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.
Recent results and prospective of the LUNA experiment / Imbriani, Gianluca. - In: PROGRESS IN PARTICLE AND NUCLEAR PHYSICS. - ISSN 0146-6410. - STAMPA. - 59:1(2007), pp. 193-195. [10.1016/j.ppnp.2006.12.006]
Recent results and prospective of the LUNA experiment
IMBRIANI, GIANLUCA
2007
Abstract
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.I documenti in IRIS sono protetti da copyright e tutti i diritti sono riservati, salvo diversa indicazione.
