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- W2005778807 abstract "In the present article, we have obtained a new class of well behaved charged super-dense star models after prescribing a particular form of the metric potential and electric intensity. The metric describing the super-dense stars model joins smoothly with the Reissner-Nordstrom metric at the pressure free boundary. The interior of the stars possess there energy density, pressure, pressure-density ratio and velocity of sound to be monotonically decreasing towards the pressure free interface" @default.
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- W2005778807 date "2012-01-01" @default.
- W2005778807 modified "2023-10-16" @default.
- W2005778807 title "Analytic Well Behaved Charged Relativistic Super-dense Star Models" @default.
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- W2005778807 doi "https://doi.org/10.1016/j.proeng.2012.06.154" @default.
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