任意引力场中扭曲粒子的内禀轨道角动量旋转与轨道霍尔效应
Rotation of intrinsic orbital angular momentum and the orbital Hall effect for twisted particles in arbitrary gravitational fields
AI总结：
本文研究任意引力场中扭曲粒子的内禀轨道角动量旋转与轨道霍尔效应，推导适用于任意 Riemannian 时空的 OAM 动力学精确方程，并给出统一描述。
摘要：
针对任意引力场中的扭曲粒子，本文在一般情形下解决了内禀轨道角动量旋转和轨道霍尔效应问题。在描述扭曲光子时，无需使用弯曲时空中的 Maxwell 方程。文中推导了严格定义任意 Riemannian 时空中 OAM 动力学的精确一般方程，并给出了任意扭曲粒子轨道霍尔效应不同表现形式的一般描述。简要分析表明，所得结果可具有重要实际应用。
英文摘要：
For twisted particles in arbitrary gravitational fields, the problems of the rotation of intrinsic orbital angular momentum and the orbital Hall effect are solved in the general case. We need not use the Maxwell equations in curved spacetimes for a description of twisted photons. The exact general equation rigorously defining the OAM dynamics in any Riemannian spacetimes is derived. The general description of different manifestations of the orbital Hall effect for any twisted particles is also presented. Our short analysis shows that the results obtained can find important practical applications.
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。
