期刊
ASTRONOMISCHE NACHRICHTEN
卷 335, 期 6-7, 页码 666-671出版社
WILEY-V C H VERLAG GMBH
DOI: 10.1002/asna.201412090
关键词
equation of state; elementary particles; magnetic fields; stars: neutron
In this contribution we study the effects of strong magnetic fields on the particle population of neutron stars with hyperon degrees of freedom in their composition. The star matter is described by a multi-component model with parameterized baryon-meson interaction couplings. We study the magnetic effects on the equation of state (EoS) due to the Landau quantization, assuming a density dependent static magnetic field that reaches about 10 19 G in the center of the star. The Tolman-Oppenheimer-Volkoff equations are solved in order to understand the dependence of the mass-radius relation and hyperon population on the magnetic field intensity assuming different interaction coupling schemes. (C) 2014 WILEY-VCH Verlag GmbH & Co. KGaA, Weinheim
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