Regular Article - Theoretical Physics
Stellar modelling of PSR J1614-2230 using the Karmarkar condition
Department of Mathematics, National Defence Academy, 411023, Khadakwasla, Pune, India
* e-mail: firstname.lastname@example.org
Accepted: 7 October 2018
Published online: 30 November 2018
The main objective of the paper is to provide a new family of solutions of embedding class one describing the interior of a spherically symmetric anisotropic stellar configuration. For and 12, all the physical parameters are well-behaved within the stellar interior and our model satisfies all the required conditions to be physically viable. Due to the well-behaved nature of the solution of the above n values, we develop the model of PSR J1614-2230 (Nature 467, 1081 (2010)) and discuss the behavior of the class of solutions extensively. By analyzing the adiabatic index () we observe that for lower values of n, i.e., , the star is soft and as we increase the value of n the star becomes stiff.
© SIF, Springer-Verlag GmbH Germany, part of Springer Nature, 2018