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Equations of State for Hadronic Matter and Mass-Radius Relations of Neutron Stars with Strong Magnetic Fields

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 magnet...

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Збережено в:
Бібліографічні деталі
Автори: Chinatsu Watanabe, Naotaka Yoshinaga, Shuichiro Ebata
Формат: Artigo
Мова:Inglês
Опубліковано: MDPI AG 2022-01-01
Серія:Universe
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Онлайн доступ:https://www.mdpi.com/2218-1997/8/1/48
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