Indirect study of the 3He(n, p)3H reaction at cosmological energies. (October 2020)

• Record Type: Journal Article
• Authors: Spampinato, C.; Pizzone, R.G.; Spart`a, R.; Couder, M.; Tan, W.; Burian, V.; Chae, K.Y.; D'Agata, G.; Guardo, G.L.; La Cognata, M.; Lamia, L.; Lattuada, D.; Mrazek, J.; Oliva, A.; Palmerini, S.; Prajapati, P.; Rapisarda, G.G.; Romano, S.; Sergi, M.L.; Spitaleri, C.; Tumino, A.; Wiescher, M.; Anguilar, S.; Bardayan, D.W.; Blankstein, D.; Boccioli, L.; Callahan, L.; Clark, A.; Frentz, B.; Hall, M.; Gula, A.; Henderson, S.; Kelmar, R.; Liu, Q.; Long, J.; Majumdar, A.; McGuinness, S.; Nelson, A.; O'Malley, P.D.; Seymour, C.; Skulski, M.; Wilkinson, J.;
• Is Part Of: Journal of physics. Volume 1668(2020)
• Publication Date: 2020-10
• Subjects: Physics -- Congresses; 530.5
• DOI: 10.1088/1742-6596/1668/1/012039
• Languages: English
• ISSNs: 1742-6588

Abstract

Abstract: In the network of reactions present in the Big Bang nucleosynthesis, the 3 He(n, p) 3 H reaction has an important role which impacts the final 7 Li abundance. The Trojan Horse Method (THM) has been applied to the 3 He(d, pt)H reaction in order to extract the astrophysical S(E)-factor of the 3 He(n, p) 3 H reaction in the Gamow energy range. The experiment will be described in the present work together with the first preliminary results.