MOON (Mo Observatory Of Neutrinos) for neutrino studies in 100Mo by double beta decays and solar-ν capture reactions

Details MOON (Mo Observatory Of Neutrinos) for neutrino studies in 100Mo by double beta decays and solar-ν capture reactions MOON (Mo Observatory Of Neutrinos) for neutrino studies in 100Mo by double beta decays and solar-ν capture reactions

Apr 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002aipc..610..959h&link_type=abstract

NUCLEAR PHYSICS IN THE 21st CENTURY:International Nuclear Physics Conference INPC 2001. AIP Conference Proceedings, Volume 610,

Physics

Nuclear Physics

Neutrino Mass And Mixing, Solar Neutrinos, Weak-Interaction And Lepton Aspects

Scientific paper

Neutrino mass is a key issue of current physics, and atmospheric, solar, and accelerator experiments strongly suggest ν oscillations due to non-zero ν-mass differences and flavor mixings. It is of great interest to study ν mass with sensitivity in the 0.05 eV range. Double beta decay may be the only probe presently able to access such small ν masses. It is possible with 100Mo to carry out both spectroscopic studies of double beta decays with the sensitivity of the order of ~0.03 eV, and realtime exclusive studies of low energy solar ν. .

Affiliated with

Also associated with

No associations

Rating

MOON (Mo Observatory Of Neutrinos) for neutrino studies in 100Mo by double beta decays and solar-ν capture reactions does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with MOON (Mo Observatory Of Neutrinos) for neutrino studies in 100Mo by double beta decays and solar-ν capture reactions, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and MOON (Mo Observatory Of Neutrinos) for neutrino studies in 100Mo by double beta decays and solar-ν capture reactions will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1533643