The CROSS demonstrator: structure, performance and physics reach

27 Aug 2025, 17:20
20m
North Hall #2

North Hall #2

Oral Neutrino Physics and Astrophysics Neutrino Physics and Astrophysics

Speaker

Dr Andrea Giuliani (CNRS/IJCLab)

Description

Cryogenic detectors are promising instruments for investigating neutrinoless double beta decay. The CROSS project (Cryogenic Rare-event Observatory with Surface Sensitivity) aims to advance bolometric techniques using $^{100}$Mo and $^{130}$Te. The final detector, ready for commissioning at the underground Canfranc Laboratory in Spain, consists of 36 Li₂MoO₄ and 6 TeO₂ crystals, most of which will be enriched in the relevant isotope. Each crystal is coupled to a light detector to enable effective alpha background discrimination. Signal enhancement via the Neganov-Trofimov-Luke effect, combined with fast signal rise times (~0.5 ms), helps suppress background from random coincidences of two-neutrino double beta decay events.

With 4.7 kg of $^{100}$Mo and a background index of 3.2×10⁻³ counts/(keV·kg·yr), CROSS aims—after two years of data taking—to reach a $^{100}$Mo half-life sensitivity of 9.3×10²⁴ years. This would probe the effective Majorana mass down to 130–210 meV, potentially setting the most stringent global limits for this isotope.

Collaboration you are representing CROSS

Author

Dr Andrea Giuliani (CNRS/IJCLab)

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