Spin-polarized β-stable neutron star matter: the nuclear symmetry energy and GW170817 constraint

Magnetic field of rotating pulsar might be so strong that the equation of state (EOS) of neutron star (NS) matter is significantly affected by the spin polarization of baryons. In the present work, the EOS of the spin-polarized nuclear matter is investigated in the nonrelativistic Hartree-Fock forma...

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Bibliographic Details
Main Authors: Ngo Hai Tan, ,, Dao T. Khoa, Doan Thi Loan
Format: Article
Language:English
Published: 2020
Subjects:
Online Access:https://dlib.phenikaa-uni.edu.vn/handle/PNK/585
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