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Parameter Estimation in Searches for the Stochastic Gravitational-Wave Background
Vuk Mandic, Eric Thrane, Stefanos Giampanis +1
The stochastic gravitational-wave background (SGWB) is expected to arise from the superposition of many independent and unresolved gravitational-wave signals of either cosmological…
Gravitational Waves from Fallback Accretion onto Neutron Stars
Anthony L. Piro, Eric Thrane
Massive stars generally end their lives as neutron stars (NSs) or black holes (BHs), with NS formation typically occurring at the low mass end and collapse to a BH more likely at t…
Evidence for the Appearance of Atmospheric Tau Neutrinos in Super-Kamiokande
Kamiokande Collaboration
Super-Kamiokande atmospheric neutrino data were fit with an unbinned maximum likelihood method to search for the appearance of tau leptons resulting from the interactions of oscill…
Treatment of Calibration Uncertainty in Multi-Baseline Cross-Correlation Searches for Gravitational Waves
John T. Whelan, Emma L. Robinson, Joseph D. Romano +1
Uncertainty in the calibration of gravitational-wave (GW) detector data leads to systematic errors which must be accounted for in setting limits on the strength of GW signals. When…
Search for GUT Monopoles at Super-Kamiokande
Kamiokande Collaboration, K. Ueno, K. Abe +109
GUT monopoles captured by the Sun's gravitation are expected to catalyze proton decays via the Callan-Rubakov process. In this scenario, protons, which initially decay into pions,…
Search for Nucleon Decay into Charged Anti-lepton plus Meson in Super-Kamiokande I and II
Kamiokande Collaboration, H. Nishino, K. Abe +105
Searches for a nucleon decay into a charged anti-lepton (e^+ or μ^+) plus a light meson (π^0, π^-, η, ρ^0, ρ^-, ω) were performed using the Super-Kamiokande I and II data. Twelve n…