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

H. R. Ghate; atishsontakke

Authors

H. R. Ghate
atishsontakke

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. (2014). Global Journal of Science Frontier Research, 14(46), 1-15. https://journalofscience.org/index.php/GJSFR/article/view/

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Author Biography

H. R. Ghate

Dr. H. R. Ghate is a dedicated researcher in theoretical cosmology and gravitation, affiliated with Jijamata Mahavidyalaya Buldana in Maharashtra, India. His work explores cosmological models, dark energy, scalar-tensor theories, and creation field cosmology. With over 30 publications, he has contributed to understanding Bianchi type-IX models, Kaluza-Klein theories, and bounce cosmology. His research continues to advance the field of general relativity and modern cosmology.

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