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.
|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|
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