In this conference the model-independent result on the presence of dark-matter particles in the galactic halo obtained over seven annual cycles by the 100 kg highly radiopure NaI(Tl) DAMA/NaI has been presented and several corollary investigations have also been discussed. More recently the model-independent result obtained over the first four annual cycles by the second generation 250 kg highly radiopure NaI(Tl) DAMA/LIBRA set-up at the Gran Sasso National Laboratory of the INFN has also been released. Both the experiments have the unique feature to effectively investigate the presence of dark-matter particles in the galactic halo by exploiting the model-independent annual modulation signature. The data collected by the two experiments over eleven annual cycles for a total exposure of 0.82 ton × y have pointed out at 8.2σ CL a positive result; several corollary model-dependent quests for the candidate particle(s) and related astrophysical, nuclear and particle physics scenarios are under updating. The future experimental activity can give rise to many new interesting results.
Bernabei, R., Belli, P., Cappella, F., Cerulli, R., Dai, C., D'Angelo, A., et al. (2008). Direct detection of dark matter particles. IL NUOVO CIMENTO DELLA SOCIETÀ ITALIANA DI FISICA. B, GENERAL PHYSICS, RELATIVITY, ASTRONOMY AND MATHEMATICAL PHYSICS AND METHODS, 123(6-7), 928-931 [10.1393/ncb/i2008-10561-3].
Direct detection of dark matter particles
BERNABEI, RITA;MONTECCHIA, FRANCESCO;
2008-01-01
Abstract
In this conference the model-independent result on the presence of dark-matter particles in the galactic halo obtained over seven annual cycles by the 100 kg highly radiopure NaI(Tl) DAMA/NaI has been presented and several corollary investigations have also been discussed. More recently the model-independent result obtained over the first four annual cycles by the second generation 250 kg highly radiopure NaI(Tl) DAMA/LIBRA set-up at the Gran Sasso National Laboratory of the INFN has also been released. Both the experiments have the unique feature to effectively investigate the presence of dark-matter particles in the galactic halo by exploiting the model-independent annual modulation signature. The data collected by the two experiments over eleven annual cycles for a total exposure of 0.82 ton × y have pointed out at 8.2σ CL a positive result; several corollary model-dependent quests for the candidate particle(s) and related astrophysical, nuclear and particle physics scenarios are under updating. The future experimental activity can give rise to many new interesting results.I documenti in IRIS sono protetti da copyright e tutti i diritti sono riservati, salvo diversa indicazione.