Lyra's Cosmology of Massive String in Anisotropic Bianchi-II Space-time

Details Lyra's Cosmology of Massive String in Anisotropic Bianchi-II Space-time Lyra's Cosmology of Massive String in Anisotropic Bianchi-II Space-time

2011-02-09

arxiv.org/abs/1102.2153v1

Int. J. Theor. Phys. Vol. 50, 2850 - 2863 (2011)

Physics

General Physics

12 pages, 5 figures

Scientific paper

10.1007/s10773-011-0784-0

The paper deals with a spatially homogeneous and totally anisotropic Bianchi II cosmological models representing massive strings in normal gauge for Lyra's manifold. The modified Einstein's field equations have been solved by applying variation law for Hubble's parameter. This law generates two type of solutions for average scale factor, one is of power law type and other is of exponential law type. The power law describes the dynamics of Universe from big bang to present epoch while exponential law seems reasonable to project dynamics of future Universe. It has been found that the displacement actor $(\beta)$ is a decreasing function of time and it approaches to small positive value at late time, which is collaborated with Halford (1970) as well as recent observations of SN Ia. The study reveals that massive strings dominate in early Universe and eventually disappear from Universe for sufficiently large time, which is in agreement with the current astronomical observations.

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