The LUNA experiment: studying stars by going underground
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Alessandra Guglielmetti(Universita' degli Studi di Milano and INFN)
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Europe/Paris
Amphithéâtre (CPPM)
Amphithéâtre
CPPM
Description
Cross sections of nuclear reactions powering stars are essential
ingredients for element nucleosynthesis, energy generation and neutrino
fluxes in stellar environments. The low value of such cross sections at
astrophysically relevant energies prevents their measurement in a
laboratory at the Earth's surface due to the unfavorable signal-to-noise
ratio. The LUNA collaboration installed two accelerators in the
Underground Gran Sasso National Laboratory in Italy where the cosmic
background is very much reduced and measured a few key reactions of the
Hydrogen burning and Big Bang nucleosynthesis. After a general
introduction on nuclear astrophysics, the most relevant results achieved
by LUNA will be reviewed and the future possibilities such as the LUNA MV
project described