The Measurement of and in Bianchi Type-I Anisotropic Dark Energy Cosmological Model with Constant Deceleration Parameter in Bimetric Theory of Gravitation

Borkar, M. S.; Gayakwad, P. V.

doi:10.9790/5728-10322838

IOSRJM

2014

DOI: 10.9790/5728-10322838

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The Measurement of and in Bianchi Type-I Anisotropic Dark Energy Cosmological Model with Constant Deceleration Parameter in Bimetric Theory of Gravitation

M. S. Borkar¹,

P. V. Gayakwad²

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2015

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Evaluation of Bianchi type VI₀ magnetized anisotropic dark energy models with constant deceleration parameter in bimetric theory of gravitation

Borkar

Ameen²

2015

Int. J. Mod. Phys. D

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In this paper, Bianchi type VI0 magnetized anisotropic dark energy models with constant deceleration parameter have been studied by solving the Rosen's field equations in Bimetric theory of gravitation. The models corresponding to power law expansion and exponential law expansion have been evaluated and studied their nature geometrically and physically. It is seen that there is real visible matter (baryonic matter) suddenly appeared only for small interval of time 0.7 ≤ t < 0.7598 and for the remaining whole range of time t, there is dark energy matter in the universe. Our investigations are supported to the observational fact that the usual matter described by known particle theory is about 4% and the dark energy cause the accelerating expansion of the universe and several high precision observational experiments, especially the Wilkinson Microwave Anisotropic Probe (WMAP) satellite experiment (see [C. L. Bennett et al., Astrophys. J. Suppl. Ser. 148 (2003) 1; WMAP Collab. (D. N. Spergel et al.), Astrophys. J. Suppl. Ser. 148 (2003) 175; D. N. Spergel et al., Astrophys. J. Suppl. 170 (2007) 377; WMAP Collab. (E. Komastu et al.), Astrophys. J. Suppl. 180 (2009) 330; WMAP Collab. (G. Hinshaw et al.), Astrophys. J. Suppl. 208 (2013) 19; Plank Collab. (P. A. R. Ade), arXiv:1303.5076; arXiv:1303.5082]) conclude that the dark energy occupies near about 73% of the energy of the universe and dark matter is about 23%. In exponential law of expansion, our model is fully occupied by real visible matter and there is no chance of dark energy and dark matter.

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Evaluation of Bianchi type VI₀ magnetized anisotropic dark energy models with constant deceleration parameter in bimetric theory of gravitation

Borkar

Ameen²

2015

Int. J. Mod. Phys. D

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The Measurement of and in Bianchi Type-I Anisotropic Dark Energy Cosmological Model with Constant Deceleration Parameter in Bimetric Theory of Gravitation

Cited by 1 publication

References 36 publications

Evaluation of Bianchi type VI₀ magnetized anisotropic dark energy models with constant deceleration parameter in bimetric theory of gravitation

Evaluation of Bianchi type VI₀ magnetized anisotropic dark energy models with constant deceleration parameter in bimetric theory of gravitation

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The Measurement of and in Bianchi Type-I Anisotropic Dark Energy Cosmological Model with Constant Deceleration Parameter in Bimetric Theory of Gravitation

Cited by 1 publication

References 36 publications

Evaluation of Bianchi type VI0 magnetized anisotropic dark energy models with constant deceleration parameter in bimetric theory of gravitation

Evaluation of Bianchi type VI0 magnetized anisotropic dark energy models with constant deceleration parameter in bimetric theory of gravitation

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Product

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Evaluation of Bianchi type VI₀ magnetized anisotropic dark energy models with constant deceleration parameter in bimetric theory of gravitation

Evaluation of Bianchi type VI₀ magnetized anisotropic dark energy models with constant deceleration parameter in bimetric theory of gravitation