Suppr超能文献

非线性多模波导系统中光轨道角动量的热化

Thermalization of Light's Orbital Angular Momentum in Nonlinear Multimode Waveguide Systems.

作者信息

Wu Fan O, Zhong Qi, Ren Huizhong, Jung Pawel S, Makris Konstantinos G, Christodoulides Demetrios N

机构信息

CREOL/College of Optics and Photonics, University of Central Florida, Orlando, Florida 32816, USA.

Faculty of Physics, Warsaw University of Technology, Koszykowa 75, 00-662 Warsaw, Poland.

出版信息

Phys Rev Lett. 2022 Mar 25;128(12):123901. doi: 10.1103/PhysRevLett.128.123901.

Abstract

We show that the orbital angular momentum (OAM) of a light field can be thermalized in a nonlinear cylindrical multimode optical waveguide. We find that upon thermal equilibrium, the maximization of the optical entropy leads to a generalized Rayleigh-Jeans distribution that governs the power modal occupancies with respect to the discrete OAM charge numbers. This distribution is characterized by a temperature that is by nature different from that associated with the longitudinal electromagnetic momentum flow of the optical field. Counterintuitively and in contrast to previous results, we demonstrate that even under positive temperatures, the ground state of the fiber is not always the most populated in terms of power. Instead, because of OAM, the thermalization processes may favor higher-order modes. A new equation of state is derived along with an extended Euler equation resulting from the extensivity of the entropy itself. By monitoring the nonlinear interaction between two multimode optical wave fronts with opposite spins, we show that the exchange of angular momentum is dictated by the difference in OAM temperatures, in full accord with the second law of thermodynamics. The theoretical analysis presented here is corroborated by numerical simulations that take into account the complex nonlinear dynamics of hundreds of modes. Our results may pave the way toward high-power optical sources with controllable orbital angular momenta, and at a more fundamental level, they may open up opportunities in drawing parallels with other complex multimode nonlinear systems like rotating atomic clouds.

摘要

我们表明,光场的轨道角动量(OAM)可在非线性圆柱形多模光波导中实现热化。我们发现,在热平衡时,光学熵的最大化会导致一种广义瑞利 - 金斯分布,该分布支配着相对于离散OAM电荷数的功率模态占有率。这种分布的特征在于一个本质上不同于与光场纵向电磁动量流相关的温度。与直觉相反且与先前结果不同的是,我们证明即使在正温度下,光纤的基态在功率方面也并非总是占据最多。相反,由于OAM,热化过程可能有利于高阶模。我们推导了一个新的状态方程以及一个由熵本身的广延性产生的扩展欧拉方程。通过监测具有相反自旋的两个多模光波前之间的非线性相互作用,我们表明角动量的交换由OAM温度的差异决定,这完全符合热力学第二定律。这里给出的理论分析得到了考虑数百个模式的复杂非线性动力学的数值模拟的证实。我们的结果可能为具有可控轨道角动量的高功率光源铺平道路,并且在更基础的层面上,它们可能为与旋转原子云等其他复杂多模非线性系统进行类比开辟机会。

文献检索

告别复杂PubMed语法,用中文像聊天一样搜索,搜遍4000万医学文献。AI智能推荐,让科研检索更轻松。

立即免费搜索

文件翻译

保留排版,准确专业,支持PDF/Word/PPT等文件格式,支持 12+语言互译。

免费翻译文档

深度研究

AI帮你快速写综述,25分钟生成高质量综述,智能提取关键信息,辅助科研写作。

立即免费体验