Anisotropic Neutral Models With Van Der Waals Equation Of State

ABSTRACT

We find new exact solutions to Einstein-Maxwell field equation for neutral anisotropy

stellar stars with Van der Waals equation of state. We adopted Sunzu, Maharaj and Ray‘s

metric function and measure of anisotropy. The solutions are obtained after considering

the transformed Einstein-Maxwell field equations for neutral anisotropic matter. In our

models, we regain previous anisotropic and isotropic results as a special case. We consider

the space-time geometry to be static spherically symmetry. The exact solutions to

the Einstein-Maxwell field equations corresponding to our models are found explicitly

in terms of elementary functions namely simple algebraic functions. The gravitational

potentials and matter variables generated are well behaved. We also generate relativistic

stellar masses consistent with the stars PSR J1614-2230, Vela X-1, 4U 1538-52, LMC

X-4, SMC X-4, Cen X-3, Her X-1, SAX J1808.4-3658 and EXO 1785-248.