Purely kinetic k-essence description of cs2(w) barotropic fluid models

被引:6
作者
Perkovic, Dalibor [1 ]
Stefancic, Hrvoje [2 ]
机构
[1] Univ Appl Hlth Sci, Mlinarska St 38, Zagreb 10000, Croatia
[2] Catholic Univ Croatia, Ilica 242, Zagreb 10000, Croatia
来源
PHYSICS OF THE DARK UNIVERSE | 2021年 / 32卷
关键词
DARK-MATTER; INFLATIONARY UNIVERSE; ENERGY; COSMOLOGY; DYNAMICS; FLATNESS; HORIZON;
D O I
10.1016/j.dark.2021.100827
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Purely kinetic k-essence models have been shown in the literature to be a field theory equivalent of barotropic fluid models of dark energy or dark matter-dark energy unification. In the modeling framework where the speed of sound squared of a barotropic fluid is modeled as a function of its Equation of State parameter, a systematic procedure of obtaining the Lagrangian density of an equivalent purely kinetic k-essence model is presented. As this modeling approach starts from the speed of sound, purely kinetic k-essence models can be constructed for which the speed of sound is in agreement with the observational constraints. Depending on the chosen functional form for the barotropic fluid speed of sound squared, analytically tractable examples of solutions for the purely kinetic k-essence Lagrangian density in parametric and closed form are obtained. (C) 2021 Elsevier B.V. All rights reserved.
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页数:8
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