Highlights on signals from Dark Matter particles
Dip. di Fisica, Università di Roma “Tor Vergata”, I-00133 Rome, Italy
2 INFN sez. Roma “Tor Vergata”, I-00133 Rome, Italy
3 Dip. di Fisica, Università di Roma “La Sapienza”, I-00185 Rome, Italy
4 INFN sez. Roma, I-00185 Rome, Italy
5 INFN, Laboratori Nazionali del Gran Sasso, I-67100 Assergi (AQ), Italy
6 Key Laboratory of Particle Astrophysics, IHEP, 100049 Beijing, P. R. China
a e-mail: email@example.com
Published online: 5 December 2017
Many experimental observations and theoretical arguments have pointed out that a large fraction of the Universe is composed by Dark Matter particles. Many possibilities are open on the nature and interaction types of such relic particles. In particular, this paper summarizes the main results obtained by exploiting the model independent Dark Matter annual modulation signature for the presence of Dark Matter particles in the galactic halo by DAMA experiment.
© The Authors, published by EDP Sciences, 2017
This is an Open Access article distributed under the terms of the Creative Commons Attribution License 4.0, which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited. (http://creativecommons.org/licenses/by/4.0/).