activity
19962025
most citedSemi-empirical calculation of quenching factors for ions in scintillators

221 citations · 4.3k across the 121 of their papers we have counts for

collaborators

118 papers

nucl-ex2025★ 8 cited

Comprehensive Review of 2 Decay Half-Lives

B. Pritychenko, V. I. Tretyak

The double-beta (2)-decay is the rarest nuclear physics process, and its experimental half-lives (T) exceed the age of the Universe from nine to fourteen orders of magni…

hep-ex2023★ 14 cited

The background model of the CUPID-Mo experiment

Mo Collaboration, C. Augier, A. S. Barabash +79

CUPID-Mo, located in the Laboratoire Souterrain de Modane (France), was a demonstrator for the next generation decay experiment, CUPID. It consisted of an array of 20 enrich…

physics.ins-det2023★ 12 cited

A first test of CUPID prototypal light detectors with NTD-Ge sensors in a pulse-tube cryostat

CUPID collaboration, K. Alfonso, A. Armatol +176

CUPID is a next-generation bolometric experiment aiming at searching for neutrinoless double-beta decay with ~250 kg of isotopic mass of Mo. It will operate at 10 mK…

physics.ins-det2023★ 11 cited

Twelve-crystal prototype of LiMoO scintillating bolometers for CUPID and CROSS experiments

CUPID, CROSS collaborations, : +182

An array of twelve 0.28 kg lithium molybdate (LMO) low-temperature bolometers equipped with 16 bolometric Ge light detectors, aiming at optimization of detector structure for CROSS…

nucl-ex2022

New measurement of double beta decays of Mo to excited states of Ru with the CUPID-Mo experiment

Mo Collaboration, C. Augier, A. S. Barabash +79

The CUPID-Mo experiment, located at Laboratoire Souterrain de Modane (France), was a demonstrator experiment for CUPID. It consisted of an array of 20 LiMoO (LMO) cal…

physics.ins-det2022★ 1 cited

Characterization of a kg-scale archaeological lead-based cryogenic detectors for the RES-NOVA experiment

J. W. Beeman, G. Benato, C. Bucci +41

One of the most energetic events in the Universe are core-collapse Supernovae (SNe), where almost all the star's binding energy is released as neutrinos. These particles are direct…