Magnetized anisotropic dark energy models with constant deceleration parameter

被引：6
作者：
Shaikh, A. Y. [1 ]
Katore, S. D. [2 ]
机构：
[1] Indira Gandhi Mahavidyalaya, Dept Math, Ralegaon 445402, India
[2] SGB Amravati Univ, PG Dept Math, Amravati 444602, India
来源：
PRAMANA-JOURNAL OF PHYSICS | 2016年 / 87卷 / 06期
关键词：
Dark energy; magnetism; HIGH-REDSHIFT SUPERNOVAE; BIANCHI-I UNIVERSE; COSMOLOGICAL MODELS; GRAVITATION; DYNAMICS; EQUATION; OMEGA; STATE; TIME;
D O I：
10.1007/s12043-016-1272-0
中图分类号：
O4 [物理学];
学科分类号：
0702 ;
摘要：
In this paper, we have studied the solutions of plane-symmetric Universe with variable omega in the presence and the absence of magnetic field of energy density rho(B). A special law of variation for Hubble's parameter proposed by Bermann in Nuovo Cimento B 74, 182 (1983) has been utilized to solve the field equations. Some physical and kinematical properties of the models are also discussed.
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页数：9
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