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Title: On the theory of magnetic field generation by relativistically strong laser radiation

Technical Report ·
DOI:https://doi.org/10.2172/373897· OSTI ID:373897
;  [1];  [2]
  1. International Centre for Theoretical Physics, Trieste (Italy)
  2. Texas Univ., Austin, TX (United States). Inst. for Fusion Studies

The authors consider the interaction of subpicosecond relativistically strong short laser pulses with an underdense cold unmagnetized electron plasma. It is shown that the strong plasma inhomogeneity caused by laser pulses results in the generation of a low frequency (quasistatic) magnetic field. Since the electron density distribution is determined completely by the pump wave intensity, the generated magnetic field is negligibly small for nonrelativistic laser pulses but increases rapidly in the ultrarelativistic case. Due to the possibility of electron cavitation (complete expulsion of electrons from the central region) for narrow and intense beams, the increase in the generated magnetic field slows down as the beam intensity is increased. The structure of the magnetic field closely resembles that of the field produced by a solenoid; the field is maximum and uniform in the cavitation region, then it falls, changes polarity and vanishes. In extremely dense plasmas, highly intense laser pulses in the self-channeling regime can generate magnetic fields {approximately} 100 Mg and greater.

Research Organization:
Univ. of Texas, Austin, TX (United States). Institute for Fusion Studies
Sponsoring Organization:
USDOE Office of Energy Research, Washington, DC (United States)
DOE Contract Number:
FG03-96ER54346
OSTI ID:
373897
Report Number(s):
DOE/ER/54346-752; IFSR-752; ON: DE96014770; TRN: 96:025585
Resource Relation:
Other Information: PBD: Jul 1996
Country of Publication:
United States
Language:
English

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