INHOMOGENEOUS BIANCHI TYPE VI0 STRING DUST COSMOLOGICAL MODEL OF PERFECT FLUID DISTRIBUTION IN GENERAL RELATIVITY
被引:0
作者:
Tyagi, Atul
论文数: 0引用数: 0
h-index: 0
机构:
MLS Univ, Univ Coll Sci, Dept Math & Stat, Udaipur 313001, IndiaMLS Univ, Univ Coll Sci, Dept Math & Stat, Udaipur 313001, India
Tyagi, Atul
[1
]
Sharma, Arvind
论文数: 0引用数: 0
h-index: 0
机构:
Sir Padampat Singhania Univ, Dept Math, Udaipur 313601, IndiaMLS Univ, Univ Coll Sci, Dept Math & Stat, Udaipur 313001, India
Sharma, Arvind
[2
]
Chhajed, Dhirendra
论文数: 0引用数: 0
h-index: 0
机构:
Sir Padampat Singhania Univ, Dept Math, Udaipur 313601, IndiaMLS Univ, Univ Coll Sci, Dept Math & Stat, Udaipur 313001, India
Chhajed, Dhirendra
[2
]
机构:
[1] MLS Univ, Univ Coll Sci, Dept Math & Stat, Udaipur 313001, India
[2] Sir Padampat Singhania Univ, Dept Math, Udaipur 313601, India
来源:
JOURNAL OF RAJASTHAN ACADEMY OF PHYSICAL SCIENCES
|
2015年
/
14卷
/
01期
关键词:
Bianchi -VI0 space times;
cosmic string and general relativity;
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:
We have investigated inhomogeneous Bianchi type VI0 string dust cosmological model in general relativity. To obtain the deterministic solution of Einstein's field equations, we assume that string tension density lambda is equal to rest density rho i.e. lambda = rho. The model obtained is expanding, shearing and non-rotating universe. Some physical and geometrical features of the model are also discussed.