Abstract:
This thesis investigates nonlinear acoustic wave phenomena in both strongly and weakly
coupled collisionless unmagnetized plasmas using analytical and numerical methods. By
developing mathematical models for different plasma environments, the study employs the
reductive perturbation technique (RPT) to derive nonlinear evolution equations (NLEEs).
These equations are then used to analyze the propagation of shock waves, solitons, and
periodic waves in various plasma configurations.
In Chapter 2, Burgers equations involving quadratic, cubic, and combined
quadratic-cubic nonlinearities are derived for a coupled complex plasma system consisting
of Boltzmann-distributed electrons, nonthermal ions, and charged dust particles. The
generalized Riccati equation mapping method (GREMM) is employed to obtain both shock
and oscillatory wave solutions from these equations, while parametric effects on wave
characteristics are systematically examined.
Chapter 3 investigates heavy ion-acoustic shock waves (HIASWs) in a plasma
comprising inertial heavy ions, Maxwellian light ions, and (α,q)-distributed electrons, by
deriving the Burgers, modified Burgers, and mixed modified Burgers equations. The study
presents stationary shock wave solutions for these equations and examines how plasma
parameters influence shock wave characteristics.
Chapter 4 investigates the dust acoustic (DA) shock wave phenomena in an strongly
coupled dusty plasma. By deriving Burgers equations with quadratic, cubic, and quartic
nonlinearities, we analyze shock wave behavior near critical values (CVs) and super-critical
values (SCVs), revealing how polarization force and coupling parameter modifies shock
wave excitations.
Chapter 5 analyzes heavy ion-acoustic (HIA) solitons and dressed solitons in
weakly/strongly coupled plasmas with nonthermal electrons.
Chapter 6 advances the Chapter 3 framework by examining HIASWs near CVs and
SCVs, deriving a non-integrable NLEE with combined cubic-quartic nonlinearities that
necessitates numerical solution via Runge-Kutta-Fehlberg analysis.
Thus, the thesis enhances understanding of nonlinear coherent structures observed in
various space and astrophysical environments.