High energy neutrinos from charm in astrophysical sources
  Charm production gives rise to a flux of very high energy neutrinos from astrophysical sources with jets driven by central engines, such as gamma ray bursts or supernovae with jets. The neutrino flux from semi-leptonic decays of charmed mesons is subject to much less hadronic and radiative cooling than the conventional flux from pion and kaon decays and therefore has a dominant contribution at higher energies, of relevance to future ultrahigh energy neutrino experiments. 
Rikard Enberg (Arizona), Mary Hall Reno (Iowa), Ina Sarcevic (Arizona)