| 铁磁相变与中子星模型 |
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| 引用本文： | 黄文宏 于久威. 铁磁相变与中子星模型[J]. 北京师范大学学报(自然科学版), 1989, 0(1): 36-41 |
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| 作者姓名： | 黄文宏 于久威 |
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| 作者单位： | 北京师范大学物理系，北京师范大学物理系，北京师范大学物理系 |
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| 摘 要： |
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| 关 键 词： | 铁磁相变 中子星模型 中子物质 |
THE FERROMAGNETIC TRANSITION AND THE NEUTRON STAR MODELS |
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| Huang Wenhong Yu Jiuwei Gao Shanghui. THE FERROMAGNETIC TRANSITION AND THE NEUTRON STAR MODELS[J]. Journal of Beijing Normal University(Natural Science), 1989, 0(1): 36-41 |
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| Authors: | Huang Wenhong Yu Jiuwei Gao Shanghui |
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| Affiliation: | Department of Physics |
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| Abstract: | The effect of each composition of two-body central potential on the critical density for ferromagnetic transition is calculated for neutron matter. The results show that the radius of the hard core plays an important role in the critical density. For neutron matter with M-S interaction, the critical density of the ferromagnetic transition, the equation of state and the neutron star models are calculated. The critical density k_F is 5.45fm~(-1). The maximum mass of the neutron star with the ferromagnetic phase is lower than that without the ferromagnetic phase. |
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| Keywords: | ferromagnetic transition equation of state neutron star model. |
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