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.

1.
D.
Banerjee
,
J. S.
Mylavarapu
, and
N.
Chakrabarti
,
Physics of Plasmas
17
,
113708
(
2010
)
2.
F.
Verheest
,
Waves in dusty space plasma
(
Kluwer Academic
,
Dordrecht
,
2000
).
3.
H.
Ikeji
,
Phys. Fluids
29
,
1764
(
1986
).
4.
G.
Ogilvie
and
A. T.
Potter
,
Phys. Rev Lett.
100
,
74503
(
2008
).
5.
P. K.
Kaw
and
A.
Sen
,
Phys. Plasmas
5
,
10
,
3552
(
1998
).
6.
S.
Nunomura
,
D.
Samsonov
, and
J.
Goree
,
Phys. Rev. Lett.
84
,
22
,
5141
(
2000
).
7.
J.
Pramanik
,
G.
Prasad
,
A.
Sen
, and
P. K.
Kaw
,
Phys. Rev. Lett.
88
,
17
,
175001
(
2002
)
8.
S. A.
Khrapak
and
Hubertus M.
Thomas
Phys. Rev. E
91
,
033110
(
2015
).
9.
A. G.
Khrapak
and
S. A.
Khrapak
,
Phys. Plasmas
25
,
034502
(
2018
).
10.
P.
Sharma
,
Eur. Phys. Lett.
107
15001
(
2014
).
This content is only available via PDF.
You do not currently have access to this content.