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Direct dark matter search with the CRESST-III experiment - status and perspectives

Authors :
Willers, M
Angloher, G
Bento, A
Bucci, C
Canonica, L
Defay, X
Erb, A
von Feilitzsch, F
Iachellini, N
Gutlein, A
Gorla, P
Hauff, D
Jochum, J
Kiefer, M
Kluck, H
Kraus, H
Lanfranchi, J
Loebell, J
Mancuso, M
Munster, A
Pagliarone, C
Petricca, F
Potzel, W
Probst, F
Puig, R
Reindl, F
Schaffner, K
Schieck, J
Schonert, S
Seidel, W
Stahlberg, M
Stodolsky, L
Strandhagen, C
Strauss, R
Tanzke, A
Thi, H
Turkoglu, C
Uffinger, M
Ulrich, A
Usherov, I
Wawoczny, S
Wustrich, M
Zoller, A
Willers M
Angloher G
Bento A
Bucci C
Canonica L
Defay X
Erb A
von Feilitzsch F
Iachellini NF
Gutlein A
Gorla P
Hauff D
Jochum J
Kiefer M
Kluck H
Kraus H
Lanfranchi JC
Loebell J
Mancuso M
Munster A
Pagliarone C
Petricca F
Potzel W
Probst F
Puig R
Reindl F
Schaffner K
Schieck J
Schonert S
Seidel W
Stahlberg M
Stodolsky L
Strandhagen C
Strauss R
Tanzke A
Thi HHT
Turkoglu C
Uffinger M
Ulrich A
Usherov I
Wawoczny S
Wustrich M
Zoller A
Willers, M
Angloher, G
Bento, A
Bucci, C
Canonica, L
Defay, X
Erb, A
von Feilitzsch, F
Iachellini, N
Gutlein, A
Gorla, P
Hauff, D
Jochum, J
Kiefer, M
Kluck, H
Kraus, H
Lanfranchi, J
Loebell, J
Mancuso, M
Munster, A
Pagliarone, C
Petricca, F
Potzel, W
Probst, F
Puig, R
Reindl, F
Schaffner, K
Schieck, J
Schonert, S
Seidel, W
Stahlberg, M
Stodolsky, L
Strandhagen, C
Strauss, R
Tanzke, A
Thi, H
Turkoglu, C
Uffinger, M
Ulrich, A
Usherov, I
Wawoczny, S
Wustrich, M
Zoller, A
Willers M
Angloher G
Bento A
Bucci C
Canonica L
Defay X
Erb A
von Feilitzsch F
Iachellini NF
Gutlein A
Gorla P
Hauff D
Jochum J
Kiefer M
Kluck H
Kraus H
Lanfranchi JC
Loebell J
Mancuso M
Munster A
Pagliarone C
Petricca F
Potzel W
Probst F
Puig R
Reindl F
Schaffner K
Schieck J
Schonert S
Seidel W
Stahlberg M
Stodolsky L
Strandhagen C
Strauss R
Tanzke A
Thi HHT
Turkoglu C
Uffinger M
Ulrich A
Usherov I
Wawoczny S
Wustrich M
Zoller A
Publication Year :
2017

Abstract

The CRESST-III experiment, located in the Gran Sasso underground laboratory (LNGS, Italy), aims at the direct detection of dark matter (DM) particles. Scintillating CaWO4 crystals operated as cryogenic detectors are used as target material for DM-nucleus scattering. The simultaneous measurement of the phonon signal from the CaWO4 crystal and of the emitted scintillation light in a separate cryogenic light detector is used to discriminate backgrounds from a possible dark matter signal. The experiment aims to significantly improve the sensitivity for low-mass (less than or similar to 5-10 GeV/c(2)) DM particles by using optimized detector modules with a nuclear recoil-energy threshold less than or similar to 100 eV. The current status of the experiment as well as projections of the sensitivity for spin-independent DM-nucleon scattering will be presented.

Details

Database :
OAIster
Notes :
STAMPA, English
Publication Type :
Electronic Resource
Accession number :
edsoai.on1434547835
Document Type :
Electronic Resource