Abstract
DAMA is searching for rare processes by developing and using several kinds of radiopure scintillators: in particular, NaI(Tl), liquid Xenon and CaF2(Eu). Here only the results released so far on the WIMP annual modulation signature are summarized and compared with results from other experiments, including the recent re-analysis of CDMS-I data. Next perspectives are also shortly addressed.
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Bernabei, R. et al. (2002). WIMP Search by the DAMA Experiment at Gran Sasso. In: Klapdor-Kleingrothaus, H.V., Viollier, R.D. (eds) Dark Matter in Astro- and Particle Physics. Springer, Berlin, Heidelberg. https://doi.org/10.1007/978-3-642-55739-2_42
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DOI: https://doi.org/10.1007/978-3-642-55739-2_42
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