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Search for steady point-like sources in the astrophysical muon neutrino flux with 8 years of IceCube data
IceCube Collaboration, M. G. Aartsen, M. Ackermann +325
The IceCube Collaboration has observed a high-energy astrophysical neutrino flux and recently found evidence for neutrino emission from the blazar TXS 0506+056. These results open…
Unified atmospheric neutrino passing fractions for large-scale neutrino telescopes
Carlos A. Argüelles, Sergio Palomares-Ruiz, Austin Schneider +2
The atmospheric neutrino passing fraction, or self-veto, is defined as the probability for an atmospheric neutrino not to be accompanied by a detectable muon from the same cosmic-r…
On the Charm Contribution to the Atmospheric Neutrino Flux
Francis Halzen, Logan Wille
We revisit the estimate of the charm particle contribution to the atmospheric neutrino flux that is expected to dominate at high energies because long-lived high-energy pions and k…
Upper Limit on Forward Charm Contribution to Atmospheric Neutrino Flux
Francis Halzen, Logan Wille
We revisit the calculation of charm particle production in hadron collisions, focusing on the production of charm particles that carry a large fraction of the momentum of the incid…
Improved limits on dark matter annihilation in the Sun with the 79-string IceCube detector and implications for supersymmetry
IceCube Collaboration, M. G. Aartsen, K. Abraham +315
We present an improved event-level likelihood formalism for including neutrino telescope data in global fits to new physics. We derive limits on spin-dependent dark matter-proton s…
The High-Energy Behavior of Photon, Neutrino and Proton Cross Sections
Carlos A. Arguelles, Francis Halzen, Logan Wille +2
By combining the color dipole model of the nucleon with the assumption that cross sections behave asymptotically as , we are able to describe the data for photon, neutrin…