Boeltzig, A.A.BoeltzigBruno, C. G.C. G.BrunoCavanna, F.F.CavannaCRISTALLO, SergioSergioCRISTALLODavinson, T.T.DavinsonDepalo, R.R.DepalodeBoer, R. J.R. J.deBoerDi Leva, A.A.Di LevaFerraro, F.F.FerraroImbriani, G.G.ImbrianiMarigo, P.P.MarigoTerrasi, F.F.TerrasiWiescher, M.M.Wiescher2020-05-122020-05-1220161434-6001http://hdl.handle.net/20.500.12386/24715The nucleosynthesis of light elements, from helium up to silicon, mainly occurs in Red Giant and Asymptotic Giant Branch stars and Novae. The relative abundances of the synthesized nuclides critically depend on the rates of the nuclear processes involved, often through non-trivial reaction chains, combined with complex mixing mechanisms. In this paper, we summarize the contributions made by LUNA experiments in furthering our understanding of nuclear reaction rates necessary for modeling nucleosynthesis in AGB stars and Novae explosions.STAMPAenArticle10.1140/epja/i2016-16075-42-s2.0-84964019073000373644500004https://link.springer.com/article/10.1140%2Fepja%2Fi2016-16075-42016EPJA...52...75BFIS/04 - FISICA NUCLEARE E SUBNUCLEAREERC sectors::Physical Sciences and Engineering::PE2 Fundamental constituents of matter: particle, nuclear, plasma, atomic, molecular, gas, and optical plasma