2013
DOI: 10.1140/epjc/s10052-013-2648-7
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Final model independent result of DAMA/LIBRA–phase1

Abstract: The results obtained with the total exposure of 1.04 ton × yr collected by DAMA/LIBRA-phase1 deep underground at the Gran Sasso National Laboratory (LNGS) of the I.N.F.N. during 7 annual cycles (i.e. adding a further 0.17 ton × yr exposure) are presented. The DAMA/LIBRAphase1 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, at 7.5σ C.L. Including also … Show more

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Cited by 515 publications
(624 citation statements)
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References 57 publications
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“…The DAMA/NaI [110][111][112] and DAMA/Libra [113][114][115] experiments have observed an annual modulation at 9.3 σ C.L. [116,117], as expected for a signal from dark particles. Different anomalies in other direct detection experiments, CoGeNT [118], CRESST-II [119] and recently CDMS-II (CDMS-Si) [120], may be reconciled with DAMA results.…”
Section: Wimps and Dark Mattermentioning
confidence: 88%
“…The DAMA/NaI [110][111][112] and DAMA/Libra [113][114][115] experiments have observed an annual modulation at 9.3 σ C.L. [116,117], as expected for a signal from dark particles. Different anomalies in other direct detection experiments, CoGeNT [118], CRESST-II [119] and recently CDMS-II (CDMS-Si) [120], may be reconciled with DAMA results.…”
Section: Wimps and Dark Mattermentioning
confidence: 88%
“…Nonphysical events such as electronic noise and tower vibrations, as well as particle interactions in the thermistors, follow an oblique distribution. The green solid line corresponds to the 90th percentile of the OT χ 2 distribution (OT χ 2 90% ) calculated in the region [35][36][37][38][39][40][41][42][43][44][45][46][47][48][49][50] keV and OT χ 2 < 10 using physics data. The magenta (orange) dashed line corresponds to the 90th (50th) percentile calculated using calibration data in the region [100-500] keV and OT χ 2 < 10, assuming linear dependence on energy.…”
Section: Dataset-bolometer Selection Criteriamentioning
confidence: 99%
“…For comparison, we also show the 5σ , 3σ and 90% C.L. regions resulting from a ML analysis reported in [31] on the DAMA/LIBRA annual modulation positive result [37,38] using the same parameters for the SHM. Thanks to the 741 kg of target mass of CUORE, we expect to achieve the sensitivity required to fully explore the parameter region implied by the DAMA/LIBRA posi-tive annual modulation signal with 5 years of data-taking.…”
Section: Wimp Sensitivity Of Cuorementioning
confidence: 99%
“…Some experiments report possible observations of dark matter scattering [27,28,29] while others exclude the mass and cross section regions where such signals would occur. In general, increasing sensitivity of direct searches tend to exclude weakly interacting dark matter with mass comparable to those of heavy nuclei most strongly, unless the reported scattering events are indeed due to the dark matter.…”
Section: General Statusmentioning
confidence: 99%