Perfect fluid cosmological Universes: One equation of state and the most general solution

被引:8
作者
Das, Anadijiban [1 ]
Banerjee, Asit [2 ]
Chakraborty, Subenoy [3 ]
Pan, Supriya [4 ]
机构
[1] Simon Fraser Univ, Dept Math, Burnaby, BC V5A 1S6, Canada
[2] Jadavpur Univ, Dept Phys, Kolkata 700032, India
[3] Jadavpur Univ, Dept Math, Kolkata 700032, India
[4] Indian Inst Sci Educ & Res, Dept Phys Sci, Kolkata 741246, Mohanpur, India
来源
PRAMANA-JOURNAL OF PHYSICS | 2018年 / 90卷 / 02期
关键词
Perfect fluid; equation of state; cosmological solutions;
D O I
10.1007/s12043-017-1511-z
中图分类号
O4 [物理学];
学科分类号
0702 ;
摘要
Considering a homogeneous and isotropic Universe characterised by the Friedmann-Lemaitre-Robertson-Walker line element, in this work, we have prescribed a general formalism for the cosmological solutions when the equation of state of the cosmic substance follows the general structure phi(p, rho) = 0, where p, rho are respectively the pressure and the energy density of the cosmic substance. Using the general formalism we recover some well-known solutions, namely, when the cosmic substance obeys the linear equation of state, a Chaplygin-type equation of state, or a nonlinear equation of state. Thus, the current work offers a new technique to solve the cosmological solutions without any prior relation between p and rho.
引用
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页数:6
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