Kantowski-Sachs Ghost Dark Energy Cosmological Model with Specific Hubble Parameter in f(R, T) Gravity

被引：0

作者：

Ghate, H. R. ^{[1
]}

Sontakke, Atish S. ^{[1
]}

机构：

[1] Jijamata Mahavidyalaya, Dept Math, Buldana 443001, India

来源：

IRANIAN JOURNAL OF SCIENCE AND TECHNOLOGY TRANSACTION A-SCIENCE | 2018年 / 42卷 / A2期

基金：

英国科研创新办公室;

关键词：

f(R. T) gravity; Ghost dark energy; Kantowski-Sachs metric; Specific Hubble parameter; PROBE WMAP OBSERVATIONS; EQUATION-OF-STATE; SPACE-TELESCOPE; V COSMOLOGY; F R; UNIVERSE; CONSTRAINTS; RECONSTRUCTION; DECELERATION; SUPERNOVAE;

D O I：

10.1007/s40995-017-0229-6

中图分类号：

O [数理科学和化学]; P [天文学、地球科学]; Q [生物科学]; N [自然科学总论];

学科分类号：

07 ; 0710 ; 09 ;

摘要：

Kantowski-Sachs cosmological model is studied in the framework of f(R, T) gravity proposed by Harko et al. (Phys Rev D 84:024020, 2011). The source for energy momentum tensor is non-interacting two fluids viz. matter and ghost dark energy. The held equations have been solved using a specihc form of Hubble parameter proposed by Singh (Astrophys. Space Sci. 318, 2008). Then some physical and mathematical properties of the model are also discussed.

引用

页码：847 / 855

页数：9

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