Exact solutions for compact stars in general relativity

نویسندگان

چکیده

Abstract Complete, exact, analytic solutions to the spherically symmetric Einstein equations have been constructed. Beginning with Tolman VII solution we first “complete” by computing an expression for pressure and subsequently equation of state. The is then extended include non-zero mass densities at fluid-vacuum interface. method developed construct these transverse pressures charge. Furthermore quadratic density profile type modified quartic profiles that lead expressions in terms Jacobi elliptic integrals. It shown that, depending on outer boundary conditions placed density, state either a set polytropes or behaviour mimics strange quark matter.

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ژورنال

عنوان ژورنال: Journal of physics

سال: 2023

ISSN: ['0022-3700', '1747-3721', '0368-3508', '1747-3713']

DOI: https://doi.org/10.1088/1742-6596/2536/1/012003