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(n,cp) reactions study at the n_TOF facility at CERN: Results for the Cosmological Lithium problem

Authors :
Barbagallo, M.
Aberle, O.
Alcayne, V.
Andrzejewski, J.
Audouin, L.
Bécares, V.
Babiano-Suarez, V.
Bacak, M.
Benedikt, Th
Bennett, S.
Berthoumieux, E.
Billowes, J.
Bosnar, D.
Brown, A.
Busso, M.
Caamaño, M.
Caballero-Ontanaya, L.
Calviño, F.
Calviani, M.
Cano-Ott, D.
Casanovas, A.
Cerutti, F.
Chiaveri, E.
Colonna, N.
Cortés, G.
Cortés-Giraldo, M. A.
Cosentino, L.
Cristallo, S.
Damone, L. A.
Davies, P. J.
Dietz, M.
Domingo-Pardo, C.
Dressler, R.
Ducasse, Q.
Dupont, E.
Durán, I.
Eleme, Z.
Fernández-Domínguez, B.
Ferrari, A.
Finocchiaro, P.
Furman, V.
Göbel, K.
Gawlik, A.
Gilardoni, S.
Gonçalves, I. F.
González-Romero, E.
Guerrero, C.
Gunsing, F.
Heinitz, S.
Heyse, J.
Jenkins, D. G.
Junghans, A.
Käppeler, F.
Kadi, Y.
Kimura, A.
Knapova, I.
Kokkoris, M.
Kopatch, Y.
Krtička, M.
Kurtulgil, D.
Ladarescu, I.
Lederer-Woods, C.
Lonsdale, S. J.
Macina, D.
Manna, A.
Martínez, T.
Masi, A.
Massimi, C.
Mastinu, P.
Mastromarco, M.
Maugeri, E. A.
Mazzone, A.
Mendoza, E.
Mengoni, A.
Michalopoulou, V.
Milazzo, P. M.
Mingrone, F.
Moreno-Soto, J.
Musumarra, A.
Negret, A.
Ogállar, F.
Oprea, A.
Patronis, N.
Pavlik, A.
Perkowski, J.
Persanti, L.
Petrone, C.
Pirovano, E.
Ignacio Porras
Praena, J.
Quesada, J. M.
Ramos-Doval, D.
Rauscher, T.
Reifarth, R.
Rochman, D.
Sabaté-Gilarte, M.
Saxena, A.
Schillebeeckx, P.
Schumann, D.
Sekhar, A.
Smith, A. G.
Sosnin, N. V.
Sprung, P.
Stamatopoulos, A.
Tagliente, G.
Tain, J. L.
Tarifeño-Saldivia, A.
Tassan-Got, L.
Tsinganis, A.
Ulrich, J.
Urlass, S.
Valenta, S.
Vannini, G.
Variale, V.
Vaz, P.
Ventura, A.
Vescovi, D.
Vlachoudis, V.
Vlastou, R.
Wallner, A.
Woods, P. J.
Wright, T.
Žugec, P.
Institut de Physique Nucléaire d'Orsay (IPNO)
Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris-Sud - Paris 11 (UP11)
Institut de Recherches sur les lois Fondamentales de l'Univers (IRFU)
Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay
n_TOF
Université Paris-Sud - Paris 11 (UP11)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)
Source :
Scopus-Elsevier, CERN Proc., 15th International Conference on Nuclear Reaction Mechanisms, 15th International Conference on Nuclear Reaction Mechanisms, Jun 2018, Varenna, Italy. pp.259-264, INSPIRE-HEP, Diego Vescovi

Abstract

International audience; The Big Bang Nucleosynthesis describes the production of the lightest nuclides from deuterium to Li at the early stages of the Universe. While a general good agreement is found for most of the isotopes involved in the synthesis, a serious discrepancy between the predicted abundance of $^{7}$Li and the related experimental observations is still present. This discrepancy has been referred since several decades as Cosmological Lithium Problem. In one last attempt to find nuclear solutions to this longstanding conundrum, the $^{7}$Be(n,α)$^{4}$He and $^7}$Be(n,p)$^{7}$Li reactions, that affect predominantly the production of 7Li via the destruction of his parent nucleus 7Be, have been studied. Here we present the $^{7}$Be(n,α)$^{4}$He and $^{7}$Be(n,p)$^{7}$Li reaction cross- section measurements performed at the high-resolution n_TOF facility using the time-of-flight technique and high purity samples. The result of the experiments definitely rules out neutron induced reactions as a solution to the puzzle, thus indicating that explanations have to be sought out in other Physics scenarios.

Details

Database :
OpenAIRE
Journal :
Scopus-Elsevier, CERN Proc., 15th International Conference on Nuclear Reaction Mechanisms, 15th International Conference on Nuclear Reaction Mechanisms, Jun 2018, Varenna, Italy. pp.259-264, INSPIRE-HEP, Diego Vescovi
Accession number :
edsair.dedup.wf.001..16401780001f1fb746545cd955e19b42