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Maximum mass of magnetic white dwarfs

Research in Astronomy and Astrophysics 2015年第10期15卷 1735-1741页

作者： daryel manreza paret Jorge Ernesto Horvath Aurora Pérez Martínez Departamento de Fisica General Facultad de FísicaUniversidad de la Habana Instituto de Astronomia Geofisica e Ciencias Atmosfericas USP Instituto de Cibernética Matemática y Física(ICIMAF)

We revisit the problem of the maximum masses of magnetized white dwarfs （WDs）. The impact of a strong magnetic field on the structure equations is addressed. The pressures become anisotropic due to the presence of the magnetic field and split into parallel and perpendicular components. We first construct stable solutions of the Tolman-Oppenheimer-Volkoff equations for parallel pressures and find that physical solutions vanish for the perpendicular pressure whenB ≥ 10^13 G. This fact estab- lishes an upper bound for a magnetic field and the stability of the configurations in the （quasi） spherical approximation. Our findings also indicate that it is not possible to obtain stable magnetized WDs with super-Chandrasekhar masses because the val- ues of the magnetic field needed for them are higher than this bound. To proceed into the anisotropic regime, we can apply results for structure equations appropriate for a cylindrical metric with anisotropic pressures that were derived in our previous work. From the solutions of the structure equations in cylindrical symmetry we have con- firmed the same bound for B- 10^13 G, since beyond this value no physical solutions are possible. Our tentative conclusion is that massive WDs with masses well beyond the Chandrasekhar limit do not constitute stable solutions and should not exist.

关键词： magnetic fields -- white dwarfs -- equation of state

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Anisotropic stellar structure equations for magnetized strange stars

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Research in Astronomy and Astrophysics 2015年第7期15卷 975-985页

作者： daryel manreza paret Jorge Ernesto Horvath Aurora Pérez Mart'nez Departamento de F'sica General Facultad de F'sica Universidad de la Habana Instituto de Astronomia Geofisica e Ciencias Atmosfericas USP Instituto de Cibernética Matemática y Física (ICIMAF)

The fact that a fermion system in an external magnetic field breaks the spherical symmetry suggests that its intrinsic geometry is axisymmetric rather than spherical. In this work we analyze the impact of anisotropic pressures, due to the presence of a magnetic field, in the structure equations of a magnetized quark *** assume a cylindrical metric and an anisotropic energy momentum tensor for the source. We found that there is a maximum magnetic field that a strange star can sustain, closely related to the violation of the virial relations.

关键词： magnetic fields -- stars: neutron -- equation of state

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