13,182 research outputs found
Dust acoustic wave in a strongly magnetized pair-dust plasma
The existence of the dust acoustic wave (DAW) in a strongly magnetized
electron-positron (pair)-dust plasma is demonstrated. In the DAW, the restoring
force comes from the pressure of inertialess electrons and positrons, and the
dust mass provides the inertia. The waves could be of interest in astrophysical
settings such as the supernovae and pulsars, as well as in cluster explosions
by intense laser beams in laboratory plasmas.Comment: 6 pages, revtex
The Intense Radiation Gas
We present a new dispersion relation for photons that are nonlinearly
interacting with a radiation gas of arbitrary intensity due to photon-photon
scattering. It is found that the photon phase velocity decreases with
increasing radiation intensity, it and attains a minimum value in the limit of
super-intense fields. By using Hamilton's ray equations, a self-consistent
kinetic theory for interacting photons is formulated. The interaction between
an electromagnetic pulse and the radiation gas is shown to produce pulse
self-compression and nonlinear saturation. Implications of our new results are
discussed.Comment: 7 pages, 1 figure, version to appear in Europhys. Let
Self-compression and catastrophic collapse of photon bullets in vacuum
Photon-photon scattering, due to photons interacting with virtual
electron-positron pairs, is an intriguing deviation from classical
electromagnetism predicted by quantum electrodynamics (QED). Apart from being
of fundamental interest in itself, collisions between photons are believed to
be of importance in the vicinity of magnetars, in the present generation
intense lasers, and in intense laser-plasma/matter interactions; the latter
recreating astrophysical conditions in the laboratory. We show that an intense
photon pulse propagating through a radiation gas can self-focus, and under
certain circumstances collapse. This is due to the response of the radiation
background, creating a potential well in which the pulse gets trapped, giving
rise to photonic solitary structures. When the radiation gas intensity has
reached its peak values, the gas releases part of its energy into `photon
wedges', similar to Cherenkov radiation. The results should be of importance
for the present generation of intense lasers and for the understanding of
localized gamma ray bursts in astrophysical environments. They could
furthermore test the predictions of QED, and give means to create ultra-intense
photonic pulses.Comment: 4 pages, 1 figur
Nonlinear propagation of broadband intense electromagnetic waves in an electron-positron plasma
A kinetic equation describing the nonlinear evolution of intense
electromagnetic pulses in electron-positron (e-p) plasmas is presented. The
modulational instability is analyzed for a relativistically intense partially
coherent pulse, and it is found that the modulational instability is inhibited
by the spectral pulse broadening. A numerical study for the one-dimensional
kinetic photon equation is presented. Computer simulations reveal a
Fermi-Pasta-Ulam-like recurrence phenomena for localized broadband pulses. The
results should be of importance in understanding the nonlinear propagation of
broadband intense electromagnetic pulses in e-p plasmas in laser-plasma systems
as well as in astrophysical plasma settings.Comment: 16 pages, 5 figures, to appear in Phys. Plasma
Nonlinear dynamics of large amplitude dust acoustic shocks and solitary pulses in dusty plasmas
We present a fully nonlinear theory for dust acoustic (DA) shocks and DA
solitary pulses in a strongly coupled dusty plasma, which have been recently
observed experimentally by Heinrich et al. [Phys. Rev. Lett. 103, 115002
(2009)], Teng et al. [Phys. Rev. Lett. 103, 245005 (2009)], and Bandyopadhyay
et al. [Phys. Rev. Lett. 101, 065006 (2008)]. For this purpose, we use a
generalized hydrodynamic model for the strongly coupled dust grains, accounting
for arbitrary large amplitude dust number density compressions and potential
distributions associated with fully nonlinear nonstationary DA waves.
Time-dependent numerical solutions of our nonlinear model compare favorably
well with the recent experimental works (mentioned above) that have reported
the formation of large amplitude non-stationary DA shocks and DA solitary
pulses in low-temperature dusty plasma discharges.Comment: 9 pages, 4 figures. To be published in Physical Review
Self-Diffusion in 2D Dusty Plasma Liquids: Numerical Simulation Results
We perform Brownian dynamics simulations for studying the self-diffusion in
two-dimensional (2D) dusty plasma liquids, in terms of both mean-square
displacement and velocity autocorrelation function (VAF). Super-diffusion of
charged dust particles has been observed to be most significant at infinitely
small damping rate for intermediate coupling strength, where the
long-time asymptotic behavior of VAF is found to be the product of and
. The former represents the prediction of early theories in
2D simple liquids and the latter the VAF of a free Brownian particle. This
leads to a smooth transition from super-diffusion to normal diffusion, and then
to sub-diffusion with an increase of the damping rate. These results well
explain the seemingly contradictory scattered in recent classical molecular
dynamics simulations and experiments of dusty plasmas.Comment: 10 pages 5 figures, accepted by PR
Simulation study of the filamentation of counter-streaming beams of the electrons and positrons in plasmas
The filamentation instability driven by two spatially uniform and
counter-streaming beams of charged particles in plasmas is modelled by a
particle-in-cell (PIC) simulation. Each beam consists of the electrons and
positrons. The four species are equally dense and they have the same
temperature. The one-dimensional simulation direction is orthogonal to the beam
velocity vector. The magnetic field grows spontaneously and rearranges the
particles in space, such that the distributions of the electrons of one beam
and the positrons of the second beam match. The simulation demonstrates that as
a result no electrostatic field is generated by the magnetic field through its
magnetic pressure gradient prior to its saturation. This electrostatic field
would be repulsive at the centres of the filaments and limit the maximum charge
and current density. The filaments of electrons and positrons in this
simulation reach higher charge and current densities than in one with no
positrons. The oscillations of the magnetic field strength induced by the
magnetically trapped particles result in an oscillatory magnetic pressure
gradient force. The latter interplays with the statistical fluctuations in the
particle density and it probably enforces a charge separation, by which
electrostatic waves grow after the filamentation instability has saturated.Comment: 13 pages, 8 figure
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