具有粘性的熵宇宙学的热力学方面

I. Brevik, A. Timoshkin, A. Timoshkin
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引用次数: 6

摘要

我们用变指数的广义非扩展Tsallis熵,从热力学角度描述了宇宙早期和晚期的演化。我们分析中的一个新元素是在宇宙流体的描述中包含了体粘度。利用广义的弗里德曼方程,得到了早期宇宙和晚期宇宙的描述。
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Thermodynamic aspects of entropic cosmology with viscosity
We describe the evolution of the early and late universe from thermodynamic considerations, using the generalized non-extensive Tsallis entropy with a variable exponent. A new element in our analysis is the inclusion of a bulk viscosity in the description of the cosmic fluid. Using the generalized Friedmann equation, a description of the early and the late universe is obtained.
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