作者: Bikash Chandra Paul , Rumi Deb
DOI: 10.1007/S10509-014-2097-2
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摘要: We present a class of new relativistic solutions with anisotropic fluid for compact stars in hydrostatic equilibrium. The interior space-time geometry considered here objects are described by parameters namely, λ, k, A, R and n. values the geometrical determined obtaining physically viable stellar models. energy-density, radial pressure tangential finite positive inside stars. Considering some known mass we models which describe astrophysical nuclear density.