Imbriani, Gianluca (2007) Recent results and prospective of the LUNA experiment. [Rivista]

Full text not available from this repository.


I will describe the measurement of 14N(p,γ)15O done in the context of the LUNA experiment. The determination of the astrophysical S-factor of the 14N(p,γ)15O reaction is of great interest because this reaction represents the bottleneck of the CNO cycle, which in turn has a large influence on the determination of the age of globular clusters and also plays a role in the estimation of the solar neutrino fluxes. Moreover I discuss the prospective of the LUNA experiment.

Item Type: Rivista
Uncontrolled Keywords: Nuclear reactions, Nucleosynthesis, Abundances, Stars: evolution
Depositing User: ing Paolo Nicastro
Date Deposited: 20 Oct 2010 08:33
Last Modified: 30 Apr 2014 19:42

Actions (login required)

View Item View Item