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  • PACS. 52.50.Jm Plasma production and heating by laser beams - 52.40.Nk Laser-plasma interactions (e.g., anomalous absorption, backscattering, magnetic field generation, fast particle generation) - 52.25.Rv Emission, absorption, and scattering of visible and infrared radiation  (1)
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  • PACS. 52.50.Jm Plasma production and heating by laser beams - 52.40.Nk Laser-plasma interactions (e.g., anomalous absorption, backscattering, magnetic field generation, fast particle generation) - 52.25.Rv Emission, absorption, and scattering of visible and infrared radiation  (1)
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    Electronic Resource
    Electronic Resource
    Springer
    The European physical journal 8 (2000), S. 153-156 
    ISSN: 1434-6079
    Keywords: PACS. 52.50.Jm Plasma production and heating by laser beams - 52.40.Nk Laser-plasma interactions (e.g., anomalous absorption, backscattering, magnetic field generation, fast particle generation) - 52.25.Rv Emission, absorption, and scattering of visible and infrared radiation
    Source: Springer Online Journal Archives 1860-2000
    Topics: Physics
    Notes: Abstract: It is well established that, at sub-relativistic intensities, the absorption of laser light by underdense plasmas decreases with increasing pulse intensity as interaction enters a non-linear regime. On the other hand, as the relativistic interaction regime is reached, further absorption mechanisms can be activated which can account for a substantial energy transfer. Using the particle code WAKE, we performed numerical simulations of the relativistic interaction of intense laser pulses with underdense plasmas in conditions that can be experimentally tested. Our simulations show that, while the relativistic laser intensity generates a population of fast electrons, a considerable fraction of the pulse energy goes into a population of thermal electrons. These findings open new possibilities for a direct observation of relativistic interaction processes using high resolution soft X-ray techniques.
    Type of Medium: Electronic Resource
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