Yaroshenko V V, Jacobs G, Verheest F
Sterrenkundig Observatorium, Universiteit Gent, Krijgslaan 281, B-9000 Gent, Belgium.
Phys Rev E Stat Nonlin Soft Matter Phys. 2001 Sep;64(3 Pt 2):036401. doi: 10.1103/PhysRevE.64.036401. Epub 2001 Aug 14.
Using a kinetic description, dust-acoustic waves are considered for dusty plasmas containing, besides the electrons and ions, dust particles with continuous mass (size) distributions. For broad size spectra, self-gravitational effects cannot be neglected anymore because in the competition between electromagnetic and gravitational forces, the scale tips over towards gravitation for the heavier dust grains. Self-gravitational effects are clearly interwoven with the grain size distribution and here the effects of different power-law size distributions on the propagation, damping, and instability of low-frequency waves are discussed.
利用动力学描述,研究了除电子和离子外还包含具有连续质量(尺寸)分布的尘埃颗粒的尘埃等离子体中的尘埃声波。对于宽尺寸谱,自引力效应不再能被忽略,因为在电磁力和引力的竞争中,对于较重的尘埃颗粒,尺度向引力倾斜。自引力效应显然与颗粒尺寸分布相互交织,这里讨论了不同幂律尺寸分布对低频波传播、阻尼和不稳定性的影响。