The Dark Matter annual modulation results from DAMA/LIBRA

The DAMA/LIBRA experiment, running at the Gran Sasso National Laboratory of the I.N.F.N. in Italy, has a sensitive mass of about 250 kg highly radiopure NaI(Tl). It is mainly devoted to the investigation of Dark Matter (DM) particles in the Galactic halo by exploiting the model independent DM annual...

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Main Authors: Bernabei R., Belli P., Cappella F., Caracciolo V., Cerulli R., Dai C.J., d’Angelo A., Di Marco A., He H.L., Incicchitti A., Ma X.H., Montecchia F., Sheng X.D., Wang R.G., Ye Z.P.
Format: Article
Language:English
Published: EDP Sciences 2014-04-01
Series:EPJ Web of Conferences
Online Access:http://dx.doi.org/10.1051/epjconf/20147000043
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author Bernabei R.
Belli P.
Cappella F.
Caracciolo V.
Cerulli R.
Dai C.J.
d’Angelo A.
Di Marco A.
He H.L.
Incicchitti A.
Ma X.H.
Montecchia F.
Sheng X.D.
Wang R.G.
Ye Z.P.
author_facet Bernabei R.
Belli P.
Cappella F.
Caracciolo V.
Cerulli R.
Dai C.J.
d’Angelo A.
Di Marco A.
He H.L.
Incicchitti A.
Ma X.H.
Montecchia F.
Sheng X.D.
Wang R.G.
Ye Z.P.
author_sort Bernabei R.
collection DOAJ
description The DAMA/LIBRA experiment, running at the Gran Sasso National Laboratory of the I.N.F.N. in Italy, has a sensitive mass of about 250 kg highly radiopure NaI(Tl). It is mainly devoted to the investigation of Dark Matter (DM) particles in the Galactic halo by exploiting the model independent DM annual modulation signature. The present DAMA/LIBRA experiment and the former DAMA/NaI one (the first generation experiment having an exposed mass of about 100 kg) have released so far results corresponding to a total exposure of 1.17 ton × yr over 13 annual cycles. They provide a model independent evidence of the presence of DM particles in the galactic halo at 8.9 σ C.L. on the basis of the investigated DM signature. The data of another annual cycle in the same DAMA/LIBRA running conditions are at hand. After the replacement at the end of 2012 of all the photomultipliers (PMTs) with new ones, having higher quantum efficiency, DAMA/LIBRA has entered to its phase 2; such a replacements allowed the lowering of the software energy threshold of the experiment in the present data taking. A short summary of the obtained results is presented and future perspectives of the experiment mentioned.
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spelling doaj.art-75c1e51647c345f8979a3d8a1ca90f712022-12-21T17:24:03ZengEDP SciencesEPJ Web of Conferences2100-014X2014-04-01700004310.1051/epjconf/20147000043epjconf_icfp2012_00043The Dark Matter annual modulation results from DAMA/LIBRABernabei R.Belli P.0Cappella F.Caracciolo V.1Cerulli R.2Dai C.J.3d’Angelo A.Di Marco A.He H.L.4Incicchitti A.5Ma X.H.6Montecchia F.Sheng X.D.7Wang R.G.8Ye Z.P.INFN, sez. Roma “Tor Vergata”Laboratori Nazionali del Gran Sasso, I.N.F.N.Laboratori Nazionali del Gran Sasso, I.N.F.N.IHEP, Chinese AcademyIHEP, Chinese AcademyINFN, sez. RomaIHEP, Chinese AcademyIHEP, Chinese AcademyIHEP, Chinese AcademyThe DAMA/LIBRA experiment, running at the Gran Sasso National Laboratory of the I.N.F.N. in Italy, has a sensitive mass of about 250 kg highly radiopure NaI(Tl). It is mainly devoted to the investigation of Dark Matter (DM) particles in the Galactic halo by exploiting the model independent DM annual modulation signature. The present DAMA/LIBRA experiment and the former DAMA/NaI one (the first generation experiment having an exposed mass of about 100 kg) have released so far results corresponding to a total exposure of 1.17 ton × yr over 13 annual cycles. They provide a model independent evidence of the presence of DM particles in the galactic halo at 8.9 σ C.L. on the basis of the investigated DM signature. The data of another annual cycle in the same DAMA/LIBRA running conditions are at hand. After the replacement at the end of 2012 of all the photomultipliers (PMTs) with new ones, having higher quantum efficiency, DAMA/LIBRA has entered to its phase 2; such a replacements allowed the lowering of the software energy threshold of the experiment in the present data taking. A short summary of the obtained results is presented and future perspectives of the experiment mentioned.http://dx.doi.org/10.1051/epjconf/20147000043
spellingShingle Bernabei R.
Belli P.
Cappella F.
Caracciolo V.
Cerulli R.
Dai C.J.
d’Angelo A.
Di Marco A.
He H.L.
Incicchitti A.
Ma X.H.
Montecchia F.
Sheng X.D.
Wang R.G.
Ye Z.P.
The Dark Matter annual modulation results from DAMA/LIBRA
EPJ Web of Conferences
title The Dark Matter annual modulation results from DAMA/LIBRA
title_full The Dark Matter annual modulation results from DAMA/LIBRA
title_fullStr The Dark Matter annual modulation results from DAMA/LIBRA
title_full_unstemmed The Dark Matter annual modulation results from DAMA/LIBRA
title_short The Dark Matter annual modulation results from DAMA/LIBRA
title_sort dark matter annual modulation results from dama libra
url http://dx.doi.org/10.1051/epjconf/20147000043
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