Instituto de Plasmas e Fusão Nuclear--Laboratório Associado, Instituto Superior Tecnico,Avenida Rovisco Pais 1, 1049-001 Lisboa, Portugal.
Phys Rev Lett. 2010 Jul 16;105(3):035001. doi: 10.1103/PhysRevLett.105.035001. Epub 2010 Jul 12.
The inverse Faraday effect is usually associated with circularly polarized radiation; here, we show that it can also occur for linearly polarized radiation. The quasistatic axial magnetic field generated by a laser propagating in plasma can be calculated by considering both the spin and the orbital angular momenta of the laser pulse. A net spin is present when the radiation is circularly polarized and a net orbital angular momentum is present if there is any deviation from perfect rotational symmetry. The orbital angular momentum gives an additional contribution to the axial magnetic field that can enhance or reduce the effect usually attributed to circular polarization and strongly depends on the intensity profile of the Laguerre-Gaussian modes involving the azimuthal and radial mode numbers.
反法拉第效应通常与圆偏振辐射有关;在这里,我们表明它也可能发生在线偏振辐射中。当激光在等离子体中传播时,由激光脉冲的自旋和轨道角动量产生的准静态轴向磁场可以通过考虑这两个角动量来计算。当辐射为圆偏振时,存在净自旋,而当存在任何偏离完美旋转对称时,存在净轨道角动量。轨道角动量对轴向磁场有额外的贡献,可以增强或减少通常归因于圆偏振的效应,并且强烈依赖于涉及轨道角动量和径向模数的拉盖尔-高斯模的强度分布。