DarkSide-50 is a dark matter direct search experiment at LNGS, searching for rare nuclear recoils possibly induced by WIMPs. It has two nested vetoes and a dual phase liquid argon TPC as dark matter detector. Key features of this experiment are the use of underground argon as radio-pure target and of muon and neutron active vetoes to suppress the background. The first data-taking campaign was running from November 2013 to April 2015 with an atmospheric argon target and a reduced efficiency neutron veto due to internal contamination. However, an upper limit on the WIMP-nucleon cross section of 6.1×10−44 cm2 at 90% CL was obtained for a WIMP mass of 100 GeV/c2 and an exposure of (1422 ± 67) kg·d. At present DarkSide-50 started a 3 years run...
DarkSide uses a dual-phase Liquid Argon Time Projection Chamber to search for WIMP dark matter. The ...
The DarkSide-50 experiment, located at the "Laboratori Nazionali del Gran Sasso (INFN)", is based on...
We present a search for dark matter particles with sub-GeV/c^{2} masses whose interactions have fina...
The DarkSide experiment aims to perform a background-free direct search for dark matter with a dual-...
The existence of dark matter is known because of its gravitational effects, and although its nature ...
DarkSide is direct-detection dark-matter experimental project based on radiopure argon. The main goa...
DarkSide is direct-detection dark-matter experimental project based on radiopure argon. The main goa...
We present the results of a search for dark matter weakly interacting massive particles (WIMPs) in t...
AbstractWe report the first results of DarkSide-50, a direct search for dark matter operating in the...
The DarkSide-50 direct-detection dark matter experiment is a dual-phase argon time projection chambe...
We report the first results of DarkSide-50, a direct search for dark matter operating in the undergr...
DarkSide is a graded experimental project based on radiopure argon, and is now, and will be, used in...
DarkSide (DS) at Gran Sasso underground laboratory is a direct Dark Matter search program based on T...
Although the existence of dark matter is supported by many evidences, based on astrophysical measure...
Although the existence of dark matter is supported by many evidences, based on astrophysical measure...
DarkSide uses a dual-phase Liquid Argon Time Projection Chamber to search for WIMP dark matter. The ...
The DarkSide-50 experiment, located at the "Laboratori Nazionali del Gran Sasso (INFN)", is based on...
We present a search for dark matter particles with sub-GeV/c^{2} masses whose interactions have fina...
The DarkSide experiment aims to perform a background-free direct search for dark matter with a dual-...
The existence of dark matter is known because of its gravitational effects, and although its nature ...
DarkSide is direct-detection dark-matter experimental project based on radiopure argon. The main goa...
DarkSide is direct-detection dark-matter experimental project based on radiopure argon. The main goa...
We present the results of a search for dark matter weakly interacting massive particles (WIMPs) in t...
AbstractWe report the first results of DarkSide-50, a direct search for dark matter operating in the...
The DarkSide-50 direct-detection dark matter experiment is a dual-phase argon time projection chambe...
We report the first results of DarkSide-50, a direct search for dark matter operating in the undergr...
DarkSide is a graded experimental project based on radiopure argon, and is now, and will be, used in...
DarkSide (DS) at Gran Sasso underground laboratory is a direct Dark Matter search program based on T...
Although the existence of dark matter is supported by many evidences, based on astrophysical measure...
Although the existence of dark matter is supported by many evidences, based on astrophysical measure...
DarkSide uses a dual-phase Liquid Argon Time Projection Chamber to search for WIMP dark matter. The ...
The DarkSide-50 experiment, located at the "Laboratori Nazionali del Gran Sasso (INFN)", is based on...
We present a search for dark matter particles with sub-GeV/c^{2} masses whose interactions have fina...