DAMA/LIBRA–phase2 results and implications on several dark matter scenarios

Author:

Bernabei R.12,Belli P.12,Caracciolo V.12,Cerulli R.12,Merlo V.12,Cappella F.34,d’Angelo A.34,Incicchitti A.34,Di Marco A.2,Dai C. J.5,He H. L.5,Ma X. H.5,Sheng X. D.5,Montecchia F.26,Ye Z. P.57

Affiliation:

1. Dip. di Fisica, Università di Roma “Tor Vergata”, Rome, Italy

2. INFN, sez. Roma “Tor Vergata”, Rome, Italy

3. Dip. di Fisica, Università di Roma “La Sapienza”, Rome, Italy

4. INFN, sez. Roma, Rome, Italy

5. Key Laboratory of Particle Astrophysics, Institute of High Energy Physics, Chinese Academy of Sciences, Beijing, P. R. China

6. Dip. Ingegneria Civile e Ingegneria Informatica, Università di Roma “Tor Vergata”, Rome, Italy

7. University of Jinggangshan, Ji’an, Jiangxi, P. R. China

Abstract

The first DAMA/LIBRA–phase2 model-independent results (exposure: [Formula: see text], and software energy threshold at 1 keV). They further confirm — with high confidence level — the evidence already observed by DAMA/NaI and DAMA/LIBRA–phase1 on the basis of the exploited model-independent dark matter (DM) annual modulation signature. The total exposure of the three experiments above the 2 keV software energy threshold is [Formula: see text]. Here, several DM candidate particles and related scenarios are analyzed including the latest results. Thanks to the increased exposure and to the lower software energy threshold, corollary model-dependent analyses permit to significantly restrict the allowed regions for the parameters spaces of various dark matter candidates and astrophysical, particle and nuclear physics scenarios.

Publisher

World Scientific Pub Co Pte Lt

Subject

Astronomy and Astrophysics,Nuclear and High Energy Physics,Atomic and Molecular Physics, and Optics

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