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- W2973068728 abstract "In this paper, we investigate gravastar configurations in which the interior of the compact object is modeled through a Chaplygin fluid. This is motivated by the fact that Chaplygin fluid and the associated exotic equation of state, have often been used as models for the dark energy sector. We derive the relativistic equations of the stellar structure for non-rotating configurations. A special focus is denoted in particular to the mass-radius function and the equation of state for the shell of the gravastars, for which we derive the analytical expressions." @default.
- W2973068728 created "2019-09-19" @default.
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- W2973068728 date "2019-12-19" @default.
- W2973068728 modified "2023-10-03" @default.
- W2973068728 title "Relativistic gravastar configurations in which the interior matter distribution is modeled through a Chaplygin fluid" @default.
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- W2973068728 doi "https://doi.org/10.1142/s0217732319503255" @default.
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