论文标题
磁铁中强弹性磁场的起源
Origin of the Strong Toroidal Magnetic Field in Magnetars
论文作者
论文摘要
提出了一种简单的手性不对称模型来解释强弹性磁场的起源。与形成该场的动力学相关的电子在具有超相关的费米能的量子退化状态。使用缩放的H-bar方法通过Dirac Hartree Fock方法描述了该系统。中子星正在旋转并具有较大的角动量，这是由曲柄模型形成并破坏时间逆转的。由于克利福德的数字，狄拉克电流被分解为对流和自旋电流。强弹性磁场是由旋转形成的，就像电流一样，由手性不对称产生的电流导致了由均衡弱弱相互作用引起的电子捕获。
A simple model of chiral asymmetry is proposed to interpret the origin of the strong toroidal magnetic field. The electrons relevant to dynamics forming the the field are in a quantume degenerate state with ultra-relativistic Fermi energy. The system is described by Dirac Hartree Fock method using scaled h-bar method. Neutron stars are rotating and have large angular momentum which is formed by cranking model and breaks time reversal. Dirac current is decomposed into convection and spin currents due to Clifford number. The strong toroidal magnetic field is formed by the spin like current resulted by the chiral asymmetry brought about electron capture caused by the parity-violating weak interaction.
