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Plane Symmetric Anisotropic Dark Energy Cosmological Model in the Bimetric Theory of Gravitation

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Astrophysics Aims and scope

The plane symmetric space-times with anisotropic dark energy and with constant deceleration parameter have been derived by solving the Rosen's field equations in the Bimetric theory of gravitation. We explored both models in power law as well as in exponential law. In power law, the model attains both phases accelerating as well as decelerating in the expansion with anisotropic fluid, which is in the form of dark energy, and there is no chance of real matter in this power law. In exponential law, the model is dust, isotropized in nature with constant acceleration in the expansion. Further, other geometrical and physical aspects of the models are also studied.

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Authors and Affiliations

  1. Nagpur University, Nagpur, India

    M. S. Borkar

  2. Institute of Engineering and Technology, Nagpur, India

    A. Ameen

Authors
  1. M. S. Borkar
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  2. A. Ameen
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Correspondence to M. S. Borkar.

Additional information

Published in Astrofizika, Vol. 60, No. 2, pp. 263-276 (May 2017).

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Borkar, M.S., Ameen, A. Plane Symmetric Anisotropic Dark Energy Cosmological Model in the Bimetric Theory of Gravitation. Astrophysics 60, 242–258 (2017). https://doi.org/10.1007/s10511-017-9479-4

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  • DOI: https://doi.org/10.1007/s10511-017-9479-4

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