Some Astrophysical Implications of the Helical Cerenkov Effect

Details Some Astrophysical Implications of the Helical Cerenkov Effect Some Astrophysical Implications of the Helical Cerenkov Effect

Nov 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998aps..dpp.q7f12s&link_type=abstract

American Physical Society, Division of Plasma Physics Meeting, November 16-20, 1998 New Orleans, LA, abstract #Q7F.12

Physics

Plasma Physics

Scientific paper

The neutron stars (pulsar) and supernovas can have magnetic fields whose values can easily be in the range of 10^5-10^9 T. The medium in which these magnetic fields reside is likely to be an ionized medium; that is, a plasma, which, as usual, may be assumed to be dominated by electrons. Here we wish to argue that in such a strong magnetic field dominated medium, at least on a classical level, a new radiation process associated with the helical Cerenkov radiation could be rather important.

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