2006
DOI: 10.1063/1.2357046
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Nonlinear response of a relativistic plasma to intense fields: Generation of strong quasistatic magnetic fields

Abstract: Instabilities and generation of a quasistationary magnetic field by the interaction of relativistically intense electromagnetic wave with a plasma

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Cited by 7 publications
(14 citation statements)
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“…In the same figure, one can also observe packets of electrons heated symmetrically in both positive and negative p y directions. To interpret this result, one can notice that the phase space, although more diffuse in our case, is very similar to what has been already observed 30,31 at higher laser intensities and denser plasmas due to the self-generation of large quasistatic magnetic fields [32][33][34] at the plasma surface. In our case, the magnetic field component at the surface is dominated by the resonant oscillating magnetic field of the surface wave.…”
Section: Electron Acceleration By Surface Plasma Wavessupporting
confidence: 85%
“…In the same figure, one can also observe packets of electrons heated symmetrically in both positive and negative p y directions. To interpret this result, one can notice that the phase space, although more diffuse in our case, is very similar to what has been already observed 30,31 at higher laser intensities and denser plasmas due to the self-generation of large quasistatic magnetic fields [32][33][34] at the plasma surface. In our case, the magnetic field component at the surface is dominated by the resonant oscillating magnetic field of the surface wave.…”
Section: Electron Acceleration By Surface Plasma Wavessupporting
confidence: 85%
“…In the same figure, one can also observe packets of electrons heated symmetrically in both positive and negative p y directions. To interpret this result, one can notice that the phase space, although more diffuse in our case, is very similar to what has been already observed 30,31 at higher laser intensities and denser plasmas due to the self-generation of large quasistatic magnetic fields [32][33][34] at the plasma surface. In our case, the magnetic field component at the surface is dominated by the resonant oscillating magnetic field of the surface wave.…”
Section: -5supporting
confidence: 59%
“…In this case all three-waves processes are absent. This means in pair plasma the coupling of transverse plasmons will not excite low-frequency magnetization currents, this result is consistent with that in [25,26] if they are extended to pair plasmas. (5) In this paper we focus on investigating the behavior of transverse plasmons in pair plasmas without ambient magnetic field by a kinetic method.…”
Section: Discussionsupporting
confidence: 93%