2019
DOI: 10.1134/s1063780x19070109
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Radiative and Gravitational Modes and Instabilities in an Inhomogeneous Magneto Dusty Plasma with Charge Variation

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Cited by 2 publications
(5 citation statements)
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“…We numerically analyze the dispersion relation (25) to see how the ionization, recombination, polarization force, neutral dynamics and dust thermal velocity modify the growth rate of instabilities. For the numerical estimation, equation (25) is written in dimensionless form as For numerical calculations we have chosen the typical plasma parameters from [34,38,40,41] which are found in various astrophysical dusty plasma situations. In order to analyze the effects of various parameters on the growth rate of instabilities, we have plotted the real positive values of dimensionless growth rate of equation (34) versus the normalized wave number.…”
Section: Numerical Estimationmentioning
confidence: 99%
See 3 more Smart Citations
“…We numerically analyze the dispersion relation (25) to see how the ionization, recombination, polarization force, neutral dynamics and dust thermal velocity modify the growth rate of instabilities. For the numerical estimation, equation (25) is written in dimensionless form as For numerical calculations we have chosen the typical plasma parameters from [34,38,40,41] which are found in various astrophysical dusty plasma situations. In order to analyze the effects of various parameters on the growth rate of instabilities, we have plotted the real positive values of dimensionless growth rate of equation (34) versus the normalized wave number.…”
Section: Numerical Estimationmentioning
confidence: 99%
“…For the numerical estimation, equation (25) is written in dimensionless form as For numerical calculations we have chosen the typical plasma parameters from [34,38,40,41] which are found in various astrophysical dusty plasma situations. In order to analyze the effects of various parameters on the growth rate of instabilities, we have plotted the real positive values of dimensionless growth rate of equation (34) versus the normalized wave number. The results are presented in the form of figures 1-7.…”
Section: Numerical Estimationmentioning
confidence: 99%
See 2 more Smart Citations
“…In another effort to understand polarization force, Asaduzzaman et al [34] studied linear modes of dust acoustic waves in a non-uniform dusty plasma in the presence of such a polarizing force. The gravitational instability of magnetized dusty plasmas with collisional effects is studied including dust polarization force and dust charge variation along with radiatively cooled electron and ions by Sharma et al [35]. Saini et al [36] analytically examined the dust acoustic shock waves in dusty plasma considering polarization force.…”
Section: Introductionmentioning
confidence: 99%