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To explain the 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 the presence of a quintessence field which is characterized by a parameter q with -1< q<-13. The model has been developed by choosing the Vaidya–Tikekar ansatz (J Astrophys Astron 3: 325, 1982). Our model satisfies all the physical requirements. We have analyzed our result analytically as well as with the help of a graphical representation.
Piyali Bhar (Sun,) studied this question.