Bossa, M. (2015) DArKSIDE-50: A view of the first atmospheric argon run. Il nuovo cimento C, 38 (1). pp. 1-2. ISSN 1826-9885
|
Text
ncc10928.pdf - Published Version Download (315kB) | Preview |
Official URL: https://www.sif.it/riviste/sif/ncc/econtents/2015/...
Abstract
The DArKside (DS) program aims to detect the so-called WIMPs (Weakly Interactive Massive Particle) which are considered the best candidates for Dark Matter. WIMPs elastically scattering would be detected by using a twophase Time Projection Chamber (TPC) based on argon nuclei target. Thanks to the properties of the scintillation and ionization signals detected by the TPC it is possible to discriminate a WIMP-induced signal from one induced by background. DS-50 started its data taking on November 2013 with atmospheric argon (later with underground argon depleted in 39Ar.)
Item Type: | Article |
---|---|
Uncontrolled Keywords: | Dark matter (stellar, interstellar, galactic, and cosmological) ; Radiation detectors |
Subjects: | 500 Scienze naturali e Matematica > 530 Fisica |
Depositing User: | Marina Spanti |
Date Deposited: | 26 May 2020 09:58 |
Last Modified: | 26 May 2020 09:58 |
URI: | http://eprints.bice.rm.cnr.it/id/eprint/18912 |
Actions (login required)
View Item |