The ≃ 100 kg highly radiopure NaI(Tl) set-up of the DAMA project (DAMA/NaI) has investigated the model- independent WIMP annual modulation signature over seven annual cycles for a total exposure of 107731 kg × day, obtaining a model-independent evidence for the presence of a dark matter particle component in the galactic halo at 6.3 σ C.L.. Some of the many possible corollary model-dependent quests for the candidate particle have been investigated with the total exposure as well. © 2004 Elsevier B.V. All rights reserved.
Further results on the WIMP annual modulation signature by DAMA/NaI / R., Bernabei; Cappella, Fabio; A., Incicchitti; Prosperi, Daniele. - In: NUCLEAR PHYSICS B-PROCEEDINGS SUPPLEMENTS. - ISSN 0920-5632. - 138:1-3(2005), pp. 45-47. [10.1016/j.nuclphysbps.2004.11.009]
Further results on the WIMP annual modulation signature by DAMA/NaI
CAPPELLA, fabio;PROSPERI, Daniele
2005
Abstract
The ≃ 100 kg highly radiopure NaI(Tl) set-up of the DAMA project (DAMA/NaI) has investigated the model- independent WIMP annual modulation signature over seven annual cycles for a total exposure of 107731 kg × day, obtaining a model-independent evidence for the presence of a dark matter particle component in the galactic halo at 6.3 σ C.L.. Some of the many possible corollary model-dependent quests for the candidate particle have been investigated with the total exposure as well. © 2004 Elsevier B.V. All rights reserved.I documenti in IRIS sono protetti da copyright e tutti i diritti sono riservati, salvo diversa indicazione.
