Le Châtelier-Braun principle in cosmological physics

Diego Pavón; Bin Wang

doi:10.1007/s10714-008-0656-y

Le Châtelier-Braun principle in cosmological physics

Diego Pavón, Bin Wang

Departament de Física

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Assuming that dark energy may be treated as a fluid with a well-defined temperature, close to equilibrium, we argue that if nowadays there is a transfer of energy between dark energy and dark matter, it must be such that the latter gains energy from the former and not the other way around. © 2008 Springer Science+Business Media, LLC.

Idioma original	Anglès
Pàgines (de-a)	1-5
Revista	General Relativity and Gravitation
Volum	41
Número	1
DOIs	https://doi.org/10.1007/s10714-008-0656-y
Estat de la publicació	Publicada - 1 de gen. 2009

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10.1007/s10714-008-0656-y

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title = "Le Ch{\^a}telier-Braun principle in cosmological physics",

abstract = "Assuming that dark energy may be treated as a fluid with a well-defined temperature, close to equilibrium, we argue that if nowadays there is a transfer of energy between dark energy and dark matter, it must be such that the latter gains energy from the former and not the other way around. {\textcopyright} 2008 Springer Science+Business Media, LLC.",

keywords = "Cosmology, Dark energy, Thermodynamics",

author = "Diego Pav{\'o}n and Bin Wang",

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doi = "10.1007/s10714-008-0656-y",

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AU - Wang, Bin

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N2 - Assuming that dark energy may be treated as a fluid with a well-defined temperature, close to equilibrium, we argue that if nowadays there is a transfer of energy between dark energy and dark matter, it must be such that the latter gains energy from the former and not the other way around. © 2008 Springer Science+Business Media, LLC.

AB - Assuming that dark energy may be treated as a fluid with a well-defined temperature, close to equilibrium, we argue that if nowadays there is a transfer of energy between dark energy and dark matter, it must be such that the latter gains energy from the former and not the other way around. © 2008 Springer Science+Business Media, LLC.

KW - Cosmology

KW - Dark energy

KW - Thermodynamics

UR - https://www.scopus.com/pages/publications/58149346171

U2 - 10.1007/s10714-008-0656-y

DO - 10.1007/s10714-008-0656-y

M3 - Article

SN - 0001-7701

VL - 41

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JO - General Relativity and Gravitation

JF - General Relativity and Gravitation

IS - 1

ER -

Le Châtelier-Braun principle in cosmological physics

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