▪ Abstract High-energy (> 100 MeV) neutrino astrophysics enters an era of opportunity and
discovery as the sensitivity of detectors approaches astrophysically relevant flux levels. We …

The central challenge in building a quantum computer is error correction. Unlike classical
bits, which are susceptible to only one type of error, quantum bits (qubits) are susceptible to …

We report on a search for particle dark matter with the XENON100 experiment, operated at
the Laboratori Nazionali del Gran Sasso for 13 months during 2011 and 2012. XENON100 …

We report new calculations of the cross sections for deeply inelastic neutrino-nucleon
scattering at neutrino energies between 10 9 eV and 10 21 eV. We compare with results in …

Muon attenuation in matter can be used to infer the average material density along the path
length of muons underground. By mapping the intensity of cosmic ray muons with an …

The XENON1T experiment at the Laboratori Nazionali del Gran Sasso (LNGS) is the first
WIMP dark matter detector operating with a liquid xenon target mass above the ton-scale …

We provide a comprehensive study of the cosmic-ray muon flux and induced activity as a
function of overburden along with a convenient parametrization of the salient fluxes and …

In the past decades, numerous experiments have emerged to unveil the nature of dark
matter, one of the most discussed open questions in modern particle physics. Among them …

A new model called “PHITS-based Analytical Radiation Model in the Atmosphere (PARMA)
version 4.0” was developed to facilitate instantaneous estimation of not only omnidirectional …

We measured two-neutrino double beta decay of Te 130 using an exposure of 300.7 kg yr
accumulated with the CUORE detector. Using a Bayesian analysis to fit simulated spectra to …