Issue |
EPJ Web Conf.
Volume 182, 2018
6th International Conference on New Frontiers in Physics (ICNFP 2017)
|
|
---|---|---|
Article Number | 02026 | |
Number of page(s) | 10 | |
Section | Talks | |
DOI | https://doi.org/10.1051/epjconf/201818202026 | |
Published online | 03 August 2018 |
https://doi.org/10.1051/epjconf/201818202026
Search for rare processes with DAMA experimental set-ups
1
National Research Centre “Kurchatov Institute”, Institute of Theoretical and Experimental Physics, 117218 Moscow, Russia
2
INFN, sez. Roma “Tor Vergata”, 00133 Rome, Italy
3
Dip. di Fisica, Università di Roma “Tor Vergata”, 00133 Rome, Italy
4
Institute for Nuclear Research, 03028 Kyiv, Ukraine
5
Joint Institute for Nuclear Research, 141980 Dubna, Russia
6
INFN, sez. Roma, 00185 Rome, Italy
7
Laboratori Nazionali del Gran Sasso, INFN, 67100 Assergi (AQ), Italy
8
Kavli Institute for the Physics and Mathematics of the Universe (WPI), University of Tokyo, Kashiwa, 277-8583, Japan
9
Key Laboratory of Particle Astrophysics, Institute of High Energy Physics, Chinese Academy of Sciences, P.O. Box 918/3, Beijing 100049, China
10
Dip. di Ingegneria Civile e Ingegneria Informatica, Università di Roma “Tor Vergata”, 00133 Rome, Italy
11
CSNSM, Univ. Paris-Sud, CNRS/IN2P3, Université Paris-Saclay, 91405 Orsay, France
12
Nikolaev Institute of Inorganic Chemistry, 630090 Novosibirsk, Russia
13
University of Jing Gangshan, Ji'an, Jiangxi, China
a e-mail: fabio.cappella@roma1.infn.it
Published online: 3 August 2018
Profiting of the favourable conditions offered by the Gran Sasso underground laboratory and of the several low-background DAMA set-ups, many and competitive results have been obtained for rare processes. Here the main results will be briefly resumed and some more details about the latest activities will be given. In particular, the searches on ββdecays of 106Cd and 116Cd and the perspectives of a complementary investigation on those Dark Matter (DM) candidates inducing just nuclear recoils, by exploiting the directionality approach with the anisotropic ZnWO4 scintillators, will be underlined.
© The Authors, published by EDP Sciences 2018
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