DAMA/LIBRA results and perspectives
R. Bernabei (1), P. Belli (1), S. d'Angelo (1), A. Di Marco (1), F., Montecchia (1,5), A. d'Angelo (2), A. Incicchitti (2), F. Cappella (3), V., Caracciolo (3), R. Cerulli (3), C.J. Dai (4), H.L. He (4), H.H. Kuang (4),, X.H. Ma (4), X.D. Sheng (4), R.G. Wang (4), Z.P. Ye (4

TL;DR
The DAMA/LIBRA experiment has observed a significant annual modulation signal consistent with dark matter particles in the galactic halo, with ongoing phase 2 aiming to improve sensitivity.
Contribution
This paper reports the first phase results of DAMA/LIBRA confirming dark matter detection via annual modulation, and discusses perspectives for phase 2 improvements.
Findings
9.3 sigma evidence for dark matter particles
No systematic effects mimicking the signal
Ongoing phase 2 with increased sensitivity
Abstract
The DAMA/LIBRA experiment ( 250 kg of highly radio-pure NaI(Tl)) is running deep underground at the Gran Sasso National Laboratory (LNGS) of the I.N.F.N. Here we briefly recall the results obtained in its first phase of measurements (DAMA/LIBRA--phase1, total exposure: 1.04 ton yr). DAMA/LIBRA--phase1 and the former DAMA/NaI (cumulative exposure: ton yr) give evidence at 9.3 C.L. for the presence of DM particles in the galactic halo by exploiting the model-independent DM annual modulation signature. No systematic or side reaction able to mimic the exploited DM signature has been found or suggested by anyone over more than a decade. At present DAMA/LIBRA--phase2 is running with increased sensitivity.
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