2,801 research outputs found
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
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
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
KAM-tori near an analytic elliptic fixed point
We study the accumulation of an elliptic fixed point of a real analytic
Hamiltonian by quasi-periodic invariant tori. We show that a fixed point with
Diophantine frequency vector \o_0 is always accumulated by invariant complex
analytic KAM-tori. Indeed, the following alternative holds: If the Birkhoff
normal form of the Hamiltonian at the invariant point satisfies a R\"ussmann
transversality condition, the fixed point is accumulated by real analytic
KAM-tori which cover positive Lebesgue measure in the phase space (in this part
it suffices to assume that \o_0 has rationally independent coordinates). If
the Birkhoff normal form is degenerate, there exists an analytic subvariety of
complex dimension at least passing through 0 that is foliated by complex
analytic KAM-tori with frequency . This is an extension of previous
results obtained in \cite{EFK} to the case of an elliptic fixed point
Slow test charge response in a dusty plasma with Kappa distributed electrons and ions
The electrostatic potential around a slowly moving test charge is studied in a dusty plasma where the ions and electrons follow a powerlaw Kappa distribution in velocity space. A test charge moving with a speed much smaller than the dust thermal speed gives rise to a short-scale Debye-Hueckel potential as well as a long-range far-field potential decreasing as inverse cube of the distance to the test charge along the propagation direction. The potentials are significantly modified in the presence of high-energy tails, modeled by lower spectral indices in the ion and electron Kappa distribution functions. Plasma parameters relevant to laboratory dusty plasmas are discussed
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