“…The concept of two-temperature electrons (electrons with two distinct temperatures) is now well established from the theoretical [34][35][36][37][38] and experimental [39,40] points of view. Thus, at equilibrium the quasineutrality condition implies, n i0 = n e10 + n e20 + Z d n d0 , where n s0 is the unperturbed number densities of the species s (here s = i, e1, e2, d for ion, electrons with temperature T e1 , electrons with temperature T e2 , and immobile dust, respectively) and Z d is the number of electrons residing onto the dust grain surface.…”