Particle Dark Matter and DAMA/LIBRA

2); (2) INFN Roma Tor Vergata; (3) Univ. Roma; 4); (4) INFN Roma; (5) INFN LNGS; (6) IHEP Beijing; 7); (7) Ing. Medica; 8) ((1) Univ. Roma Tor Vergata

Particle Dark Matter and DAMA/LIBRA

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arxiv 0912.0660 v1 pith:67CBV6GS submitted 2009-12-03 astro-ph.GA

R. Bernabei (1 , 2) , P. Belli (2) , F. Cappella (3 , 4) , R. Cerulli (5) , C.J. Dai (6) , A. d'Angelo (3

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H.L. He (6) A. Incicchitti (4) X.H. Ma (6) F. Montecchia (2 7) F. Nozzoli (1 D. Prosperi (3 X.D. Sheng (6) R.G. Wang (6) Z.P. Ye (6 8) ((1) Univ. Roma Tor Vergata (2) INFN Roma Tor Vergata (3) Univ. Roma (4) INFN Roma (5) INFN LNGS (6) IHEP Beijing (7) Ing. Medica Univ. Tor Vergata (8) Univ. Jing Gangshan)

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The DAMA/LIBRA set-up (about 250 kg highly radiopure NaI(Tl) sensitive mass) is running at the Gran Sasso National Laboratory of the I.N.F.N.. The first DAMA/LIBRA results confirm the evidence for the presence of a Dark Matter particle component in the galactic halo, as pointed out by the former DAMA/NaI set-up; cumulatively the data support such evidence at 8.2 sigma C.L. and satisfy all the many peculiarities of the Dark Matter annual modulation signature. The main aspects and prospects of this model independent experimental approach will be outlined.

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The SABRE South Technical Design Report Executive Summary
physics.ins-det 2024-11 conditional novelty 5.0 of 10

SABRE South, a 35-50 kg NaI(Tl) detector with a liquid scintillator veto at the Stawell Underground Physics Laboratory, is projected to reach 5 sigma discovery or 3 sigma exclusion of the DAMA/LIBRA annual modulation ...

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