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

M. Barbagallo , O. Aberle , V. Alcayne , J. Andrzejewski , L. Audouin (1) , V. Bécares , V. Babiano-Suarez , M. Bacak (2) , Th. Benedikt , S. Bennett , E. Berthoumieux (2) , J. Billowes , D. Bosnar , A. Brown , M. Busso , M. Caamaño , L. Caballero-Ontanaya , F. Calviño , M. Calviani , D. Cano-Ott , A. Casanovas , F. Cerutti , E. Chiaveri , N. Colonna , G. Cortes , M.A. Cortés-Giraldo , L. Consentino , S. Cristallo , L.A. Damone , P.J. Davies , M. Dietz , C. Domingo-Pardo , R. Dressler , Q. Ducasse , E. Dupont (2) , I. Duran , Z. Eleme , B. Fernández-Domínguez , A. Ferrari , P. Finocchiaro , V. Furman , K. Göbel , A. Gawlik , S. Gilardoni , I.F. Gonçalves , E. González-Romero , C. Guerrero , F. Gunsing (2) , S. Heinitz , J. Heyse , D.G. Jenkins , A. Junghans , F. Käppeler , Y. Kadi , A. Kimura , I. Knapova , M. Kokkoris , Y. Kopatch , M. Krtička , D. Kurtulgil , I. Ladarescu , C. Lederer-Woods , S.J. Lonsdale , D. Macina , A. Manna , T. Martínez , A. Masi , C. Massimi , P. Mastinu , M. Mastromarco , E.A. Maugeri , A. Mazzone , E. Mendoza , A. Mengoni , V. Michalopoulou , P.M. Milazzo , F. Mingrone , J. Moreno-Soto (2) , A. Musumarra , A. Negret , F. Ogállar , A. Oprea , N. Patronis , A. Pavlik , J. Perkowski , L. Persanti , C. Petrone , E. Pirovano , I. Porras , J. Praena , J.M. Quesada , D. Ramos-Doval (1) , T. Rauscher , R. Reifarth , D. Rochman , M. Sabaté-Gilarte , A. Saxena , P. Shillebeeckx , D. Schumann , A. Sekhar , A.G. Smith , N.V. Sosnin , P. Sprung , A. Stamatopoulos , G. Tagliente , J.L. Tain , A. Tarifeño-Saldivia , L. Tassan-Got (1) , A. Tsinganis , J. Ulrich , S. Urlass , S. Valenta , G. Vannini , V. Variale , P. Vaz , A. Ventura , D. Vescovi , V. Vlachoudis , R. Vlastou , a . Wallner , P.J. Woods , T. Wright , P. Žugec

1 IPNO - Institut de Physique Nucléaire d'Orsay
2 IRFU - Institut de Recherches sur les lois Fondamentales de l'Univers

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.

Domaines: Physique Nucléaire Expérimentale [nucl-ex]

M. Barbagallo, O. Aberle, V. Alcayne, J. Andrzejewski, L. Audouin, et al.. (n,cp) reactions study at the n_TOF facility at CERN: results for the Cosmological Lithium problem. 15th International Conference on Nuclear Reaction Mechanisms, Jun 2018, Varenna, Italy. pp.259-264. ⟨hal-02097272⟩