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arXiv 0908.1368nucl-thastro-ph.HE
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强磁场中中子物质的自旋极化态

Spin polarized states in neutron matter at a strong magnetic field

A. A. Isayev, J. Yang

摘要:

在Skyrme有效相互作用(SLy 4,SLy 7参数化)模型中考虑了强磁场中中子物质的自旋极化态。分析零温下的自洽方程,结果表明,当大多数中子自旋与磁场方向相反时,自旋极化参数作为密度函数的热力学稳定解分支对应于负自旋极化。此外,从依赖于磁场强度的阈值密度出发,自洽方程还具有自旋极化参数为正的两个分支(上、下)解。对应于上分支的自由能非常接近对应于具有负自旋极化的自旋优选分支的自由能。因此,在强磁场下,具有正自旋极化的状态可以在中子物质的高密度区实现为亚稳态,在密度降低到某个阈值密度时,中子物质转变为具有负自旋极化的自旋稳定状态。计算了中子自旋极化参数和中子能量随磁场强度的变化,结果表明,当磁场强度达到$10^{17}$ G时,磁场的影响仍然很小。

英文摘要:

Spin polarized states in neutron matter at a strong magnetic field are considered in the model with the Skyrme effective interaction (SLy4, SLy7 parametrizations). Analyzing the self-consistent equations at zero temperature, it is shown that a thermodynamically stable branch of solutions for the spin polarization parameter as a function of density corresponds to the negative spin polarization when the majority of neutron spins are oriented oppositely to the direction of the magnetic field. Besides, beginning from some threshold density being dependent on the magnetic field strength the self-consistent equations have also two other branches (upper and lower) of solutions for the spin polarization parameter with the positive spin polarization. The free energy corresponding to the upper branch turns out to be very close to the free energy corresponding to the thermodynamically preferable branch with the negative spin polarization. As a consequence, at a strong magnetic field, the state with the positive spin polarization can be realized as a metastable state at the high density region in neutron matter which under decreasing density at some threshold density changes into a thermodynamically stable state with the negative spin polarization. The calculations of the neutron spin polarization parameter and energy per neutron as functions of the magnetic field strength show that the influence of the magnetic field remains small at the field strengths up to $10^{17}$ G.

机构、总结、中文摘要均由AI分析而来,可能存在错误,请以论文正文为准。

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