Thermodynamic properties of molecular fluid mixtures of hard ellipsoids

Study of charged compact stars with class 1 metric under general relativity

“…In the present paper, we have studied the physical properties of the charged compact stars, e.g. Her X − 1, Cen X − 3, (20)(21), it is difficult to predict a exact form of EOS for the proposed charged compact stellar model. However, we have analyzed from Eq.…”

“…This embedding class is divided into the following classification scheme: (i) spherically symmetric fields of class 2, (ii) the interior Schwarzschild solution and spherically symmetric field are of class 1 [7], (iii) the exterior solution is of class 2, (iv) the Kerr metric is of class 5 [8], and (v) the cosmological metric Friedmann-Lemaître-Robertson-Walker (FLRW) metric has been shown to be of class 1. We, along with other scientists, have done a detailed discussion on different aspects of the class 1 metric and their applications in special connection to compact stars [9][10][11][12][13][14][15][16][17][18][19][20][21][22]. Also, neutron stars, like those discussed in the work by Astashenok et al [23] for magnetic field and by Capozziello et al [24] for f (R) gravity may be taken into account which would help the reader in enlarging the context of the compact stars with different approach.…”