Relativisitic non-pascalian fluid as a density contribution

Anisotropy of local pressure distribution and dissipation are essential in understanding the evolution of the internal structure of compact objects and their observable characteristics. In this work, we reinterpret local pressure anisotropy in relativistic stellar structures as a contribution to the...

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Hauptverfasser: Ospino, Justo, Suárez-Urango, Daniel, Becerra, Laura M, Hernández, Héctor, Núñez, Luis A
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Sprache:eng
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