Abstract Rayleigh–Taylor (RT) and Richtmyer–Meshkov (RM) instabilities are well-known
pathways towards turbulent mixing layers, in many cases characterized by significant mass …

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 …

Warm dense matter (WDM)—an exotic state of highly compressed matter—has attracted
increased interest in recent years in astrophysics and for dense laboratory systems. At the …

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

Unlike conventional optics, plasmonics enables unrivaled concentration of optical energy
well beyond the diffraction limit of light. However, a significant part of this energy is …

A quantum hydrodynamic (fluid) model, derived from the Wigner-Poisson equations, is used
to investigate the ultrafast electron dynamics in thin metal films. The hydrodynamic …

Quantum hydrodynamics (QHD) theory for finite temperature plasmas is consistently derived
in the framework of the local density approximation of the free energy with first order density …

Quantum plasmas are an important topic in astrophysics and high pressure laboratory
physics for more than 50 years. In addition, many condensed matter systems, including the …

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 …

Multiscale plasmonic systems (eg, extended metallic nanostructures with subnanometer
inter-distances) play a key role in the development of next-generation nanophotonic …