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arXiv 2103.07718gr-qc
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具有二次引力和非理想流体的宇宙演化

Cosmological evolution with quadratic gravity and nonideal fluids

Saikat Chakraborty, Daniele Gregoris

摘要:

基于引力理论$f(R) = R+ζR^2$和流体服从Redlich-Kwong、Berthelot和Dieterici状态方程的宇宙学模型被提出来描述不同宇宙时代之间的平滑过渡。动力学系统分析表明,这些模型包含不动点,对应于一个膨胀,辐射为主,晚时间加速时代,和一个非奇异的弹跳解决方案,后者是一个渐近不动点的紧致相空间。紧化相空间的无穷大被解释为一个区域,在该区域中,前面提到的宇宙流体的非理想行为被抑制。通过要求理论不受鬼和快子不稳定性的影响,对所采用的无量纲变量进行了物理约束,并通过宇宙学分析提出了一种新的宇宙学解释。阐明了状态方程参数对平衡解的数目及其稳定性的不同影响。这些模型,这是不敏感的特定流体考虑,确定了一些通用的属性,而差异进行了严格的检查,显示Redlich-Kwong的情况下承认第二个辐射主导的时代和大撕裂奇点。

英文摘要:

Some cosmological models based on the gravitational theory $f(R) = R+ζR^2$, and on fluids obeying to the equations of state of Redlich-Kwong, Berthelot, and Dieterici are proposed for describing smooth transitions between different cosmic epochs. A dynamical system analysis reveals that these models contain fixed points which correspond to an inflationary, a radiation dominated and a late-time accelerating epoch, and a nonsingular bouncing solution, the latter being an asymptotic fixed point of the compactified phase space. The infinity of the compactified phase space is interpreted as a region in which the non-ideal behaviors of the previously mentioned cosmic fluids are suppressed. Physical constraints on the adopted dimensionless variables are derived by demanding the theory to be free from ghost and tachyonic instabilities, and a novel cosmological interpretation of such variables is proposed through a cosmographic analysis. The different effects of the equation of state parameters on the number of equilibrium solutions and on their stability nature are clarified. Some generic properties of these models, which are not sensitive to the particular fluid considered, are identified, while differences are critically examined by showing that the Redlich-Kwong scenario admits a second radiation-dominated epoch and a Big Rip Singularity.

机构、总结、中文摘要均由AI分析而来,可能存在错误,请以论文正文为准。

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