Starting from a known perfect-fluid neutron star model, the paper constructs anisotropic versions via minimal geometric deformation and finds that the least compact models (SAX J1808.4-3658 and Her X-1) are the most stable.
(20) which is a linear combination of Eqs
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Anisotropic neutron stars by gravitational decoupling
Starting from a known perfect-fluid neutron star model, the paper constructs anisotropic versions via minimal geometric deformation and finds that the least compact models (SAX J1808.4-3658 and Her X-1) are the most stable.