4.5 Article Proceedings Paper

Light Collection of Some Molybdate Crystal Absorbers for Cryogenic Calorimeters at Millikelvin Temperatures

期刊

IEEE TRANSACTIONS ON NUCLEAR SCIENCE
卷 70, 期 7, 页码 1307-1311

出版社

IEEE-INST ELECTRICAL ELECTRONICS ENGINEERS INC
DOI: 10.1109/TNS.2023.3267387

关键词

Advanced Mo-based rare process experiment (AMoRE); cryogenic calorimeter; decay; molybdate crystals; neutrinoless double beta; scintillation

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This study reports on the light collection of cryogenic calorimeters using different molybdate crystals as absorbers. The light signals from gamma rays and alpha particles are studied, and the light collection of the crystals is assessed by comparing the scintillation signals with known X-ray signals. The results show that the light measurement with LMO and NMO crystals is significantly lower compared to CMO, and the quenching factor for alpha particles is also different for different crystals.
Scintillating molybdate crystals recently got significant attention for their applications in rare event searches, such as neutrinoless double beta decay experiments. In this article, we report on the light collection of cryogenic calorimeters operating at 10 mK, using CaMoO4 (CMO), (Li2MoO4)-Mo-100 (LMO), and Na2Mo2O7 (NMO) crystal absorbers. Scintillation signals from gamma rays and alpha particles are studied. Germanium (Ge) and silicon (Si) wafers, which work as light absorbers, coupled to metallic magnetic calorimeters (MMC), are used as scintillation light detectors. By comparing the scintillation signals with direct hit X-ray signals of known energies, which occurred in the light absorber, we assess the light collection of the crystal scintillation. Eight keV copper X-rays are analyzed in the case of both the Ge and Si wafer detectors. The light measurement with LMO and NMO crystals at millikelvin temperatures is 9.6x and 7.6x less compared with the CMO for 2.615-MeV gamma rays from 208Tl. Additionally, we found that for NMO, the detected scintillation light for alpha particles is quenched by a factor of 0.06 compared to that of gamma rays for a given energy by investigating the light signal from 2.615-MeV gamma rays and 5.4-MeV alpha particles. For the CMO, in the same way, the quenching factor is measured to be 0.22. The quenching factor for 4.785-MeV alpha particles (Li-6 neutron capture) in LMO crystal is about 0.28 compared to the scintillation from 2.615-MeV gamma rays.

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