Latest results of CRESST-III's search for sub-GeV/c(2) dark matter
Paper in proceeding, 2020
The CRESST-III experiment searches for direct interactions of dark matter with ordinary matter. The main event signature would be a nuclear recoil inside one of the scintillating CaWO4 crystals. Operating the crystals as cryogenic calorimeters provides a phonon signal as measure of the deposited energy. The simultaneous readout of both signals is used to actively discriminate backgrounds. CRESST-III focuses on the sub-GeV/c(2) mass region where the sensitivity is driven by the threshold. In the first data taking campaign of CRESST-III from 2016-2018 an unprecedented low threshold of 30.1 eV for nuclear recoils was obtained. In this contribution, we will report the status of the experiment and the latest results. [GRAPHICS]
Author
H. Kluck
Vienna University of Technology
Austrian Academy of Sciences
A. H. Abdelhameed
Max Planck Society
G. Angloher
Max Planck Society
P. Bauer
Max Planck Society
A. Bento
University of Coimbra
Max Planck Society
E. Bertoldo
Max Planck Society
R. Breier
Comenius University in Bratislava
C. Bucci
National Institute for Nuclear Physics
L. Canonica
Comenius University in Bratislava
A. D'Addabbo
Gran Sasso Science Institute (GSSI)
National Institute for Nuclear Physics
S. Di Lorenzo
National Institute for Nuclear Physics
Gran Sasso Science Institute (GSSI)
A. Erb
Technical University of Munich
Walther-Meissner-Institute for Low Temperature Research
F. v. Feilitzsch
Technical University of Munich
N. Ferreiro Iachellini
Max Planck Society
S. Fichtinger
Austrian Academy of Sciences
A. Fuss
Austrian Academy of Sciences
Vienna University of Technology
P. Gorla
National Institute for Nuclear Physics
D. Hauff
Max Planck Society
M. Jeskovsky
Comenius University in Bratislava
J. Jochum
University of Tübingen
J. Kaizer
Comenius University in Bratislava
A. Kinast
Technical University of Munich
H. Krauss
University of Oxford
A. Langenkaemper
Technical University of Munich
M. Mancuso
Max Planck Society
V. Mokina
Austrian Academy of Sciences
E. Mondragon
Technical University of Munich
M. Olmi
Gran Sasso Science Institute (GSSI)
National Institute for Nuclear Physics
T. Ortmann
Technical University of Munich
C. Pagliarone
Universita di Cassino e del Lazio Meridionale
National Institute for Nuclear Physics
V. Palusova
Comenius University in Bratislava
L. Pattavina
Technical University of Munich
Gran Sasso Science Institute (GSSI)
F. Petricca
Max Planck Society
W. Potzel
Technical University of Munich
P. Povinec
Comenius University in Bratislava
F. Proebst
Max Planck Society
F. Reindl
Vienna University of Technology
Austrian Academy of Sciences
J. Rothe
Max Planck Society
K. Schaeffner
Max Planck Society
J. Schieck
Austrian Academy of Sciences
Vienna University of Technology
V. Schipperges
University of Tübingen
D. Schmiedmayer
Vienna University of Technology
Austrian Academy of Sciences
S. Schoenert
Technical University of Munich
C. Schwertner
Vienna University of Technology
Austrian Academy of Sciences
M. Stahlberg
Vienna University of Technology
Austrian Academy of Sciences
L. Stodolsky
Max Planck Society
C. Strandhagen
University of Tübingen
R. Strauss
Technical University of Munich
I. Usherov
University of Tübingen
M. Willers
Technical University of Munich
Vanessa Zema
Gran Sasso Science Institute (GSSI)
Laboratori Nazionali del Gran Sasso
Chalmers, Physics, Subatomic and Plasma Physics
J. Zeman
Comenius University in Bratislava
Journal of Physics: Conference Series
1742-6588 (ISSN) 17426596 (eISSN)
Vol. 1468 1 012038
16th International Conference on Topics in Astroparticle and Underground Physics (TAUP)
Toyama, Japan,
Toyama, Japan,
Subject Categories
Accelerator Physics and Instrumentation
Subatomic Physics
Astronomy, Astrophysics and Cosmology
DOI
10.1088/1742-6596/1468/1/012038