The nondetection of GeV-scale weakly interacting massive particles (WIMPs) has led to
increased interest in more general candidates, including sub-GeV dark matter. Direct …

We have measured the flux of cosmic muons in the Laboratori Nazionali del Gran Sasso at
3800 m we to be (3.432±0.003)⋅ 10− 4 m− 2 s− 1 based on ten years of Borexino data …

Tidal measurements are of great significance since they may provide us with essential data
to apply towards protection of coastal communities and sea traffic. Currently, tide gauge …

Future dark matter direct detection experiments will reach unprecedented levels of
sensitivity. Achieving this sensitivity will require more precise models of signal and …

A bstract Production cross sections of muons from semi-leptonic decays of charm and
beauty hadrons were measured at forward rapidity (2. 5< y< 4) in proton-proton (pp) …

The OPERA experiment discovered muon neutrino into tau neutrino oscillations in
appearance mode, detecting tau leptons by means of nuclear emulsion films. The apparatus …

Abstract Thallium-Activated Sodium Iodide (NaI (Tl)) scintillators have been widely used for
radiation detection since the middle of the XXth century, being applied, for instance, in …

Visualization of the subsurface flow of geofluids with meter‐scale resolution is one of the
essential components of current and future geophysical observation technologies. The …

Using two years of data from the NOvA Near Detector at Fermilab, we report a seasonal
variation of cosmic ray induced multiple-muon (N μ≥ 2) event rates which has an opposite …

We report the rate of cosmic ray air showers with multiplicities exceeding 15 muon tracks
recorded in the NOvA Far Detector between May 2016 and May 2018. The detector is …