Thermodynamic approach to holographic dark energy and the Rényi entropy

Abstract Using the first law of thermodynamics, we propose a relation between the system entropy (S) and its IR (L) and UV ($$\Lambda $$ Λ ) cutoffs. In addition, applying this relation to the apparent horizon of flat FRW universe, whose entropy meets the Rényi entropy, a new holographic dark energy...

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Main Authors: H. Moradpour, S. A. Moosavi, I. P. Lobo, J. P. Morais Graça, A. Jawad, I. G. Salako
Format: Article
Language:English
Published: SpringerOpen 2018-10-01
Series:European Physical Journal C: Particles and Fields
Online Access:http://link.springer.com/article/10.1140/epjc/s10052-018-6309-8
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author H. Moradpour
S. A. Moosavi
I. P. Lobo
J. P. Morais Graça
A. Jawad
I. G. Salako
author_facet H. Moradpour
S. A. Moosavi
I. P. Lobo
J. P. Morais Graça
A. Jawad
I. G. Salako
author_sort H. Moradpour
collection DOAJ
description Abstract Using the first law of thermodynamics, we propose a relation between the system entropy (S) and its IR (L) and UV ($$\Lambda $$ Λ ) cutoffs. In addition, applying this relation to the apparent horizon of flat FRW universe, whose entropy meets the Rényi entropy, a new holographic dark energy model is addressed. Thereinafter, the evolution of the flat FRW universe, filled by a pressureless source and the obtained dark energy candidate, is studied. In our model, there is no mutual interaction between the cosmos sectors. We find out that the obtained model is theoretically powerful to explain the current accelerated phase of the universe. This result emphasizes that the generalized entropy formalism is suitable for describing systems including the long-range interactions such as gravity.
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spelling doaj.art-80acb94c9f944540b1bbe15df66aac202022-12-22T01:23:58ZengSpringerOpenEuropean Physical Journal C: Particles and Fields1434-60441434-60522018-10-0178101610.1140/epjc/s10052-018-6309-8Thermodynamic approach to holographic dark energy and the Rényi entropyH. Moradpour0S. A. Moosavi1I. P. Lobo2J. P. Morais Graça3A. Jawad4I. G. Salako5Research Institute for Astronomy and Astrophysics of Maragha (RIAAM)Research Institute for Astronomy and Astrophysics of Maragha (RIAAM)Departamento de Física, Universidade Federal da ParaíbaDepartamento de Física, Universidade Federal da ParaíbaDepartment of Mathematics, COMSATS University IslamabadInstitut de Mathématiques et de Sciences Physiques (IMSP)Abstract Using the first law of thermodynamics, we propose a relation between the system entropy (S) and its IR (L) and UV ($$\Lambda $$ Λ ) cutoffs. In addition, applying this relation to the apparent horizon of flat FRW universe, whose entropy meets the Rényi entropy, a new holographic dark energy model is addressed. Thereinafter, the evolution of the flat FRW universe, filled by a pressureless source and the obtained dark energy candidate, is studied. In our model, there is no mutual interaction between the cosmos sectors. We find out that the obtained model is theoretically powerful to explain the current accelerated phase of the universe. This result emphasizes that the generalized entropy formalism is suitable for describing systems including the long-range interactions such as gravity.http://link.springer.com/article/10.1140/epjc/s10052-018-6309-8
spellingShingle H. Moradpour
S. A. Moosavi
I. P. Lobo
J. P. Morais Graça
A. Jawad
I. G. Salako
Thermodynamic approach to holographic dark energy and the Rényi entropy
European Physical Journal C: Particles and Fields
title Thermodynamic approach to holographic dark energy and the Rényi entropy
title_full Thermodynamic approach to holographic dark energy and the Rényi entropy
title_fullStr Thermodynamic approach to holographic dark energy and the Rényi entropy
title_full_unstemmed Thermodynamic approach to holographic dark energy and the Rényi entropy
title_short Thermodynamic approach to holographic dark energy and the Rényi entropy
title_sort thermodynamic approach to holographic dark energy and the renyi entropy
url http://link.springer.com/article/10.1140/epjc/s10052-018-6309-8
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