Thermodynamics of scale-dependent Friedmann equations

被引:11
|
作者
Bargueno, Pedro [1 ]
Contreras, Ernesto [2 ]
Rincon, Angel [3 ]
机构
[1] Univ Alicante, Dept Fis Aplicada, Campus San Vicente Raspeig, Alicante 03690, Spain
[2] Univ San Francisco Quito, Colegio Ciencias & Ingn, Dept Fis, Quito, Ecuador
[3] Pontificia Univ Catolica Valparaiso, Inst Fis, Ave Brasil 2950, Valparaiso 4059, Chile
来源
EUROPEAN PHYSICAL JOURNAL C | 2021年 / 81卷 / 05期
关键词
CHARGED BLACK-HOLES; RELATIVISTIC STARS; INTERIOR SOLUTIONS; TENSOR; UNIVERSE; GRAVITY; STATE;
D O I
10.1140/epjc/s10052-021-09274-7
中图分类号
O412 [相对论、场论]; O572.2 [粒子物理学];
学科分类号
摘要
In this work, the role of a time-varying Newton constant under the scale-dependent approach is investigated in the thermodynamics of the Friedman equations. In particular, we show that the extended Friedman equations can be derived either from equilibrium thermodynamics when the non-matter energy momentum tensor is interpreted as a fluid or from non-equilibrium thermodynamics when an entropy production term, which depends on the time-varying Newton constant, is included. Finally, a comparison between black hole and cosmological thermodynamics in the framework of scale-dependent gravity is briefly discussed.
引用
收藏
页数:6
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