Magnetic susceptibility and magnetization properties of asymmetric nuclear matter in a strong magnetic field

被引:28
作者
Rabhi, A. [1 ,2 ]
Perez-Garcia, M. A. [3 ,4 ]
Providencia, C. [1 ]
Vidana, I. [1 ]
机构
[1] Univ Coimbra, Dept Phys, Ctr Fis Computac, P-3004516 Coimbra, Portugal
[2] Univ Tunis El Manar, Unite Rech Phys Nucl & Hautes Energies, Fac Sci Tunis, Tunis 2092, Tunisia
[3] Univ Salamanca, Dept Fis Fundamental, E-37008 Salamanca, Spain
[4] Univ Salamanca, IUFFyM, E-37008 Salamanca, Spain
来源
PHYSICAL REVIEW C | 2015年 / 91卷 / 04期
关键词
POLARIZED NEUTRON MATTER; FERROMAGNETISM; STARS; PARAMETERS; EQUATION; PHYSICS; MODELS; STATE;
D O I
10.1103/PhysRevC.91.045803
中图分类号
O57 [原子核物理学、高能物理学];
学科分类号
070202 ;
摘要
We study the effects of a strong magnetic field on the proton and neutron spin polarization and magnetic susceptibility of asymmetric nuclear matter within a relativistic mean-field approach. It is shown that magnetic fields B similar to 10(16)-10(17) G have noticeable effects on the range of densities of interest for the study of the crust of a neutron star. Although the proton susceptibility is larger for weaker fields, the neutron susceptibility becomes of the same order or even larger for small proton fractions and subsaturation densities for B > 10(16) G. We expect that neutron superfluidity in the crust will be affected by the presence of magnetic fields.
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页数:13
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