Title of article
Particle dark matter signal in DAMA/LIBRA
Author/Authors
Bernabei، نويسنده , , R. and Belli، نويسنده , , P. and Di Marco، نويسنده , , A. and Montecchia، نويسنده , , F. and Cappella، نويسنده , , F. and dʹAngelo، نويسنده , , A. and Incicchitti، نويسنده , , A. and Prosperi، نويسنده , , D. and Cerulli، نويسنده , , R. and Dai، نويسنده , , C.J. and He، نويسنده , , H.L. and Ma، نويسنده , , X.H. and Sheng، نويسنده , , X.D. and Wang، نويسنده , , R.G. and Ye، نويسنده , , Z.P.، نويسنده ,
Pages
3
From page
120
To page
122
Abstract
The DAMA/LIBRA experiment, running at LNGS, has a sensitive mass of about 250 kg highly radiopure NaI(Tl) and it is mainly devoted to the investigation of Dark Matter (DM) particles in the Galactic halo by exploiting the model independent DM annual modulation signature. The present DAMA/LIBRA experiment and the former DAMA/NaI one have released so far results corresponding to a total exposure of 1.17 ton×yr over 13 annual cycles. They provide a model independent evidence of the presence of DM particles in the galactic halo at 8.9 σ C.L.
Keywords
Scintillators , Dark matter , Rare processes , NaI(Tl)
Journal title
Astroparticle Physics
Record number
2019789
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