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Perturbative Charm Production and the Prompt Atmospheric Neutrino Flux in light of RHIC and LHC
Atri Bhattacharya, Rikard Enberg, Mary Hall Reno +2
Prompt neutrinos due to the decay of charmed mesons produced in the atmosphere from cosmic-ray and atmospheric nuclei interactions may be a significant source of background to ultr…
Probing secret interactions of eV-scale sterile neutrinos with the diffuse supernova neutrino background
Mary Hall Reno, Yu Seon Jeong, Sergio Palomares-Ruiz +1
While three flavors of "active" neutrinos are consistent with mixing angle results within error bars, there are anomalies may be hints of physics beyond the standard model that can…
Charm contribution to ultrahigh-energy neutrinos from newborn magnetars
Jose Alonso Carpio, Kohta Murase, Mary Hall Reno +2
Newborn, strongly magnetized neutron stars (so-called magnetars) surrounded by their stellar or merger ejecta are expected to be sources of ultrahigh-energy neutrinos via decay of…