La Chatelier-Braun principle in cosmological physics

被引：197

作者：

Pavon, Diego ^{[1
]}

Wang, Bin ^{[2
]}

机构：

[1] Autonomous Univ Barcelona, Dept Phys, Bellaterra 08193, Spain

[2] Fudan Univ, Dept Phys, Shanghai 200433, Peoples R China

来源：

GENERAL RELATIVITY AND GRAVITATION | 2009年 / 41卷 / 01期

关键词：

Cosmology; Dark energy; Thermodynamics; HOLOGRAPHIC DARK ENERGY; MATTER;

D O I：

10.1007/s10714-008-0656-y

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

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.

引用

页码：1 / 5

页数：5

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