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Polarisation indication of the movement of particles in a dispersion medium,caused by light pressure

机译:偏光指示颗粒在分散介质中的运动,由轻压力引起

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Absorption of light by a dispersion medium as well as its reflection and refraction at the boundary are accompanied by the appearance of mechanical forces acting on the particles as a light pressure.The light pressure was measured experimentally for the first time by P.N.Lebedev more than hundred years ago in exceptionally fine experiments.When laser sources of powerful light radiation appeared,the fields on investigation and use of light pressure widened substantially (see,for example,Afanas'ev & Katarkevich,Rubinov,Efendiev,2002).In recent years,investigations of light pressure concerned very different fields from astrophysics for explanation the effect of rotation of cosmic dust particles to biology for manipulation by individual cells.Despite the tempting perspectives of application,the theory of light pressure and movement of-particles of a medium under its action in the conditions of multiple scattered light in the medium was practically not developed till now.This is explained by the complexity of the process of interaction of light radiation with an individual particle and the limited possibilities of the radiative transfer theory which gives analytical solutions only for case of coarse idealisations.The main difficulty that is considered as insuperable in analytical solving the problem is,as known,the necessity of taking into account an infinitely large number of terms when the scattering indicatrix is expanded in terms of orthogonal functions.
机译:分散介质对光的吸收以及在边界处的反射和折射都伴随着机械力的出现,即作为光压作用在粒子上。PNLebedev首次对光压进行了实验测量几年前,在非常精细的实验中。当强大的光辐射的激光源出现时,光压研究和使用的领域大大拓宽了(例如,参见Afanas'ev和Katarkevich,Rubinov,Efendiev,2002)。光压的研究涉及与天体物理学截然不同的领域,以解释宇宙尘埃粒子的旋转对生物学的影响,以单个细胞进行操纵。尽管有诱人的应用前景,光压理论和介质在其下的粒子运动到目前为止,在介质中存在多种散射光的情况下,几乎还没有产生任何作用。光辐射与单个粒子相互作用过程的复杂性以及辐射传递理论的可能性有限,该理论仅在粗糙理想化的情况下提供了解析解。在解析解决问题时被认为是不可克服的主要困难是:众所周知,当散射指标根据正交函数展开时,必须考虑无限多个项。

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