2014
DOI: 10.1007/s12043-014-0827-1
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The effect of positive dust mass on instability in four-component magnetodustyplasma in the presence of polarization force

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Cited by 5 publications
(3 citation statements)
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“…The plasma species (electrons, ions and dust grains) follow the quasi-neutrality condition -= n n Z n e i d d with n j ( j=electron, ion and dust) is the number density of the plasma species and Z d (=Q e, / Q is the dust charge number and e is the electron charge)is the number of electrons present on the dust grain surface. In the present case, we have taken positively charged dust grains whereas for negatively charged dust Z d will be negative [40,42]. In addition, we study a plasma system comprising of Maxwellian distributed ions and electrons and the full hydrodynamic equations of dust grains where the dust charge is not constant.…”
Section: Theoretical Model Equationsmentioning
confidence: 99%
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“…The plasma species (electrons, ions and dust grains) follow the quasi-neutrality condition -= n n Z n e i d d with n j ( j=electron, ion and dust) is the number density of the plasma species and Z d (=Q e, / Q is the dust charge number and e is the electron charge)is the number of electrons present on the dust grain surface. In the present case, we have taken positively charged dust grains whereas for negatively charged dust Z d will be negative [40,42]. In addition, we study a plasma system comprising of Maxwellian distributed ions and electrons and the full hydrodynamic equations of dust grains where the dust charge is not constant.…”
Section: Theoretical Model Equationsmentioning
confidence: 99%
“…They showed that polarization force and the charge gradient force get coupled with the compressional viscoelastic wave mode in the kinetic regime. The dust grains can be found either positively charged or negatively charged or both along with the sufficient amount of neutrals in background [42]. In various space and laboratory plasma systems the presence of positively charged dust with negative dust grains has been established.…”
Section: Introductionmentioning
confidence: 99%
“…This work will be helpful to describe the relaxed structures in different regions of space such as comentary tails [22,37], Jupiter's magnetosphere [22,39], and mesosphere [36]. The plasma model in our manuscript can be used for astrophysical plasmas as well as for experimental observations [74][75][76] that have the same conditions (a magnetized dusty plasmas with electrons, ions, positively and negatively charged dust fluid).…”
Section: Introductionmentioning
confidence: 99%