Author:
,Angloher G.,Banik S.,Benato G.,Bento A.,Bertolini A.,Breier R.,Bucci C.,Burkhart J.,Canonica L.,D’Addabbo A.,Lorenzo S. Di,Einfalt L.,Erb A.,Feilitzsch F. v.,Fichtinger S.,Fuchs D.,Garai A.,Ghete V. M.,Gorla P.,Guillaumon P. V.,Gupta S.,Hauff D.,Jes̆kovský M.,Jochum J.,Kaznacheeva M.,Kinast A.,Kluck H.,Kraus H.,Kuckuk S.,Langenkämper A.,Mancuso M.,Marini L.,Mauri B.,Meyer L.,Mokina V.,Olmi M.,Ortmann T.,Pagliarone C.,Pattavina L.,Petricca F.,Potzel W.,Povinec P.,Pröbst F.,Pucci F.,Reindl F.,Rothe J.,Schäffner K.,Schieck J.,Schönert S.,Schwertner C.,Stahlberg M.,Stodolsky L.,Strandhagen C.,Strauss R.,Usherov I.,Wagner F.,Willers M.,Zema V.
Abstract
AbstractDiamond operated as a cryogenic calorimeter is an excellent target for direct detection of low-mass dark matter candidates. Following the realization of the first low-threshold cryogenic detector that uses diamond as absorber for astroparticle physics applications, we now present the resulting exclusion limits on the elastic spin-independent interaction cross-section of dark matter with diamond. We measured two 0.175 g CVD (Chemical Vapor Deposition) diamond samples, each instrumented with a Transition Edge Sensor made of Tungsten (W-TES). Thanks to the energy threshold of just 16.8 eV of one of the two detectors, we set exclusion limits on the elastic spin-independent interaction of dark matter particles with carbon nuclei down to dark matter masses as low as 0.122 GeV/c$$^2$$
2
. This work shows the scientific potential of cryogenic detectors made from diamond and lays the foundation for the use of this material as target for direct detection dark matter experiments.
Publisher
Springer Science and Business Media LLC