I. Introduction
The physics of dusty plasma has gained much interest and rapid maturation during the last two decades. Their widespread occurrence in diverse environments [1]–[4] makes them as one of the best candidates for the understanding of the underlying physics of space and astrophysical observations, as well as laboratory experiments. In addition to electrons and ions, a dusty plasma contains highly charged and massive particulates [5]–[7]. The presence of dust grains can significantly alter the properties and behavior of a plasma in which they are immersed [4], [8]. It affects all kinds of plasma wave modes and, remarkably, gives rise to new, very low-frequency dust modes. The dust-acoustic wave (DAW) is one such new mode [9], peculiar to this system with the dust particles providing inertia and the pressure contributions for sustaining the wave, coming from both the lighter species (the electrons and the ions).