Equations of State for Hadronic Matter and Mass-Radius Relations of Neutron Stars with Strong Magnetic Fields
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Neutron star is an important object for us to verify the equation of state of hadronic matter. For a specific choice of equations of state, mass and radius of a neutron star are determined, for which there are constraints from observations. According to some previous studies, since the strong magnetic field acts as a repulsive force, there is a possibility that neutron stars with strong magnetic fields may have relatively heavier masses than other non-magnetized neutron stars. In this paper, the structure of a neutron star with a strong internal magnetic field is investigated by changing its internal functional form to see how much the neutron star can be massive and also how radius of a neutron star can be within a certain range.
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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2020 ◽
Vol 496
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pp. 5052-5071
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1996 ◽
Vol 10
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pp. 1141-1149
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