Vaidya-Tikekar Type Superdense Star Admitting Conformal Motion in Presence of Quintessence Field

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.

9 pages,13 figures

References in corpus (8)

• Charged gravastars admitting conformal motion
• Dark energy models with variable equation of state parameter
• Conformally symmetric traversable wormholes
• Tikekar superdense stars in electric fields
• Singularity free anisotropic strange quintessence star
• Wormhole geometries with conformal motions
• A class of solutions for anisotropic stars admitting conformal motion
• Variable Equation of State for Generalized Dark Energy Model

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