A generalized response (dielectric) function for twisted electrostatic waves is derived for an un-magnetized self-gravitating thermal dusty plasma, whose constituents are the Boltzmann-distributed electrons and positive ions in the presence of negatively charged micrometre-sized massive dust particulates. For this purpose, a set of Vlasov-Poisson coupled equations is solved along with the perturbed Laguerre-Gauss distribution function, as well as the electrostatic and gravitational potentials in the limit of paraxial approximation. For plane wave solution, the wavefronts of the dust-acoustic (DA) wave are assumed to have a constant phase with electric and gravitational field lines propagating straight along the propagation axis. On the other hand, non-planar wave solutions show helical (twisted) wavefronts, in which field lines spiral around the propagation axis owing to the azimuthal velocity component to account for the finite orbital angular momentum (OAM) states. The dispersion relation and damping rate for twisted DA waves are studied both analytically and numerically. It is shown that finite OAM states, the dust to electron temperature ratio, and dust self-gravitation effects significantly affect the linear dispersion and Landau damping frequencies. In particular, the phase speed of twisted DA waves is reduced with the variation of the twist parameter (= k/lq ), dust concentration (= n d0 /n i0 ), and dust self-gravitation (= Jd / pd ). The relevance of our findings to interstellar dust clouds is also discussed for micrometre-sized massive dust grains. KEYWORDS dusty plasma, electrostatic twisted waves, landau damping, orbital angular momentum
INTRODUCTIONLight beam exchanges its energy and momentum [1] with matter upon interaction with it. The total angular momentum of the light beam can be composed of spin and orbital parts due to planar and helical wavefronts, respectively. In other words, the spin and orbital angular momenta have their origin from the polarization states and azimuthal phase structure, which are the well-known properties of polarized light beams. Using a specific experimental set-up, Beth [2] was the first to verify Poynting's idea and measure the mechanical torque of circularly polarized light by transferring the angular momentum to a half-wave plate. Later, Allen et al. [3] ) discussed a theoretical model for calculating the average angular momentum density per unit power and studied the well-defined orbital angular momentum (OAM) states due to the Laguerre-Gaussian (LG) light beams. In 2011, Yao and Padgett [4] presented a historical background of the angular momentum to explain various aspects of the OAM states, e.g. the generation of helical beams, the origin and behaviour of OAM, its transformation and possible applications, mode conversion and beam coherence, etc. Recently, several investigations [5][6][7][8][9][10][11][12] have been made with reference to the plasma physics to study the importance of the plasma modes and instabilities with finite OAM, e.g. nonlinear wave couplin...