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Anisotropic Dark Energy Bianchi Type-II Cosmological Models in Lyra Geometry

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Abstract

The spatially homogeneous and totally anisotropic Bianchi type-II cosmological model has been discussed in general relativity in the presence of a hypothetical anisotropic dark energy fluid with constant deceleration parameter within the frame work of Lyra’s manifold with uniform and time varying displacement field vector. With the help of special law of variation for Hubble’s parameter proposed by Bermann (Nuovo Cimento 74B:182, 1983) a dark energy cosmological model is obtained in this theory. We use the power law relation between average Hubble parameter H and average scale factor R to find the solution. The assumption of constant deceleration parameter leads to two models of universe, i.e. power law model and exponential model. Some physical and kinematical properties of the model are also discussed.

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Acknowledgements

The authors express his thanks to Prof. Raj Senani, Director, NSIT, and Prof. Vijay Gupta, Head, School of Applied Sciences, NSIT, India for their continuing encouragement and providing necessary facilities during the work. The authors also express his thanks to the referee for valuable suggestions.

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  1. School of Applied Sciences, Netaji Subhash Institute of Technology, University of Delhi, Sector-3, Dwarka, New Delhi, 110078, India

    J. K. Singh & N. K. Sharma

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  1. J. K. Singh
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  2. N. K. Sharma
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Correspondence to N. K. Sharma.

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Singh, J.K., Sharma, N.K. Anisotropic Dark Energy Bianchi Type-II Cosmological Models in Lyra Geometry. Int J Theor Phys 53, 1375–1386 (2014). https://doi.org/10.1007/s10773-013-1934-3

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  • DOI: https://doi.org/10.1007/s10773-013-1934-3

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