The DAMA/LIBRA{phase1 and the former DAMA/NaI data (cumulative exposure 1:33 ton yr, corresponding to 14 annual cycles) give evidence at 9.3 C.L. 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. Results and comparisons will be brie y recalled. Recent analyses on possible diurnal eects and on the Earth shadowing eect (the latter holds only for some DM candidates) will be mentioned. Finally, the perspectives of the running DAMA/LIBRA{phase2 will be mentioned.

Bernabei, R., Belli, P., D'Angelo, S., Di Marco, A., Montecchia, F., D'Angelo, A., et al. (2017). Recent results from DAMA/LIBRA-phase1 and perspectives. ASTRONOMICAL AND ASTROPHYSICAL TRANSACTIONS, 30(1), 71-80.

Recent results from DAMA/LIBRA-phase1 and perspectives

BERNABEI, RITA;D'ANGELO, SILIO;MONTECCHIA, FRANCESCO;Caracciolo V;
2017-01-01

Abstract

The DAMA/LIBRA{phase1 and the former DAMA/NaI data (cumulative exposure 1:33 ton yr, corresponding to 14 annual cycles) give evidence at 9.3 C.L. 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. Results and comparisons will be brie y recalled. Recent analyses on possible diurnal eects and on the Earth shadowing eect (the latter holds only for some DM candidates) will be mentioned. Finally, the perspectives of the running DAMA/LIBRA{phase2 will be mentioned.
2017
Pubblicato
Rilevanza internazionale
Articolo
Esperti anonimi
Settore FIS/04 - FISICA NUCLEARE E SUBNUCLEARE
English
Con Impact Factor ISI
scintillation detectors; elementary particle processes; Dark Matter
Bernabei, R., Belli, P., D'Angelo, S., Di Marco, A., Montecchia, F., D'Angelo, A., et al. (2017). Recent results from DAMA/LIBRA-phase1 and perspectives. ASTRONOMICAL AND ASTROPHYSICAL TRANSACTIONS, 30(1), 71-80.
Bernabei, R; Belli, P; D'Angelo, S; Di Marco, A; Montecchia, F; D'Angelo, A; Incicchitti, A; Cappella, F; Caracciolo, V; Cerulli, R; Dai, Cj; He, Hl; Kuang, Hh; Ma, Xh; Sheng, Xd; Wang, Rg; Ye, Zp
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Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/2108/257503
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