1991
DOI: 10.1007/bf00646951
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Gravitational instability of a heat-conducting plasma

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Cited by 18 publications
(12 citation statements)
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“…Equation represents the general dispersion relation for an infinitely conducting Walters B′ viscoelastic and self‐gravitating rotating fluid with pressure anisotropy through Brinkman porous medium in the presence of a uniform magnetic field and heat flux vector. Note that, in the absence of porous medium and kinematic viscoelasticity, (i) if we ignore the effect of rotation, the dispersion relation can be easily verified with other previous results obtained and (ii) if we ignore the effects of rotation and self‐gravitation, the dispersion relation agrees with that obtained earlier by Kalra et al . On removing the effects of kinematic viscoelasticity and porous medium terms ( μ = μ ′ = 0, ε = 1 and k 1 → ∞ ), Eq.…”
Section: Dispersion Relationsupporting
confidence: 89%
“…Equation represents the general dispersion relation for an infinitely conducting Walters B′ viscoelastic and self‐gravitating rotating fluid with pressure anisotropy through Brinkman porous medium in the presence of a uniform magnetic field and heat flux vector. Note that, in the absence of porous medium and kinematic viscoelasticity, (i) if we ignore the effect of rotation, the dispersion relation can be easily verified with other previous results obtained and (ii) if we ignore the effects of rotation and self‐gravitation, the dispersion relation agrees with that obtained earlier by Kalra et al . On removing the effects of kinematic viscoelasticity and porous medium terms ( μ = μ ′ = 0, ε = 1 and k 1 → ∞ ), Eq.…”
Section: Dispersion Relationsupporting
confidence: 89%
“…In the absence of viscosity, this equation shows exactly the same relation as obtained by Singh and Kalra (1986) and Bora and Nayyar (1991).…”
Section: Propagation Perpendicular To the Magnetic Fieldsupporting
confidence: 78%
“…The equations for a gravitating, anisotropic, heat-conducting, infinite plasma are written as (Bora and Nayyar 1991) d dt The equations for a gravitating, anisotropic, heat-conducting, infinite plasma are written as (Bora and Nayyar 1991) d dt…”
Section: Basic Equationsmentioning
confidence: 99%
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“…Many authors [3][4][5][6][7][8] have investigated the problems of astrophysical interest in anisotropic collisionless plasma. It is an established fact that rotation has played an important role in the theory of star formation and fragmentation of the protostellar dusty clouds.…”
Section: Introductionmentioning
confidence: 99%