“…In laboratory experiments and most of the astrophysical environments (Arshad and Mahmood, 2010; the charged particles exhibit non-Maxwellian or non-thermal distribution. These non-Maxwellian distributions are well reproduced by the power-laws or the so-called Kappa distribution functions (Pierrard and Lazar, 2010;Lazar et al, 2012), which recently were applied for modeling the twisted plasma waves, such as Langmuir (electron) twisted waves and ion acoustic twisted waves (Arshad et al, 2016). In space special form of plasma like permeating plasmas (Arshad et al, 2014a,b,c), streaming plasmas (Novo et al, 2015;Lazar et al, 2008;Youdin et al, 2005;Bret, 2009;Khalil, 2015;Torney et al, 2006) and drifting plasmas (Davidson, 2014) exhibit various novel instabilities in the presence of neutral and charged dust particles.…”