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000408355 020__ $$a978-3-935702-83-6
000408355 0247_ $$2datacite_doi$$a10.3204/DESY-PROC-2013-04/cerulli_riccardo
000408355 0247_ $$2ISSN$$a1435-8077
000408355 037__ $$aPUBDB-2018-02808
000408355 041__ $$aEnglish
000408355 0881_ $$aDESY-PROC-2013-04
000408355 088__ $$2DESY$$aDESY-PROC-2013-04
000408355 1001_ $$0P:(DE-HGF)0$$aBernabei, R.$$b0
000408355 1112_ $$0C13-06-24.5$$2inspire$$a9th Patras Workshop on Axions, WIMPs and WISPs$$cMainz$$d2013-06-24 - 2013-06-28$$gAXION-WIMP 2013$$wGermany
000408355 245__ $$aResults from DAMA/LIBRA and perspectives
000408355 260__ $$aHamburg$$bVerlag Deutsches Elektronen-Synchrotron$$c2013
000408355 29510 $$aBernabei, R. "Results from DAMA/LIBRA and perspectives" in Proceedings, 9th Patras Workshop on Axions, WIMPs and WISPs (AXION-WIMP 2013) / Oberlack, Uwe, Sissol, Pierre (eds.), 2013 ; AXION-WIMP 2013 : 9th Patras Workshop on Axions, WIMPs and WISPs , 2013-06-23 - 2013-06-28, Mainz
000408355 300__ $$a179-183
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000408355 4900_ $$0PERI:(DE-600)2450075-6$$aDESY-PROC
000408355 520__ $$aThe DAMA/LIBRA experiment (about 250 kg of highly radiopure NaI(Tl)) is in operation at the Gran Sasso National Laboratory of the INFN. The main aim of the experiment is to further investigate the Dark Matter (DM) particles in the Galactic halo by exploiting the model independent DM annual modulation signature. At the time of this Workshop, the DAMA/LIBRA experiment and the former DAMA/NaI one (the first generation experiment having an exposed mass of about 100 kg) have released results corresponding to a total exposure of 1.17 ton × yr over 13 annual cycles; they have provided a model independent evidence of the presence of DM particles in the galactic halo at 8.9 $σ$ C.L.. The results of a further annual cycle, concluding the DAMA/LIBRA–phase1, have been released after this Workshop and are not included here. After the upgrade at fall 2010 when all the PMTs have been replaced with new ones having higher quantum efficiency, the feasibility to decrease the software energy threshold has been demonstrated and the setup is running in this new configuration, named DAMA/LIBRA–phase2. 
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000408355 7001_ $$0P:(DE-HGF)0$$aBelli, P.$$b1
000408355 7001_ $$0P:(DE-HGF)0$$aCappella, F.$$b2
000408355 7001_ $$0P:(DE-HGF)0$$aCaracciolo, V.$$b3
000408355 7001_ $$0P:(DE-HGF)0$$aCastellano, S.$$b4
000408355 7001_ $$0P:(DE-HGF)0$$aCerulli, R.$$b5$$eCorresponding author
000408355 7001_ $$0P:(DE-HGF)0$$aDai, C. J.$$b6
000408355 7001_ $$0P:(DE-HGF)0$$ad’Angelo, A.$$b7
000408355 7001_ $$0P:(DE-HGF)0$$ad’Angelo, S.$$b8
000408355 7001_ $$0P:(DE-HGF)0$$aDi Marco, A.$$b9
000408355 7001_ $$0P:(DE-HGF)0$$aHe, H. L.$$b10
000408355 7001_ $$0P:(DE-HGF)0$$aIncicchitti, A.$$b11
000408355 7001_ $$0P:(DE-HGF)0$$aMa, X. H.$$b12
000408355 7001_ $$0P:(DE-HGF)0$$aMontecchia, F.$$b13
000408355 7001_ $$0P:(DE-HGF)0$$aSheng, X. D.$$b14
000408355 7001_ $$0P:(DE-HGF)0$$aWang, R. G.$$b15
000408355 7001_ $$0P:(DE-HGF)0$$aYe, Z. P.$$b16
000408355 7870_ $$0PUBDB-2015-05816$$aOberlack, Uwe et. al.$$iisPartOf$$rDESY-PROC-2013-04$$tProceedings, 9th Patras Workshop on Axions, WIMPs and WISPs (AXION-WIMP 2013)
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