Five dimensional universe model with variable cosmological term Λ and a big bounce

被引:0
作者
G. S. Khadekar
Vaishali Kamdi
Anirudh Pradhan
Saeed Otarod
机构
[1] R.T.M. Nagpur University,Department of Mathematics
[2] Hindu Post-graduate College,Department of Mathematics
[3] Yasouj University,Department of Physics
来源
Astrophysics and Space Science | 2007年 / 310卷
关键词
Cosmology; Induced matter theory; Variable cosmological constant; 98.80.Jk; 98.80.Es;
D O I
暂无
中图分类号
学科分类号
摘要
We assume the four dimensional induced matter of the 5D Ricci flat bouncing cosmological solution contains a perfect fluid. The big bounce singularity of simple 5D cosmological model is studied with the cosmological term Λ=αρ and Λ=βH2 where α and β are constants and ρ and H are respectively energy density and Hubble parameter. This big bounce singularity is found to be an event horizon at which the scale factor and mass density of the universe are finite, while the pressure is infinite.
引用
收藏
页码:141 / 147
页数:6
相关论文
共 51 条
[1]  
Al-Rawaf A.S.(1996)undefined Gen. Relativ. Gravit. 28 935-undefined
[2]  
Taha M.O.(1998)undefined Mod. Phys. Lett. A 13 429-undefined
[3]  
Al-Rawaf A.S.(2003)undefined J. Cosmol. Astropart. Phys. 05 008-undefined
[4]  
Arbab A.I.(2003)undefined Class. Quantum Gravit. 20 93-undefined
[5]  
Arbab A.I.(1992)undefined Annu. Rev. Astron. Astrophys. 30 499-undefined
[6]  
Carroll S.M.(2000)undefined Int. J. Mod. Phys. A 15 697-undefined
[7]  
Press W.H.(1921)undefined Sitz. Preuss. Akad. Wiss. 33 966-undefined
[8]  
Turner E.L.(1926)undefined Z. Phys. 37 895-undefined
[9]  
Cheng Y.C.N.(2006)undefined Int. J. Mod. Phys. D 15 95-undefined
[10]  
Krauss L.M.(1995)undefined Astrophys. J. 441 L55-undefined