Jeans instability of dark-baryonic matter model in the context of Kaniadakis' statistic distribution

Figures & data

Figure 1. The normalized frequency ${\omega }_{\ast }=\gamma /\sqrt{4\pi G{\rho }_d^0}$ versus the normalized wave number $k_{\ast }=k/k_{Jd}$ with different $\kappa$ and the fixed value of ${\sigma }_{\ast }=1.83$, ${\rho }_{\ast }=5.47$.

Figure 2. The normalized frequency ${\mathrm{\Omega }}_{\ast }=\gamma /\sqrt{4\pi G{\rho }_b^0}$ versus the normalized wave number $K_{\ast }=k/k_{Jb}$ with different ${\rho }_{\ast }$ and the fixed value of $\kappa =0.2$, ${\sigma }_{\ast }=1.83$.