Bianchi Type-IX Dark Energy Model in Sen-Dunn Scalar-Tensor Theory of Gravitation

H. R. Ghate

Authors

H. R. Ghate

Dark Energy, Bianchi Type-Ix, Sen-Dunn Scalar Tensor Theory

Abstract

R 1 sinh ξ = , where ξ and n are positive constants, which render time dependent deceleration parameter. The physical and geometrical properties of the models are also discussed.

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How to Cite

Bianchi Type-IX Dark Energy Model in Sen-Dunn Scalar-Tensor Theory of Gravitation. (2015). Global Journal of Science Frontier Research, 14(F7), 1-15. https://journalofscience.org/index.php/GJSFR/article/view/1435

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