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arXiv · 1307.7450

Hyperon Stars in Strong Magnetic Fields

R. O. Gomes·V. Dexheimer·C. A. Z. Vasconcellos
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Abstract

We investigate the effects of strong magnetic fields on the properties of hyperon stars. The matter is described by a hadronic model with parametric coupling. The matter is considered to be at zero temperature, charge neutral, beta-equilibrated, containing the baryonic octet, electrons and muons. The charged particles have their orbital motions Landau-quantized in the presence of strong magnetic fields (SMF). Two parametrisations of a chemical potential dependent static magnetic field are considered, reaching $1-2 \times 10^{18}\,G$ in the center of the star. Finally, the Tolman-Oppenheimer-Volkov (TOV) equations are solved to obtain the mass-radius relation and population of the stars.

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R. O. Gomes, V. Dexheimer, C. A. Z. Vasconcellos. 2013-07-29. Hyperon Stars in Strong Magnetic Fields. https://arxiv.org/abs/1307.7450

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