14–24 Jul 2025
CICG - International Conference Centre - Geneva, Switzerland
Europe/Zurich timezone
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Development of a GAGG-based low-background neutron detector

23 Jul 2025, 16:05
15m
Room 4

Room 4

Talk Dark-Matter Physics DM

Speaker

Andrea MOLINARIO (Istituto Nazionale di Astrofisica)

Description

In rare events experiments, such as those devoted to the direct search of dark matter, a precise knowledge of the environmental gamma and neutron backgrounds is crucial for the design of appropriate shieldings. The neutron component is often poorly known due to the lack of a scalable detector technology for the measurement of low-flux neutron spectra in a short time.
Thanks to their high gadolinium content, we are investigating the possibility of using scintillating Gd$_3$Al$_2$Ga$_3$O$_{12}$ (GAGG) crystals as portable neutron detectors, in alternative to $^3$He counters. GAGG features a high scintillation light yield, good timing performance, and the capability of particle identification via pulse-shape discrimination. In a low-background environment, the distinctive signature produced by neutron capture on gadolinium, namely a $\gamma$-ray cascade releasing $\sim$8 MeV of total energy, and the efficient particle identification provided by GAGG would yield a background-free neutron capture signal.
In this contribution, we will present the characterization of a first GAGG detector prototype in terms of particle discrimination performance, intrinsic radioactive contamination, and neutron response. We will then discuss possible further developments of this detector technology towards the realization of a portable setup for the neutron spectrum measurement in various locations at the INFN Gran Sasso National Laboratory (LNGS).

Authors

Giovanni Benato (Gran Sasso Science Institute) Yingjie Chu (Gran Sasso Science Institute) Giuseppe Di Carlo (INFN - National Institute for Nuclear Physics) Andrea MOLINARIO (Istituto Nazionale di Astrofisica) Silvia Vernetto (Istituto Nazionale di Astrofisica)

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