In the present work, we have obtained the equation of state for neutron star matter considering the in uence of the ferromagnetic and antiferromagnetic spin state. We have also investigated the structure of neutron stars. According to our results, the spin asymmetry sti ens the equation of state and leads to high mass for the neutron star.
Bigdeli, M., Roohi, N., & Zamani, M. (2016). Spin and Isospin Asymmetry, Equation of State and Neutron Stars. Iranian Journal of Astronomy and Astrophysics, 3(2), 73-80. doi: 10.22128/ijaa.2016.60
MLA
Mohsen Bigdeli; Nariman Roohi; Mina Zamani. "Spin and Isospin Asymmetry, Equation of State and Neutron Stars", Iranian Journal of Astronomy and Astrophysics, 3, 2, 2016, 73-80. doi: 10.22128/ijaa.2016.60
HARVARD
Bigdeli, M., Roohi, N., Zamani, M. (2016). 'Spin and Isospin Asymmetry, Equation of State and Neutron Stars', Iranian Journal of Astronomy and Astrophysics, 3(2), pp. 73-80. doi: 10.22128/ijaa.2016.60
VANCOUVER
Bigdeli, M., Roohi, N., Zamani, M. Spin and Isospin Asymmetry, Equation of State and Neutron Stars. Iranian Journal of Astronomy and Astrophysics, 2016; 3(2): 73-80. doi: 10.22128/ijaa.2016.60
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