Nonsingular decaying vacuum cosmology and entropy production
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- 作者：J. A. S. Lima ; Spyros Basilakos ; Joan Solà
- 关键词：Cosmology ; Theory ; Early universe
- 刊名：General Relativity and Gravitation
- 出版年：2015
- 出版时间：April 2015
- 年：2015
- 卷：47
- 期：4
- 全文大小：280 KB
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- 刊物主题：Physics
Mathematical and Computational Physics
Relativity and Cosmology
Differential Geometry
Quantum Physics
Astronomy, Astrophysics and Cosmology - 出版者：Springer Netherlands
- ISSN：1572-9532
文摘
The thermodynamic behavior of a decaying vacuum cosmology describing the entire cosmological history evolving between two extreme (early and late time) de Sitter eras is investigated. The thermal evolution from the early de Sitter to the radiation phase is discussed in detail. The temperature evolution law and the increasing entropy function are analytically determined. The entropy of the effectively massless particles is initially zero but evolves continuously to the present day maximum value within the current Hubble radius, \(S_0 \sim 10^{88}\) in natural units. By using the Gibbons–Hawking temperature relation for the de Sitter spacetime, it is found that the ratio between the primeval and the late time vacuum energy densities is \(\rho _{vI}/\rho _{v0} \sim 10^{123}\) , as required by some naive estimates from quantum field theory.