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arXiv 2312.01079quant-phnucl-th
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非相对论中子与超短激光脉冲的自旋相互作用

Spin interaction of non-relativistic neutrons with an ultrashort laser pulse

Peter Christian Aichelburg, Christian Spreitzer

AI总结:

本文用非相对论泡利方程研究慢中子与超短激光脉冲的自旋相互作用,通过推导波函数连接条件获得散射振幅,并给出极化中子束的显式表达式和数值估计。

摘要:

利用非相对论泡利方程研究慢中子与短磁脉冲的相互作用。在极端极限下,该脉冲仅在一个时间瞬间作用于中子的磁矩。我们通过推导泡利波函数跨越脉冲时的连接条件,得到了散射振幅。对于一束受到空间恒定磁场强度脉冲作用的极化平面波中子,给出了显式表达式。假设该磁场由超短激光脉冲产生,我们提供了粗略的数值估计。

英文摘要:

The non-relativistic Pauli equation is used to study the interaction of slow neutrons with a short magnetic pulse. In the extreme limit, the pulse is acting on the magnetic moment of the neutron only at one instant of time. We obtain the scattering amplitude by deriving the junction conditions for the Pauli wave function across the pulse. Explicit expressions are given for a beam of polarized plane wave neutrons subjected to a pulse of spatially constant magnetic field strength. Assuming that the magnetic field is generated by an ultrashort laser pulse, we provide crude numerical estimates.

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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