434-60522018-04-017841910.1140/epjc/s10052-018-5822-0Gauss–Bonnet dark energy on Hořava–Lifshitz cosmologySamuel Lepe0Giovanni Otalora1Instituto de Física, Pontificia Universidad Católica de ValparaísoInstituto de Física, Pontificia Universidad Católica de ValparaísoAbstract We investigate the Gauss–Bonnet dark energy model and its deformed version on Hořava–Lifshitz cosmology, which belongs to the class of cosmologies obtained from the so-called projectable version of Hořava–Lifshitz gravity. In particular, we investigate the bulk/boundary interaction in this scenario through the Q function, which we interpret as a measure of the energy transference between the bulk and the spacetime boundary. Then we discuss whether the thermal equilibrium will be stable or not, once it is reached, and the validity of the generalized second law. We show that the Q function can exhibit sign changes along the cosmic evolution and the Universe reaches the thermal equilibrium as a transient phenomenon.http://link.springer.com/article/10.1140/epjc/s10052-018-5822-0
spellingShingle Samuel Lepe
Giovanni Otalora
Gauss–Bonnet dark energy on Hořava–Lifshitz cosmology
European Physical Journal C: Particles and Fields
title Gauss–Bonnet dark energy on Hořava–Lifshitz cosmology
title_full Gauss–Bonnet dark energy on Hořava–Lifshitz cosmology
title_fullStr Gauss–Bonnet dark energy on Hořava–Lifshitz cosmology
title_full_unstemmed Gauss–Bonnet dark energy on Hořava–Lifshitz cosmology
title_short Gauss–Bonnet dark energy on Hořava–Lifshitz cosmology
title_sort gauss bonnet dark energy on horava lifshitz cosmology
url http://link.springer.com/article/10.1140/epjc/s10052-018-5822-0
work_keys_str_mv AT samuellepe gaussbonnetdarkenergyonhoravalifshitzcosmology
AT giovanniotalora gaussbonnetdarkenergyonhoravalifshitzcosmology