1. DAMA: an observatory for rare processes @LNGS
Roma2, Roma, LNGS, IHEP/Beijing
DAMA
DAMA: an observatory for rare
low bckg Ge
for sampling
meas.
LXe
R&D
NaI(Tl) LIBRA

2. DAMA/LXe experiment: results on rare processes
NIMA482(2002)728
Recent DARK MATTER investigations ...
Limits on recoils investigating the WIMP-129Xe elastic scattering by means of Pulse Shape Discrimination PLB436(1998)379
Limits on WIMP-129Xe inelastic scattering PLB387(1996)222, NJP2(2000)15.1
Neutron calibration PLB436(1998)379, EPJdirectC11(2001)1
129Xe vs 136Xe by using PSD  comparing SD vs SI signal to increase the sensitivity on the SD component data taking
... other rare processes
Nuclear level excitation of 129Xe during CNC processes PLB465(1999)315 .
Nucleon and di-nucleon decay into invisible channels
PLB493(2000)12
Electron decay e-  neg PRD61(2000)117301
2b decay in 134Xe PLB527(2002)182
Improved results on 2b in 134Xe and 136Xe PLB546(2002)23

3. DAMA/R&D set-up: results on rare processes
WIMPs:
WIMP search with CaF2(Eu) Astrop.Phys.7(1999)73
Other rare process:
2b decay in 136Ce and in 142Ce Il Nuov.Cim.A110(1997)189
2EC2n 40Ca decay using CaF2(Eu) scintillator Astrop.Phys.7(1999)73
2b decay in 46Ca and in 40Ca NPB563(1999)97
2b+ decay in 106Cd Astrop.Phys.10(1999)115
2b and b decay in 48Ca NPA705(2002)29
2EC2n in 136Ce and in 138Ce and a decay in 142Ce NIMA498(2003)352
The R&D shield closed
The R&D shield open
Fulfilling the inner Cu box

4. ~100 kg NaI(Tl) DAMA set-up: data taking completed on July 2002
Performances: N.Cim.A112(1999)545
Results on rare processes:
Possible Pauli exclusion principle violation PLB408(1997)439
Nuclear level excitation of 127I and 23Na during CNC processes PRC60(1999)065501
Electron stability and non-paulian transitions in Iodine atoms (by L-shell) PLB460(1999)235
Exotic Dark Matter search PRL83(1999)4918
Search for solar axions by Primakoff effect in NaI(Tl) crystals PLB515(2001)6
Exotic Matter search EPJdirect C14(2002)1
NaI(Tl) detectors
Results on WI MPS:
PSD: PLB389(1996)757
Investigation on diurnal effect: N.Cim.A112(1999)1541
Annual Modulation Signature: PLB424(1998)195, PLB450(1999)448, PRD61(1999)023512, PLB480(2000)23, PLB509(2001)197, EPJ C18(2000)283, EPJ C23 (2002)61, PRD66(2002)043503
Model independent evidence for WIMPs in galactic halo by annual modulation signature
57986 kgd
The several peculiar features of the signature satisfied; no systematics or side reactions able to mimic it (see e.g. EPJC18(2000)283)+ some of the many possible model frameworks investigated in the corollary quests for a candidate
other kg d (3 cycles) will be presented in few for a total exposure of: kgd

5. The new LIBRA set-up ~250 kg NaI(Tl)
(Large sodium Iodide Bulk for RAre processes)
in the DAMA experiment
running since March 2003
As a result of a new R&D for radiopurer NaI(Tl) by
exploiting new chemical/physical radiopurification techniques
(all operations involving crystals and PMTs - including photos - in HP Nitrogen atmosphere)
PMT
+HV
divider
storing new crystals
Improving installation
etching staff
at work
Installing LIBRA
detectors

6. DAMA/LIBRA (~250 kg NaI(Tl)) running and looking forward:
Summary
Successfully running ~100kg NaI(Tl), 6.5 kg LXe and R&D set-ups
over many years
Many rare processes investigated with all the set-ups
LXe alternatively running with 129Xe and 136Xe
R&D set-up running with small scale expts
100 kg NaI(Tl): 4 annual cycles released (~60000 kg day)
 Model independent analysis: presence of annual modulation with the proper
features; neither systematics nor side reactions able to mimic the signature
Model dependent analyses: pure SI coupling, pure SD, mixed SI/SD, WIMP with preferred inelastic scattering in some of the possible model frameworks + studies on the uncertainties of the parameters and on the assumptions + halo models + many other possibilities under study
New data to be presented on July 21, 2003
@LNGS (~ kg day) -- set-up out of operation on July 2002
From an improved R&D for radiopurity
DAMA/LIBRA (~250 kg NaI(Tl)) running and looking forward:
a new R&D for further radiopurifications started, toward 1 ton set-up we proposed in 1996