The polarization force and the charge-gradient force effects in strongly coupled dusty plasma along with the effects of viscosity are studied using theoretical techniques. The strongly coupled dusty medium is suitably described by the simplified phenomenological fluid model. The plasma model is considered to compose of Maxwellian distribution of ions and radiative electrons along with comparatively massive dust grains. With the Generalized Hydrodynamic (GHD) fluid model, the dispersion relation is deduced and the collective properties of the medium are discussed. The viscoelastic and low frequency modes of the waves derived from the dispersion relation and the instabilities of the plasma are inspected in detail to understand the hydrodynamic mode of propagation and the kinetic mode of propagation.
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24 April 2019
PROF. DINESH VARSHNEY MEMORIAL NATIONAL CONFERENCE ON PHYSICS AND CHEMISTRY OF MATERIALS: NCPCM 2018
27–28 December 2018
Indore, India
Research Article|
April 24 2019
Kinetic and hydrodynamic modes of propagation in strongly coupled dusty plasma with radiative effects
Linda Xavier;
Linda Xavier
a)
Physics Department, Ujjain Engineering College
, Ujjain, M. P. - 456010, India
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Archana Patidar;
Archana Patidar
b)
Physics Department, Ujjain Engineering College
, Ujjain, M. P. - 456010, India
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Prerana Sharma
Prerana Sharma
c)
Physics Department, Ujjain Engineering College
, Ujjain, M. P. - 456010, India
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AIP Conf. Proc. 2100, 020169 (2019)
Citation
Linda Xavier, Archana Patidar, Prerana Sharma; Kinetic and hydrodynamic modes of propagation in strongly coupled dusty plasma with radiative effects. AIP Conf. Proc. 24 April 2019; 2100 (1): 020169. https://doi.org/10.1063/1.5098723
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