Gravitational Instability of Rotating Viscoelastic Partially Ionized Plasma in the Presence of an Oblique Magnetic Field and Hall Current

Table 4

Variation of 𝑊, given by (14), with the wavenumber for different values of 𝑣_𝑐. At 𝜇^=0.1 gm cm⁻¹ sec⁻², 𝜇=0.1 gm cm⁻¹ sec⁻¹, 𝜂=1 mH cm⁻¹, Ω=0.05 rad sec⁻¹, 𝐿=0.1 cm² sec⁻¹, 𝜌_𝑑=0.001 gm cm⁻³, 𝜃=0^∘, and 𝐻_𝑧=0.1 Amp cm⁻¹.

𝑘	𝑣𝑐=0.1	𝑣𝑐=0.1	𝑣𝑐=0.2
0.1	1.36664	1.423	1.47494
0.2	1.31426	1.32782	1.33983
0.3	1.2968	1.30284	1.30814
0.4	1.28205	1.28547	1.28847
0.5	1.26666	1.26887	1.27081
0.6	1.25032	1.25188	1.25325
0.7	1.23339	1.23455	1.23556
0.8	1.21631	1.21722	1.218
0.9	1.19955	1.20027	1.20089
1	1.18344	1.18403	1.18454