COSINUS:TES-instrumented NaI Crystals for Direct Dark Matter Search

被引：0

作者：

Stahlberg, M. ^{[1
]}

Angloher, G. ^{[1
]}

Bharadwaj, M. R. ^{[1
]}

Cababie, M. R. ^{[5
,6
]}

Dafinei, I. ^{[2
,3
]}

Di Marco, N. ^{[2
,4
]}

Einfalt, L. ^{[5
,6
]}

Ferroni, F. ^{[2
,3
]}

Fichtinger, S. ^{[5
]}

Filipponi, A. ^{[4
,7
]}

Frank, T. ^{[1
]}

Friedl, M. ^{[5
]}

Fuss, A. ^{[5
,6
]}

Ge, Z. ^{[9
]}

Heikinheimo, M. ^{[10
]}

Hughes, M. N. ^{[1
]}

Huitu, K. ^{[10
]}

Kellermann, M. ^{[1
]}

Maji, R. ^{[5
,6
]}

Mancuso, M. ^{[1
]}

Pagnanini, L. ^{[2
,4
]}

Petricca, F. ^{[1
]}

Pirro, S. ^{[2
]}

Proebst, F. ^{[1
]}

Profeta, G. ^{[4
,7
]}

Puiu, A. ^{[2
,4
]}

Reindl, F. ^{[5
,6
]}

Schaeffner, K. ^{[1
]}

Schieck, J. ^{[5
,6
]}

Schmiedmayer, D. ^{[5
,6
]}

Schreiner, P. ^{[5
,6
]}

Schwertner, C. ^{[5
,6
]}

Shera, K. ^{[1
]}

Stendahl, A. ^{[10
]}

Stukel, M. ^{[2
,4
]}

Tresca, C. ^{[4
,8
]}

Wagner, F. ^{[5
]}

Yue, S. ^{[9
]}

Zema, V. ^{[1
]}

Zhu, Y. ^{[9
]}

机构：

[1] Max Planck Inst Phys & Astrophys, D-80805 Munich, Germany

[2] Gran Sasso Sci Inst, I-67100 Laquila, Italy

[3] INFN, Sez Roma, I-00185 Rome, Italy

[4] INFN, Lab Nazl Gran Sasso, I-67100 Laquila, Italy

[5] Austrian Acad Sci, Inst Hochenergiephys, A-1050 Vienna, Austria

[6] Tech Univ Wien, Atominst, A-1050 Vienna, Austria

[7] Univ Aquila, Dipartimento Sci Fis & Chim, I-67100 Laquila, Italy

[8] Univ LAquila, Dipartimento Sci Fis & Chim, CNR SPIN, I-67100 Laquila, Italy

[9] Chinese Acad Sci, Shanghai Inst Ceram, SICCAS, Shanghai 201899, Peoples R China

[10] Univ Helsinki, Helsinki Inst Phys, Helsinki 00014, Finland

来源：

JOURNAL OF LOW TEMPERATURE PHYSICS | 2024年 / 217卷 / 3-4期

关键词：

Direct search for dark matter; Annual modulations; Transition edge sensors; Cryogenic detectors; NaI detectors;

D O I：

10.1007/s10909-024-03185-z

中图分类号：

O59 [应用物理学];

学科分类号：

摘要：

In the last years, the COSINUS (Cryogenic Observatory for SIgnals seen in Next generation Underground Searches) experiment has made significant progress both in the construction of its facility and in pursuing its physics goals: At Laboratori Nazionali del Gran Sasso (LNGS) in Italy, an underground facility was constructed, which will house experimental detectors for dark matter direct detection in a dry dilution cryostat. Construction of the main structures at the COSINUS site is finished, including the control building, the cryostat access level, and the water tank which will serve as a Cherenkov muon veto around the cryostat. With a nuclear recoil threshold of 4 keV, the latest COSINUS detector prototype approaches the design goal of 1 keV, and particle discrimination on event-by-event basis has been demonstrated. This contribution gives a brief overview on the status of COSINUS.

引用

页码：350 / 357

页数：8

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