Direct Dark Matter detection with CUORE

Details Direct Dark Matter detection with CUORE Direct Dark Matter detection with CUORE

Feb 2012

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2012jphcs.337a2067o&link_type=abstract

Journal of Physics: Conference Series, Volume 337, Issue 1, pp. 012067 (2012).

Physics

Scientific paper

The Cryogenic Underground Observatory for Rare Events (CUORE) is an experiment to search for neutrinoless double beta decay in 130Te and other rare processes. CUORE is a bolometric detector composed of 988 TeO2 crystals, with the total mass of about 1 tonne. The large detector mass, low backgrounds, and the low energy threshold of a few keV make the experiment well suited for direct detection of galactic dark matter particles and solar axions. We discuss the development of a novel low-energy trigger that enables such searches, and present the preliminary results from a test run with four CUORE-like crystals at Gran Sasso National Laboratory in Italy.

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