Cosmological models with variable G and Λ

被引:17
作者
Kilinç, CB [1 ]
机构
[1] Ege Univ, Fen Fak Astron Uzay Bilimleri Bolumu, TR-35100 Izmir, Turkey
关键词
variable G and Lambda; Bianchi I models;
D O I
10.1023/B:ASTR.0000009396.57711.53
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Einstein's equations with variable gravitational and cosmological constants are considered in the presence of a perfect fluid for the anizotropic Bianchi I universe in a way which conserving the energy- momentum tensor. Two solutions are found, one of which the cosmological term varies inversely with power law of time. The other of which cosmological term is constant.
引用
收藏
页码:103 / 109
页数:7
相关论文
共 11 条
[1]  
ABDELRAHMAN AMM, 1990, GEN RELAT GRAVIT, V22, P665
[2]   Some FRW models with variable G and Lambda [J].
Abdussattar ;
Vishwakarma, RG .
CLASSICAL AND QUANTUM GRAVITY, 1997, 14 (04) :945-953
[3]   Bianchi type I viscous universe with variable G and Λ [J].
Arbab, AI .
GENERAL RELATIVITY AND GRAVITATION, 1998, 30 (09) :1401-1405
[4]   Cosmological models with variable cosmological and gravitational ''constants'' and bulk viscous models [J].
Arbab, AI .
GENERAL RELATIVITY AND GRAVITATION, 1997, 29 (01) :61-74
[5]   BIANCHI TYPE-I COSMOLOGICAL MODELS WITH VARIABLE-G AND LAMBDA [J].
BEESHAM, A .
GENERAL RELATIVITY AND GRAVITATION, 1994, 26 (02) :159-165
[6]   Anisotropic viscous cosmology with variable G and Λ [J].
Beesham, A ;
Ghosh, SG ;
Lombard, RG .
GENERAL RELATIVITY AND GRAVITATION, 2000, 32 (03) :471-477
[7]   Cosmological models with bulk viscosity in the presence of adiabatic matter creation and with variable G, c, and Λ [J].
Belinchón, JA .
GENERAL RELATIVITY AND GRAVITATION, 2000, 32 (08) :1487-1498
[8]  
BELINCHON JA, PHYSICS9812007
[9]   COSMOLOGICAL MODELS WITH VARIABLE GRAVITATIONAL AND COSMOLOGICAL CONSTANTS [J].
BERMAN, MS .
GENERAL RELATIVITY AND GRAVITATION, 1991, 23 (04) :465-469
[10]   BIANCHI TYPE-I COSMOLOGICAL MODELS WITH VARIABLE-G AND VARIABLE-LAMBDA - A COMMENT [J].
KALLIGAS, D ;
WESSON, PS ;
EVERITT, CWF .
GENERAL RELATIVITY AND GRAVITATION, 1995, 27 (06) :645-650