LEGEND-1000 preconceptual design report

N Abgrall, I Abt, M Agostini, A Alexander… - arXiv preprint arXiv …, 2021 - arxiv.org
We propose the construction of LEGEND-1000, the ton-scale Large Enriched Germanium
Experiment for Neutrinoless $\beta\beta $ Decay. This international experiment is designed …

[HTML][HTML] Performance of ANAIS-112 experiment after the first year of data taking

J Amaré, S Cebrián, I Coarasa, C Cuesta… - The European Physical …, 2019 - Springer
ANAIS is a direct detection dark matter experiment aiming at the study of the annual
modulation expected in the interaction rate. It uses same target and technique as the …

Modulations of the cosmic muon signal in ten years of Borexino data

M Agostini, K Altenmueller, S Appel… - … of Cosmology and …, 2019 - iopscience.iop.org
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 …

Atmospheric muons and their variations with temperature

S Verpoest, D Soldin, P Desiati - Astroparticle Physics, 2024 - Elsevier
Seasonal variations of atmospheric muons are traditionally interpreted in terms of an
effective temperature that relates the atmospheric temperature profile at a given time to the …

Characterization of the varying flux of atmospheric muons measured with the Large Volume Detector for 24 years

NY Agafonova, M Aglietta, P Antonioli, VV Ashikhmin… - Physical Review D, 2019 - APS
The Large Volume Detector, hosted in the INFN Laboratori Nazionali del Gran Sasso, is
triggered by atmospheric muons at a rate of∼ 0.1 Hz. The data collected over almost a …

Seasonal variation of the underground cosmic muon flux observed at Daya Bay

FP An, AB Balantekin, HR Band, M Bishai… - … of Cosmology and …, 2018 - iopscience.iop.org
Abstract The Daya Bay Experiment consists of eight identically designed detectors located in
three underground experimental halls named as EH1, EH2, EH3, with 250, 265 and 860 …

Snowmass2021 Cosmic Frontier White Paper: Calibrations and backgrounds for dark matter direct detection

D Baxter, R Bunker, S Shaw, S Westerdale… - arXiv preprint arXiv …, 2022 - arxiv.org
Future dark matter direct detection experiments will reach unprecedented levels of
sensitivity. Achieving this sensitivity will require more precise models of signal and …

[HTML][HTML] Production of muons from heavy-flavour hadron decays in pp collisions at = 5.02 TeV

S Acharya, D Adamová, SP Adhya, A Adler… - Journal of high energy …, 2019 - Springer
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) …

Measurement of the cosmic ray muon flux seasonal variation with the OPERA detector

N Agafonova, A Alexandrov, A Anokhina… - … of Cosmology and …, 2019 - iopscience.iop.org
The OPERA experiment discovered muon neutrino into tau neutrino oscillations in
appearance mode, detecting tau leptons by means of nuclear emulsion films. The apparatus …

[PDF][PDF] Direct dark matter searches using sodium iodide targets: Status and prospects

ML Sarsa - Journal of Advanced Instrumentation in …, 2024 - jais.andromedapublisher.org
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 …