The data results collected by DAMA/LIBRA--phase1 deep underground at the Gran Sasso National Laboratory (LNGS) of the INFN during 7 annual cycles (total exposure of 1.04 ton $ imes$ yr) are briefly summarized. The DAMA/LIBRA--phase1 data give evidence for the presence of Dark Matter (DM) particles in the galactic halo, on the basis of the exploited model independent DM annual modulation signature by using highly radio-pure NaI(Tl) target. Including also the first generation DAMA/NaI experiment (cumulative exposure $1.33$ ton $ imes$ yr, corresponding to 14 annual cycles), the C.L. is 9.3 $sigma$ and the modulation amplitude of the {it single-hit} events in the (2--6) keV energy interval is: $(0.0112 pm 0.0012)$ cpd/kg/keV; the measured phase is $(144pm 7)$ days and the measured period is $(0.998pm 0.002)$ yr, values well in agreement with those expected for DM particles. No systematic or side reaction able to mimic the exploited DM signature has been found or suggested by anyone over more than a decade. Some of the perspectives of the presently running DAMA/LIBRA--phase2 are outlined.

Bernabei, R., Belli, P., Di Marco, A., Montecchia, F., Cappella, F., D'Angelo, A., et al. (2013). Particle dark matter: DAMA/LIBRA results and perspectives. In A. Studenikin (a cura di), Particle physics at the tercentenary of Mikhail Lomonosov: Proceedings of the 15. Lomonosov conference on elementary particle physics, Moscow, Russia, 18 – 24 August 2011 (pp. 219-229). singapore : World Scientific [10.1142/9789814436830_0049].

Particle dark matter: DAMA/LIBRA results and perspectives

BERNABEI, RITA;Montecchia F;
2013-01-01

Abstract

The data results collected by DAMA/LIBRA--phase1 deep underground at the Gran Sasso National Laboratory (LNGS) of the INFN during 7 annual cycles (total exposure of 1.04 ton $ imes$ yr) are briefly summarized. The DAMA/LIBRA--phase1 data give evidence for the presence of Dark Matter (DM) particles in the galactic halo, on the basis of the exploited model independent DM annual modulation signature by using highly radio-pure NaI(Tl) target. Including also the first generation DAMA/NaI experiment (cumulative exposure $1.33$ ton $ imes$ yr, corresponding to 14 annual cycles), the C.L. is 9.3 $sigma$ and the modulation amplitude of the {it single-hit} events in the (2--6) keV energy interval is: $(0.0112 pm 0.0012)$ cpd/kg/keV; the measured phase is $(144pm 7)$ days and the measured period is $(0.998pm 0.002)$ yr, values well in agreement with those expected for DM particles. No systematic or side reaction able to mimic the exploited DM signature has been found or suggested by anyone over more than a decade. Some of the perspectives of the presently running DAMA/LIBRA--phase2 are outlined.
2013
Settore FIS/04 - FISICA NUCLEARE E SUBNUCLEARE
English
Rilevanza internazionale
Capitolo o saggio
Dark Matter; DAMA; Gran Sasso; low background technique
https://www.worldscientific.com/worldscibooks/10.1142/8645
Bernabei, R., Belli, P., Di Marco, A., Montecchia, F., Cappella, F., D'Angelo, A., et al. (2013). Particle dark matter: DAMA/LIBRA results and perspectives. In A. Studenikin (a cura di), Particle physics at the tercentenary of Mikhail Lomonosov: Proceedings of the 15. Lomonosov conference on elementary particle physics, Moscow, Russia, 18 – 24 August 2011 (pp. 219-229). singapore : World Scientific [10.1142/9789814436830_0049].
Bernabei, R; Belli, P; Di Marco, A; Montecchia, F; Cappella, F; D'Angelo, A; Incicchitti, A; Prosperi, D; R., C; Dai C., J; He H., L; Ma X., H; Sheng X., D; Wang R., G; Ye, Zp
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Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/2108/255524
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