Particle Dark Matter and DAMA/LIBRA

Journal Article · Fri Mar 26 04:00:00 EDT 2010 · AIP Conference Proceedings

DOI:https://doi.org/10.1063/1.3395996· OSTI ID:21367046

Bernabei, R; Nozzoli, F ^[1]; Belli, P ^[2]; Cappella, F; D'Angelo, A; Prosperi, D ^[3]; Cerulli, R ^[4]; Dai, C J; He, H L; Ma, X H; Sheng, X D; Wang, R G ^[5]; Incicchitti, A ^[6]; Montecchia, F ^[2]; Ye, Z P ^[5]

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1. Dip. di Fisica, Universita di Roma 'Tor Vergata', I-00133 Rome (Italy)
2. INFN, sez. Roma 'Tor Vergata', I-00133 Rome (Italy)
3. Dip. di Fisica, Universita di Roma 'LaSapienza', I-00185 Rome (Italy)
4. Laboratori Nazionali del Gran Sasso, I.N.F.N., Assergi (Italy)
5. IHEP, Chinese Academy, P.O. Box 918/3, Beijing 100039 (China)
6. INFN, sez. Roma, I-00185 Rome (Italy)

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.

• OSTI ID: 21367046
• Journal Information: AIP Conference Proceedings, Journal Name: AIP Conference Proceedings Journal Issue: 1 Vol. 1223; ISSN APCPCS; ISSN 0094-243X
• Country of Publication: United States
• Language: English

Related Subjects

46 INSTRUMENTATION RELATED TO NUCLEAR SCIENCE AND TECHNOLOGY
79 ASTRONOMY AND ASTROPHYSICS
ASTROPHYSICS
COSMIC RAY DETECTION
DETECTION
ELEMENTARY PARTICLES
GALAXIES
MATTER
MEASURING INSTRUMENTS
NAI DETECTORS
NONLUMINOUS MATTER
PARTICLE IDENTIFICATION
PHYSICS
POSTULATED PARTICLES
RADIATION DETECTION
RADIATION DETECTORS
SCINTILLATION COUNTERS
SOLID SCINTILLATION DETECTORS