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- W2999447424 abstract "A charged stellar model is presented by constructing a solution to the Einstein–Maxwell equations system in a spherically symmetrical static time-space. The rate of compactness for the model depends on two parameters [Formula: see text], one of them [Formula: see text] associated to the charge, which allows a value of compactness [Formula: see text] higher than the neutral case. The density and pressure are regular functions, positive and monotonically decreasing and the function of charge is positive regular and monotonically increasing, its shown that the model satisfies the condition of causality, the geometry is regular and as such the model is physically acceptable. Although the model can be applicable for a variety of stars, considering a star with mass [Formula: see text] for [Formula: see text] the range of compactness is [Formula: see text] and radius [Formula: see text], in this case the range of values for the central density is [Formula: see text] greater than the value of the nuclear density and consistent with that expected for stars with this compactness rate." @default.
- W2999447424 created "2020-01-23" @default.
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- W2999447424 date "2020-02-01" @default.
- W2999447424 modified "2023-10-18" @default.
- W2999447424 title "Compact stars described by a charged model" @default.
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- W2999447424 doi "https://doi.org/10.1142/s0218271820500224" @default.
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