Challenges for dark matter direct search with SiPMs

Liquid xenon and liquid argon detectors are leading the direct dark matter search and are expected to be the candidate technology for the forthcoming generation of ultra-sensitive large-mass detectors. At present, scintillation light detection in those experiments is based on ultra-pure low-noise ph...

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Main Authors: Alessandro Razeto, Nicola Rossi
Format: Article
Language:English
Published: Frontiers Media S.A. 2024-01-01
Series:Frontiers in Physics
Subjects:
Online Access:https://www.frontiersin.org/articles/10.3389/fphy.2023.1290449/full
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author Alessandro Razeto
Nicola Rossi
author_facet Alessandro Razeto
Nicola Rossi
author_sort Alessandro Razeto
collection DOAJ
description Liquid xenon and liquid argon detectors are leading the direct dark matter search and are expected to be the candidate technology for the forthcoming generation of ultra-sensitive large-mass detectors. At present, scintillation light detection in those experiments is based on ultra-pure low-noise photo-multipliers. To overcome the issues in terms of the extreme radio-purity, costs, and technological feasibility of the future dark matter experiments, the novel silicon photomultiplier (SiPM)-based photodetector modules seem to be promising candidates, capable of replacing the present light detection technology. However, the intrinsic features of SiPMs may limit the present expectations. In particular, interfering phenomena, especially related to the optical correlated noise, can degrade the energy and pulse shape resolutions. As a consequence, the projected sensitivity of the future detectors has to be reconsidered accordingly.
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spelling doaj.art-59c5343052894dbe9ed173c1bfeb16bf2024-01-03T04:31:37ZengFrontiers Media S.A.Frontiers in Physics2296-424X2024-01-011110.3389/fphy.2023.12904491290449Challenges for dark matter direct search with SiPMsAlessandro RazetoNicola RossiLiquid xenon and liquid argon detectors are leading the direct dark matter search and are expected to be the candidate technology for the forthcoming generation of ultra-sensitive large-mass detectors. At present, scintillation light detection in those experiments is based on ultra-pure low-noise photo-multipliers. To overcome the issues in terms of the extreme radio-purity, costs, and technological feasibility of the future dark matter experiments, the novel silicon photomultiplier (SiPM)-based photodetector modules seem to be promising candidates, capable of replacing the present light detection technology. However, the intrinsic features of SiPMs may limit the present expectations. In particular, interfering phenomena, especially related to the optical correlated noise, can degrade the energy and pulse shape resolutions. As a consequence, the projected sensitivity of the future detectors has to be reconsidered accordingly.https://www.frontiersin.org/articles/10.3389/fphy.2023.1290449/fullnoble gas detectorstime projection chamberlight yielddark mattersilicon photomultiplieroptical cross-talk
spellingShingle Alessandro Razeto
Nicola Rossi
Challenges for dark matter direct search with SiPMs
Frontiers in Physics
noble gas detectors
time projection chamber
light yield
dark matter
silicon photomultiplier
optical cross-talk
title Challenges for dark matter direct search with SiPMs
title_full Challenges for dark matter direct search with SiPMs
title_fullStr Challenges for dark matter direct search with SiPMs
title_full_unstemmed Challenges for dark matter direct search with SiPMs
title_short Challenges for dark matter direct search with SiPMs
title_sort challenges for dark matter direct search with sipms
topic noble gas detectors
time projection chamber
light yield
dark matter
silicon photomultiplier
optical cross-talk
url https://www.frontiersin.org/articles/10.3389/fphy.2023.1290449/full
work_keys_str_mv AT alessandrorazeto challengesfordarkmatterdirectsearchwithsipms
AT nicolarossi challengesfordarkmatterdirectsearchwithsipms