We analyzed the effects of the new assumptions on standard solar models (SSMs) and compared the results obtained by adopting the revised 7Be+e − rate to those obtained by that reported in a widely used compilation of reaction rates (ADE11). In the framework of fundamental solar physics, we consider a recent evaluation for the 7Be+e − rate, which has not been used up to now, in the estimate of neutrino fluxes. In recent decades several estimates were presented, pointing out that the theoretical uncertainty in the rate is in general of a few percent.Īims. Theoretical evaluations have to account for not only the nuclear interaction, but also the processes in the plasma in which 7Be ions and electrons interact. Electron-capture on 7Be is the main production channel for 7Li in several astrophysical environments. Acitelli, 22, Assergi, L’Aquila, Italyĭivision of physics School of Science and Technology Università di Camerino, Italyįaculty of Mathematics and Physics, Charles University, Prague, Czech RepublicĮuropean Centre for Theoretical Studies in Nuclear Physics and Related Areas (ECT*-FBK) and Trento Institute for Fundamental Physics and Applications (TIFPA-INFN), Trento, ItalyĬontext. INFN, Laboratori Nazionali del Gran Sasso, Via G. University of Perugia, Department of Physics and Geology, Via A. INAF, Observatory of Abruzzo, Via Mentore Maggini snc, 64100 Teramo, Italy Gran Sasso Science Institute, Viale Francesco Crispi, 7, 67100 L’Aquila, ItalyĮ-mail: Section of Perugia, Via A. Astronomical objects: linking to databasesĭ.Including author names using non-Roman alphabets. Suggested resources for more tips on language editing in the sciences Punctuation and style concerns regarding equations, figures, tables, and footnotes
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