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- W2979669506 abstract "Abstract In this work we obtain an anisotropic neutron star solution by gravitational decoupling starting from a perfect fluid configuration which has been used to model the compact object PSR J0348+0432. Additionally, we consider the same solution to model the Binary Pulsar SAX J1808.4-3658 and X-ray Binaries Her X-1 and Cen X-3 ones. We study the acceptability conditions and obtain that the MGD-deformed solution obey the same physical requirements as its isotropic counterpart. Finally, we conclude that the most stable solutions, according to the adiabatic index and gravitational cracking criterion, are those with the smallest compactness parameters, namely SAX J1808.4-3658 and Her X-1." @default.
- W2979669506 created "2019-10-18" @default.
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- W2979669506 date "2019-10-01" @default.
- W2979669506 modified "2023-10-07" @default.
- W2979669506 title "Anisotropic neutron stars by gravitational decoupling" @default.
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- W2979669506 doi "https://doi.org/10.1140/epjc/s10052-019-7341-z" @default.
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