Showing 1–20 of 163 results
/ Date/ Name
Nov 16, 2023Physics Opportunities at a Beam Dump Facility at PIP-II at Fermilab and BeyondMay 28, 2021First Dark Matter Search Results From Coherent CAPTAIN-MillsMay 26, 2023Constraining models for the origin of ultra-high-energy cosmic rays with a novel combined analysis of arrival directions, spectrum, and composition data measured at the Pierre Auger ObservatorySep 9, 2022Ionization efficiency for nuclear recoils in silicon from $\sim 50$ eV to $3$ MeVJul 20, 2023Search for UHE Photons from Gravitational Wave Sources with the Pierre Auger ObservatoryMar 5, 2009Upper limit on the cosmic-ray photon fraction at EeV energies from the Pierre Auger ObservatoryApr 18, 2012Light Sterile Neutrinos: A White PaperJun 15, 2011Anisotropy and chemical composition of ultra-high energy cosmic rays using arrival directions measured by the Pierre Auger ObservatoryJul 30, 2020Results on Low-Mass Weakly Interacting Massive Particles from an 11 kg-day Target Exposure of DAMIC at SNOLABFeb 14, 2020Cosmic-ray anisotropies in right ascension measured by the Pierre Auger ObservatoryJan 23, 2019Data-driven estimation of the invisible energy of cosmic ray showers with the Pierre Auger ObservatoryAug 10, 2018Large-scale cosmic-ray anisotropies above 4 EeV measured by the Pierre Auger ObservatoryOct 21, 2020A search for ultra high energy neutrinos from TXS 0506+056 using the Pierre Auger ObservatoryOct 19, 2017Inferences on Mass Composition and Tests of Hadronic Interactions from 0.3 to 100 EeV using the water-Cherenkov Detectors of the Pierre Auger ObservatoryJul 11, 2014Reconstruction of inclined air showers detected with the Pierre Auger ObservatoryNov 25, 2005Thermal effects on the absorption of ultra-high energy neutrinos by the cosmic neutrino backgroundJul 13, 2005UHE neutrino damping in a thermal gas of relic neutrinosMar 12, 2005Neutrinospheres, resonant neutrino oscillations, and pulsar kicksSep 10, 2014Searches for Large-Scale Anisotropy in the Arrival Directions of Cosmic Rays Detected above Energy of $10^{19}$ eV at the Pierre Auger Observatory and the Telescope ArrayOct 19, 1999VEP oscillation solutions to the solar neutrino problem