On a possible mechanism of familon emission from a neutron star

Details On a possible mechanism of familon emission from a neutron star On a possible mechanism of familon emission from a neutron star

Nov 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989phlb..231..280a&link_type=abstract

Physics Letters B, Volume 231, Issue 3, p. 280-282.

Physics

7

Scientific paper

The energy loss rate due to familon emission from electrons accelerated
by a strong magnetic field in the crust of a neutron star is calculated.
It is shown that under certain conditions the familon luminosity can
become comparable with that of a neutrino bremsstrahlung.

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