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球体上驻波辐射力的对比度因子:以球体半径的幂次进行级数展开。

Contrast factor for standing-wave radiation forces on spheres: Series expansion in powers of sphere radius.

作者信息

Marston Philip L

机构信息

Physics and Astronomy Department, Washington State University, Pullman, Washington 99164-2814,

出版信息

JASA Express Lett. 2024 Jul 1;4(7). doi: 10.1121/10.0027928.

DOI:10.1121/10.0027928
PMID:39007701
Abstract

Recently researchers often normalize the radiation force on spheres in standing waves in inviscid fluids using an acoustic contrast factor (typically denoted by Φ) that is independent of kR where k is the wave number and R is the sphere radius. An alternative normalization uses a function Ys that depends on kR. Here, standard results for Φ are extended as a power series in kR using prior Ys results. Also, new terms are found for fluid spheres and applied to the kR dependence of Φ for strongly responsive and weakly responsive examples. Partial-wave phase shifts are used in the derivation.

摘要

最近,研究人员经常使用一个与波数(k)和球体半径(R)的乘积(kR)无关的声学对比度因子(通常用(\varPhi)表示),对无粘性流体中驻波作用于球体的辐射力进行归一化处理。另一种归一化方法使用的是依赖于(kR)的函数(Y_s)。在此,利用先前关于(Y_s)的结果,将(\varPhi)的标准结果扩展为(kR)的幂级数。此外,还发现了适用于流体球体的新项,并将其应用于强响应和弱响应示例中(\varPhi)对(kR)的依赖性。推导过程中使用了分波相移。

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