Total Pair Production Rate for Electron Neutrinos in Magnetic Fields

Details Total Pair Production Rate for Electron Neutrinos in Magnetic Fields Total Pair Production Rate for Electron Neutrinos in Magnetic Fields

Mar 2012

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2012aps..aprb15006r&link_type=abstract

American Physical Society, APS April Meeting 2012, March 31-Apr 3, 2012, abstract #B15.006

Astronomy and Astrophysics

Astrophysics

Scientific paper

We present a calculation for the total production rate for electron-positron pairs using electron-type neutrinos in an intense magnetic field. This production rate is significant to a number of astrophysical phenomena exhibiting strong magnetic fields and a sensitivity to neutrino transport, including magnetars and some varieties of supernovae. Because electron-type neutrino flux is considerably higher in supernovae events and it participates in both charged and neutral-current reactions, its contribution to the total production rate is of particular interest. We compare this to a previous calculation involving muon and tau-type neutrinos.

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