Cryogenic Wide-Area Light Detectors for Neutrino and Dark Matter Searches

被引:5
|
作者
Di Domizio, S. [1 ,7 ]
Bagni, R. [2 ]
Battistelli, E. S. [2 ]
Bellini, F. [2 ,3 ]
Bucci, C. [4 ]
Calvo, M. [5 ]
Cardani, L. [2 ,3 ]
Castellano, M. G. [6 ]
Coppolecchia, A. [2 ]
Cosmelli, C. [2 ,3 ]
Cruciani, A. [2 ]
D'Addabbo, A. [2 ,5 ]
de Bernardis, P. [2 ]
Masi, S. [2 ]
Pinci, D. [3 ]
Vignati, M. [3 ]
机构
[1] Univ Genoa, Dipartimento Fis, Genoa, Italy
[2] Univ Roma La Sapienza, Dipartimento Fis, I-00185 Rome, Italy
[3] Ist Nazl Fis Nucl, Sez Roma, Rome, Italy
[4] Ist Nazl Fis Nucl, Lab Nazl Gran Sasso, Laquila, Italy
[5] Univ Grenoble 1, CNRS, Inst Neel, F-38402 St Martin Dheres, France
[6] CNR, Ist Foton & Nanotecnol, Rome, Italy
[7] Ist Nazl Fis Nucl, Sez Genova, I-16146 Genoa, Italy
关键词
Light detectors; Kinetic inductance detectors; Rare event searches; Bolometers;
D O I
10.1007/s10909-013-1076-2
中图分类号
O59 [应用物理学];
学科分类号
摘要
Large-mass arrays of bolometers proved to be good detectors for neutrinoless double beta decay (0DBD) and dark matter searches. CUORE and LUCIFER are bolometric 0DBD experiments that will start to take data in 2015 at Laboratori Nazionali del Gran Sasso in Italy. The sensitivity of CUORE could be increased by removing the background due to particles, by detecting the small amount of erenkov light (100 eV) emitted by the s' signal and not by s. LUCIFER could be extended to detect also dark matter, provided that the background from / particles (100 eV of scintillation light) is discriminated from nuclear recoils of about 10 keV energy (no light). We have recently started to develop light detectors for CUORE, LUCIFER and similar bolometric experiments. The aim is to obtain detectors with an active area of (the face of bolometric crystals), operating at 10 mK, and with an energy resolution at the baseline below 20 eV RMS. We have chosen to develop phonon-mediated detectors with KID sensors. We are currently testing the first prototypes.
引用
收藏
页码:917 / 923
页数:7
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