Neutrino Pair Synchrotron Emission from Pulsar Polar Caps

Details Neutrino Pair Synchrotron Emission from Pulsar Polar Caps Neutrino Pair Synchrotron Emission from Pulsar Polar Caps

Jun 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002sf2a.conf..553d&link_type=abstract

SF2A-2002: Semaine de l'Astrophysique Francaise, meeting held in Paris, France, June 24-29, 2002, Eds.: F. Combes and D. Barret,

Astronomy and Astrophysics

Astrophysics

Scientific paper

Magnetars are neutron stars presenting very interesting characteristics for the production of neutrinos pairs at very high energies by a mechanism of magneto-Bremsstrahlung. We have developped a model, to calculate the power spectrum of neutrinos flux in the case of a non-thermal distribution of electrons in presence of a field of 10**14 Gauss. We are thus able to predict the number of neutrino-events detectable by the experiment ANTARES for this target, a few per year.

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