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.

引用

页数：9

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