The current understanding of some important nonlinear collective processes in quantum
plasmas with degenerate electrons is presented. After reviewing the basic properties of …

Dense quantum plasmas are ubiquitous in planetary interiors and in compact astrophysical
objects (eg, the interior of white dwarf stars, in magnetars, etc.), in semiconductors and …

Starting from the non-relativistic Pauli description of spin-particles, a set of fluid equations,
governing the dynamics of such particles interacting with external fields and other particles …

The linear and nonlinear properties of the ion-acoustic waves (IAWs) are investigated by
using the quantum hydrodynamic equations together with the Poisson equation in a three …

For quantum effects to be significant in plasmas it is often assumed that the temperature over
density ratio must be small. In this paper we challenge this assumption by considering the …

Electrons in plasmas produced by next-generation ultraintense lasers (I> 5× 10 22 W/cm 2)
can be spin polarized to a high degree (10%–70%) by the laser pulses on a femtosecond …

We consider nonlinear interactions between intense circularly polarized electromagnetic
(CPEM) waves and electron plasma oscillations (EPOs) in a dense quantum plasma, taking …

The quantum hydrodynamic (QHD) model of charged spin-1/2 particles contains physical
quantities defined for all particles of a species including particles with spin-up and with spin …

We develop a quantum representation for Newtonian viscous fluid flows by establishing a
map** between the Navier-Stokes equation (NSE) and the Schrödinger-Pauli equation …

Among the incredibly diverse variety of astrophysical objects, there are some that are
characterized by very extreme physical conditions not encountered anywhere else in the …