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arXiv · 1911.10224

Modeling anisotropic magnetized strange quark stars

S. López Pérez·D. Manreza Paret·G. Quintero Angulo·A. Pérez Martínez·D. Alvear Terrero
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Abstract

Compact objects have an intrinsic anisotropy due to the presence of strong magnetic fields that cause considerable modifications on the equations of state (EoS). In this work, we study the impact of this anisotropy in the size and shape of magnetized strange quark stars using an axially symmetric metric in spherical coordinates, the gamma-metric. The results are compared with those obtained with the standard Tolman-Oppenheimer-Volkoff (TOV) equations for the parallel and perpendicular pressures independently. Differences in the results are discussed.

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S. López Pérez, D. Manreza Paret, G. Quintero Angulo, A. Pérez Martínez, D. Alvear Terrero. 2019-11-22. Modeling anisotropic magnetized strange quark stars. https://doi.org/10.1002/asna.201913721

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