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

Himchandra Ram Ghate
Himchandra Ram Ghate * §
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§ Jijamata Mahavidyalaya Buldana

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

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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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Funding

No external funding was declared for this work.

Conflict of Interest

The authors declare no conflict of interest.

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How to Cite This Article

H. R. Ghate. 2015. "Bianchi Type-IX Dark Energy Model in Sen-Dunn Scalar-Tensor Theory of Gravitation". Global Journal of Science Frontier Research - F: Mathematics & Decision GJSFR-F Volume 14 (GJSFR Volume 14 Issue F7).

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Journal Specifications

Crossref Journal DOI 10.17406/GJSFR

Print ISSN 0975-5896

e-ISSN 2249-4626

Keywords
Bianchi Type-IxDark energySen-Dunn Scalar Tensor Theory
Classification
GJSFR-F Classification MSC 2010: 81V17
  • Submission ReceivedSeptember 8, 2014
  • Peer Review Double Blind
    Handling Editor
  • Accepted October 4, 2014
  • Published October 18, 2014
Version of record

v1.2

Issue date
January 8, 2015

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

H. Ghate
H. Ghate Jijamata Mahavidyalaya Buldana
  • Submission ReceivedSeptember 8, 2014
  • Peer Review Double Blind
    Handling Editor
  • Accepted October 4, 2014
  • Published October 18, 2014