Author:
Buompane Raffaele,Di Leva Antonino,Gialanella Lucio,D’Onofrio Antonio,De Cesare Mario,Jeremias G. Duarte,Fülöp Zsolt,Leandro R. Gasques,Gyürky György,Morales-Gallegos Lizeth,Marzaioli Fabio,Palumbo Giancarlo,Porzio Giuseppe,Rapagnani David,Roca Vincenzo,Rogalla Detlef,Romoli Mauro,Santonastaso Claudio,Schürmann Daniel
Abstract
The cross section of 7Be(p,γ)8B represents one of the most important nuclear inputs for the prediction of the high energy component of solar neutrinos and it has also a direct impact on the 7Li abundance after the Big Bang Nucleosynthesis. The importance of this reaction triggered an intense experimental work over the last decades, where discrepancies were observed between the results of different measurements. In addition, a question remains about possible common systematic effects, considering that all measurements share the same experimental approach, i.e. an intense proton beam impinging on a 7Be radioactive target. Inverse kinematics, i.e. a 7Be ion beam and a hydrogen target, with the direct measurement of the total reaction cross section by means of the detection of the 8B recoils, can shed light on such systematic effects. Efforts attempted so far were limited by the low 7Be beam intensity. We present here the results of a new measurement at Ecm = 376 to 819 keV using a high intensity 7Be beam in combination with a windowless gas target and the recoil mass separator ERNA (European Recoil mass separator for Nuclear Astrophysics) at CIRCE (Center for Isotopic Research on Cultural and Environmental heritage), Caserta, Italy. Our results, including the systematic error, are compatible with previous measurements that yields lower value of S17(0) and are compatible with the currently accepted value from [1] only at a 2-σ level.