MOON for double beta decays and X-rays from WIMP nuclear interactions

Details MOON for double beta decays and X-rays from WIMP nuclear interactions MOON for double beta decays and X-rays from WIMP nuclear interactions

Jul 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006prpnp..57..153e&link_type=abstract

Progress in Particle and Nuclear Physics, Volume 57, Issue 1, p. 153-161.

Physics

Nuclear Physics

6

Scientific paper

Neutrino-less double beta decays (0νββ) and direct observation of cold dark matter (DM) are of great interest for studying fundamental properties of neutrinos and weakly interacting massive particles (WIMPs). These are crucial for particle physics and cosmology beyond the standard electro-weak theory. The present seminar in the Erice neutrino school reports briefly (1) the effective neutrino mass studied by 0νββ, (2) the unique features and the present status of MOON (Molybdenum Observatory Of Neutrinos) for high-sensitivity 0νββ studies with 100Mo in the quasi-degenerate and inverted hierarchy regions, and (3) the direct detection of WIMPs by measuring atomic X-rays following inner-shell ionization by WIMPs nuclear interactions. The MOON project is carried out in collaboration with the MOON collaboration, and the X-ray work from WIMPs is done with Ch.C. Moustakidis and J.D. Vergados.

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