Radiation pressure on a moving body: beyond the Doppler effect
Radiation pressure on a moving body: beyond the Doppler effect
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DOI：
10.1364/josab.29.003136
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发表时间：
2011-11
影响因子：
1.9
通讯作者：
S. Horsley;M. Artoni;G. C. Rocca
中科院分区：
文献类型：
--
作者：
S. Horsley;M. Artoni;G. C. Rocca
宏观辐射压力对被推物体速度的依赖通常归因于多普勒效应。这种情况不一定是这样的，这里我们强调速度相关的辐射压力项，它们起源于实验室和材料静止框架之间的洛伦兹变换所带来的s和p极化的混合，而不是频率和波矢量的相应变换。我们发展的理论可能与运动物体的纳米光力学有关。
The dependence of macroscopic radiation pressure on the velocity of the object being pushed is commonly attributed to the Doppler effect. This need not be the case, and here we highlight velocity-dependent radiation pressure terms that have their origins in the mixing of s and p polarizations brought about by the Lorentz transformation between the lab and the material rest frame, rather than in the corresponding transformation of frequency and wavevector. The theory we develop may be relevant to the nano-optomechanics of moving bodies.