The influence of speed-changing self-similar collisions on the spectral line shape is considered in terms of the classical Fourier integral theory. The self-similar mechanism of interference of scalar perturbations for phase shifts of an atomic oscillator is developed. The motion of a radiating dipole in a perturb gas is examined in the framework of the self-similar diffusion model. A general formula for the correlation function, which allows for a combined effect of speed-dependent Doppler and pressure broadening, is derived. In the Doppler regime this formula yields the self-similar Galatry profile and in the case when speed-changing collisions are neglected it leads to the self-similar Voigt profile. In the limiting case when the self-si...
The study deals with two conceptual problems in the theory of Stark broadening by plasmas. One probl...
It is shown that the inclusive spectra of the produced hadrons in hadron-hadron and nuclear-nuclear ...
$^{1}$ A. S. Pine and J. P. Looney, this session. $^{2}$ R. M. Herman and E. W. Weber, J. Phys. B: A...
The influence of speed-changing self-similar collisions on the spectral line shape is considered in ...
A self-similar collision model for the motion of radiating particles in a perturbed gas is suggested...
The space-time evolution of an initial step-like plasma density variation is studied. We give partic...
The transport properties of a turbulent plasma are investigated in the vicinity of a self-similar tu...
The role of velocity changing collisions (VCCs) in pressure-dependent line shapes is revisited, high...
Simple analytical models are presented for hydrodynamic expansion of laser-produced plasma governed ...
The models of Vekshtein, Ryutov & Sagdeev (VRS), describing a marginally stable turbulent plasma sus...
A model of plasma oscillations in the presence of small angle collisions is presented which admits o...
In the paper one of possible reasons for explanation of strange transport in the turbulent plasma in...
We study the dynamics of classical particles in different classes of spatially extended self-similar...
We analyze the influence of the speed dependence of collisional broadening and shifting on the shape...
International audienceThe self-similar dynamics of the collision between radiative and adiabatic sup...
The study deals with two conceptual problems in the theory of Stark broadening by plasmas. One probl...
It is shown that the inclusive spectra of the produced hadrons in hadron-hadron and nuclear-nuclear ...
$^{1}$ A. S. Pine and J. P. Looney, this session. $^{2}$ R. M. Herman and E. W. Weber, J. Phys. B: A...
The influence of speed-changing self-similar collisions on the spectral line shape is considered in ...
A self-similar collision model for the motion of radiating particles in a perturbed gas is suggested...
The space-time evolution of an initial step-like plasma density variation is studied. We give partic...
The transport properties of a turbulent plasma are investigated in the vicinity of a self-similar tu...
The role of velocity changing collisions (VCCs) in pressure-dependent line shapes is revisited, high...
Simple analytical models are presented for hydrodynamic expansion of laser-produced plasma governed ...
The models of Vekshtein, Ryutov & Sagdeev (VRS), describing a marginally stable turbulent plasma sus...
A model of plasma oscillations in the presence of small angle collisions is presented which admits o...
In the paper one of possible reasons for explanation of strange transport in the turbulent plasma in...
We study the dynamics of classical particles in different classes of spatially extended self-similar...
We analyze the influence of the speed dependence of collisional broadening and shifting on the shape...
International audienceThe self-similar dynamics of the collision between radiative and adiabatic sup...
The study deals with two conceptual problems in the theory of Stark broadening by plasmas. One probl...
It is shown that the inclusive spectra of the produced hadrons in hadron-hadron and nuclear-nuclear ...
$^{1}$ A. S. Pine and J. P. Looney, this session. $^{2}$ R. M. Herman and E. W. Weber, J. Phys. B: A...