Neutron stars velocities and magnetic fields
Keyword(s):
We study a model that explain neutron stars velocities due to the anisotropic emission of neutrinos. Strong magnetic fields present in neutron stars are the source of the anisotropy in the system. To compute the velocity of the neutron star we model its core as composed by strange quark matter and analice the properties of a magnetized quark gas at finite temperature and density. Specifically we have obtained the electron polarization and the specific heat of magnetized fermions as a functions of the temperature, chemical potential and magnetic field which allow us to study the velocity of the neutron star as a function of these parameters.
2000 ◽
Vol 195
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pp. 245-254
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1994 ◽
Vol 03
(03)
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pp. 665-674
2017 ◽
Vol 13
(S337)
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pp. 213-216
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1996 ◽
Vol 160
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pp. 135-136
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2020 ◽
Vol 496
(4)
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pp. 5052-5071
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1996 ◽
Vol 10
(23)
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pp. 1141-1149
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2019 ◽
Vol 34
(29)
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pp. 1950170