BIANCHI TYPE V INFLATIONARY UNIVERSE WITH FLAT POTENTIAL AND STIFF FLUID DISTRIBUTION IN GENERAL RELATIVITY

被引：0

作者：

Bali, Raj ^{[1
]}

Kumari, Parmit ^{[1
]}

机构：

[1] Univ Rajasthan, Dept Math, Jaipur 302004, Rajasthan, India

来源：

JOURNAL OF RAJASTHAN ACADEMY OF PHYSICAL SCIENCES | 2015年 / 14卷 / 02期

关键词：

Bianchi V; Inflationary; Stiff fluid; flat potential;

D O I：

暂无

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：

Inflationary scenario for massless scalar field, flat potential and stiff fluid distribution in Bianchi Type V space-time is investigated. We find that the rate of Higgs field decreases with time. The spatial volume increases with time representing inflationary scenario. The model represents decelerating and accelerating phases of universe and also represents anisotropic space-time but isotropizes at late time. The Hubble parameter decreases with time. The model has Point Type singularity at T = 0. The particular case is also discussed. The results match with astronomical observations.

引用

页码：185 / 197

页数：13

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