Energy losses of a neutron star due to inverse muon decay in the superstrong magnetic field

Details Energy losses of a neutron star due to inverse muon decay in the superstrong magnetic field Energy losses of a neutron star due to inverse muon decay in the superstrong magnetic field

Jul 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995ruphj..38..687l&link_type=abstract

Russian Physics Journal, Volume 38, Issue 7, pp.687-691

Physics

Scientific paper

The emission of a pair of neutrinos by a charged lepton under the influence of a strong magnetic field is examined. The expression found in general form for the probability of the process l → l'vV in the strong magnetic field of a neutron star is used to evaluate the contribution of inverse muon decay e → μvV to the energy losses of the neutron star. The conditions under which this contribution to the energy losses of a neutron star may compete with that due to neutrino pair emission in the process e → evV are discussed.

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