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• W2013443163 abstract "To explain the reason of accelerated expansion of our universe dark energy is a suitable candidate. Motivated by this concept in the present paper we have obtained a new model of an anisotropic superdense star which admits conformal motions in presence of quintessence field which is characterized by a parameter $omega$ with omega lies in the range -1 to -1/3.The model has been developed by choosing Vaidya-Titekar ansatz [P C Vaidya and R Tikekar (1982)J. Astrophys .Astron. 3 325].Our model satisfy all the physical requirements.We have analyze our result analytically as well as with the help of graphical representation." @default.
• W2013443163 created "2016-06-24" @default.
• W2013443163 creator A5078025647 @default.
• W2013443163 date "2015-03-01" @default.
• W2013443163 modified "2023-10-13" @default.
• W2013443163 title "Vaidya–Tikekar type superdense star admitting conformal motion in presence of quintessence field" @default.
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• W2013443163 doi "https://doi.org/10.1140/epjc/s10052-015-3340-x" @default.
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