期刊文献+

Inhomogeneous Bulk Viscous Fluid Universe with Electromagnetic Field and Variable A-Term

Inhomogeneous Bulk Viscous Fluid Universe with Electromagnetic Field and Variable A-Term
下载PDF
导出
摘要 Cylindrically symmetric inhomogeneous cosmological model for bulk viscous fluid distribution with electro- magnetic field is obtained. The source of the magnetic field is due to an electric current produced along the z-axis. F12 is the non-vanishing component of electromagnetic field tensor. To get the deterministic solution, it has been assumed that the expansion 0 in the model is proportional to the shear σ. The values of cosmological constant for these models are found to be small and positive at late time, which are consistent with the results from recent supernovae Ia observations. Physical and geometric aspects of the models are also discussed in presence and absence of magnetic field.
出处 《Communications in Theoretical Physics》 SCIE CAS CSCD 2008年第7期279-288,共10页 理论物理通讯(英文版)
关键词 COSMOLOGY variable cosmological term electromagnetic field inhomogeneous universe 宇宙论 爆炸事件 可变理论 电磁域 不均匀性
  • 相关文献

参考文献99

  • 1R.C. Tolman, Proc. Nat. Acad. Sci. (USA) 20 (1934) 169.
  • 2H. Bondi, Mon. Not. R. Astro. Soc. 107 (1947) 410.
  • 3A.H. Taub, Ann. Math. 53 (1951) 472.
  • 4A.H. Taub, Phys. Rev. 103 (1956) 454.
  • 5N. Tomimura, II Nuovo Cimento B 44 (1978) 372.
  • 6P. Szekeres, Commun. Math. Phys. 41 (1975) 55.
  • 7C.B. Collins and D.A. Szafron, J. Math. Phys. 20 (1979) 2347.
  • 8C.B. Collins and D.A. Szafron,J. Math. Phys. 20 (1979) 2362.
  • 9D.A. Szafron and C.B. Collins, J. Math. Phys. 20 (1979) 2354.
  • 10J.M.M. Senovilla, Phys. Rev. Lett. 64 (1990) 2219.

相关作者

内容加载中请稍等...

相关机构

内容加载中请稍等...

相关主题

内容加载中请稍等...

浏览历史

内容加载中请稍等...
;
使用帮助 返回顶部