Higher Dimensional Bianchi Type-V Cosmological Models with Perfect Fluid and Dark Energy

被引:4
作者
Adhav, K. S. [1 ]
Bansod, A. S. [1 ]
Munde, S. L. [1 ]
Desale, M. S. [1 ]
机构
[1] St Gadge Baba Amravati Univ, Dept Math, Amravati, India
基金
英国科研创新办公室;
关键词
Bianchi type-V space-time; Perfect fluid; Dark energy; Higher dimensions; PROBE WMAP OBSERVATIONS; GALAXY REDSHIFT SURVEY; ACCELERATING COSMOLOGIES; DATA RELEASE; DENSITY;
D O I
10.1007/s10773-011-0751-9
中图分类号
O4 [物理学];
学科分类号
0702 ;
摘要
We have studied the Bianchi type-V cosmological models with binary mixture of perfect fluid and dark energy in five dimensions. The perfect fluid is obeying the equation of state p=gamma rho with gamma a[0,1]. The dark energy is considered to be either the quintessence or the Chaplygin gas. The exact solutions of the Einstein's field equations are obtained in quadrature form.
引用
收藏
页码:2573 / 2581
页数:9
相关论文
共 55 条
[51]   The 2dF Galaxy Redshift Survey: the bias of galaxies and the density of the Universe [J].
Verde, L ;
Heavens, AF ;
Percival, WJ ;
Matarrese, S ;
Baugh, CM ;
Bland-Hawthorn, J ;
Bridges, T ;
Cannon, R ;
Cole, S ;
Colless, M ;
Collins, C ;
Couch, W ;
Dalton, G ;
De Propris, R ;
Driver, SP ;
Efstathiou, G ;
Ellis, RS ;
Frenk, CS ;
Glazebrook, K ;
Jackson, C ;
Lahav, O ;
Lewis, I ;
Lumsden, S ;
Maddox, S ;
Madgwick, D ;
Norberg, P ;
Peacock, JA ;
Peterson, BA ;
Sutherland, W ;
Taylor, K .
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 2002, 335 (02) :432-440
[52]   Further evidence for cosmological evolution of the fine structure constant [J].
Webb, JK ;
Murphy, MT ;
Flambaum, VV ;
Dzuba, VA ;
Barrow, JD ;
Churchill, CW ;
Prochaska, JX ;
Wolfe, AM .
PHYSICAL REVIEW LETTERS, 2001, 87 (09) :913011-913014
[53]  
Weinberg S, 1986, PHYS HIGHER DIMENSIO
[54]   Accelerating cosmologies and a phase transition in M-theory [J].
Wohlfarth, MNR .
PHYSICS LETTERS B, 2003, 563 (1-2) :1-5
[55]  
WOODVASEY WM, 2007, ARXIVASTROPH0701041