Jeans instability of finitely conducting radiative rotating plasma with FLR corrections flowing through porous medium

Effect of Finite Ion Larmor Radius (FLR) Corrections on Thermal Instability of Rotating Radiative Porous Astrophysical Plasma in Interstellar Medium (ISM)

“…This dispersion relation ( 27) is alike to that obtained by Prajapati et al [11] without self-gravitation, viscosity, or electron inertia in their instance, in the absence of FLR corrections. There are two independent elements in equation (27). Equation ( 27) first factor results in, a subsidiary stable mode.…”

“…A lot of researchers have explored the problem of thermal instability and Jeans instability with diverse constraints (Vyas & Chhajlani [17], Sharma & Thakur [18], Kaothekar & Chhajlani [19], El-Sayed & Mohamed [20], Rana [21], El-Sayed & Hussein Rana [22], Chand & Rana [23], Kaothekar & Chhajlani [24], Chand et al [25] and Sutar [26]) and shows that porosity of the medium has a stabilizing influence on the growth rate of the medium. Recently Kaothekar [27] has explored the effect of porosity, finite conductivity, rotation and radiative heat-loss functions on Jeans instability of plasma medium. In this manner we see that, porosity of the medium assumes a fundamental part in flimsiness and steadiness assessments of the warm and floating polarized plasma coursing through permeable medium.…”

Transverse Thermal Instability of Radiative Plasma with FLR Corrections for Star Formation in ISM

“…Many researchers (Jukes [27]; Roberts & Taylor [28]; Rosenbluth et al [29]; Singh & Hans [30]; Herrnegger [31]; Sharma [32]; Chhonkar & Bhatia [33]; Devlen & Pekunlu [34]; Kaothekar & Chhajlani [35]; Kaothekar et al [36]; Kaothekar [37]) have discussed the importance of FLR corrections in thermal instability with different parameters. More recently Kaothekar [38] has investigated the problem of Jeans instability of finitely conducting radiative rotating plasma with FLR corrections f lowing through porous medium. Thus it is clear that FLR is a significant restriction in argument of thermal instability and Jeans-gravitational instability.…”

Impacts of Rotation Radiative Heat-loss Functions Porosity with FLR Corrections on Transverse Thermal Instability of Finitely Conducting Plasma in Interstellar Medium (ISM)

“…Many researchers [Roberts & Taylor (1962); Jukes (1964); Rosenbluth et al(1962); Singh & Hans (1965); Herrnegger (1972); Sharma (1974); Chhonkar & Bhatia (1977); Devlen & Pekunlu (2010); ; Kaothekar et al(2016); and Kaothekar (2017) have discussed the importance of FLR corrections in thermal instability with different parameters. More recently Kaothekar (2021) has investigated the problem of Jeans instability of finitely conducting radiative rotating plasma with FLR corrections flowing through porous medium. Thus it is clear that FLR is a noteworthy constraint in conversation of thermal instability and Jeans-gravitational instability.…”

“…Kaothekar (2018) has examined the thermal instability of partially ionized viscous plasma with Hall effect FLR corrections flowing through porous medium. Recently Kaothekar (2021) has explored the problem of transverse thermal instability of radiative plasma with FLR corrections for star formation in ISM. More recently Kaothekar et al (2022) have investigated the problem on effect of rotation and FLR corrections with radiative heat-loss functions on transverse thermal instability of astrophysical porous plasma in interstellar medium (ISM).…”