Barbagallo M, Musumarra A, Cosentino L, Maugeri E, Heinitz S, Mengoni A, Dressler R, Schumann D, Käppeler F, Colonna N, Finocchiaro P, Ayranov M, Damone L, Kivel N, Aberle O, Altstadt S, Andrzejewski J, Audouin L, Bacak M, Balibrea-Correa J, Barros S, Bécares V, Bečvář F, Beinrucker C, Berthoumieux E, Billowes J, Bosnar D, Brugger M, Caamaño M, Calviani M, Calviño F, Cano-Ott D, Cardella R, Casanovas A, Castelluccio D M, Cerutti F, Chen Y H, Chiaveri E, Cortés G, Cortés-Giraldo M A, Cristallo S, Diakaki M, Domingo-Pardo C, Dupont E, Duran I, Fernandez-Dominguez B, Ferrari A, Ferreira P, Furman W, Ganesan S, García-Rios A, Gawlik A, Glodariu T, Göbel K, Gonçalves I F, González-Romero E, Griesmayer E, Guerrero C, Gunsing F, Harada H, Heftrich T, Heyse J, Jenkins D G, Jericha E, Katabuchi T, Kavrigin P, Kimura A, Kokkoris M, Krtička M, Leal-Cidoncha E, Lerendegui J, Lederer C, Leeb H, Lo Meo S, Lonsdale S J, Losito R, Macina D, Marganiec J, Martínez T, Massimi C, Mastinu P, Mastromarco M, Mazzone A, Mendoza E, Milazzo P M, Mingrone F, Mirea M, Montesano S, Nolte R, Oprea A, Pappalardo A, Patronis N, Pavlik A, Perkowski J, Piscopo M, Plompen A, Porras I, Praena J, Quesada J, Rajeev K, Rauscher T, Reifarth R, Riego-Perez A, Rout P, Rubbia C, Ryan J, Sabate-Gilarte M, Saxena A, Schillebeeckx P, Schmidt S, Sedyshev P, Smith A G, Stamatopoulos A, Tagliente G, Tain J L, Tarifeño-Saldivia A, Tassan-Got L, Tsinganis A, Valenta S, Vannini G, Variale V, Vaz P, Ventura A, Vlachoudis V, Vlastou R, Vollaire J, Wallner A, Warren S, Weigand M, Weiß C, Wolf C, Woods P J, Wright T, Žugec P
INFN, Sezione di Bari, Italy.
Dipartimento di Fisica e Astronomia DFA, Università di Catania, Italy.
Phys Rev Lett. 2016 Oct 7;117(15):152701. doi: 10.1103/PhysRevLett.117.152701. Epub 2016 Oct 3.
The energy-dependent cross section of the ^{7}Be(n,α)^{4}He reaction, of interest for the so-called cosmological lithium problem in big bang nucleosynthesis, has been measured for the first time from 10 meV to 10 keV neutron energy. The challenges posed by the short half-life of ^{7}Be and by the low reaction cross section have been overcome at n_TOF thanks to an unprecedented combination of the extremely high luminosity and good resolution of the neutron beam in the new experimental area (EAR2) of the n_TOF facility at CERN, the availability of a sufficient amount of chemically pure ^{7}Be, and a specifically designed experimental setup. Coincidences between the two alpha particles have been recorded in two Si-^{7}Be-Si arrays placed directly in the neutron beam. The present results are consistent, at thermal neutron energy, with the only previous measurement performed in the 1960s at a nuclear reactor. The energy dependence reported here clearly indicates the inadequacy of the cross section estimates currently used in BBN calculations. Although new measurements at higher neutron energy may still be needed, the n_TOF results hint at a minor role of this reaction in BBN, leaving the long-standing cosmological lithium problem unsolved.
对于大爆炸核合成中所谓的宇宙锂问题具有重要意义的(^{7}Be(n,\alpha)^{4}He)反应的能量依赖截面,首次在10毫电子伏特至10千电子伏特的中子能量范围内进行了测量。由于欧洲核子研究组织(CERN)的n_TOF设施新实验区(EAR2)中前所未有的极高中子束亮度与良好分辨率的组合、足量化学纯(^{7}Be)的可得性以及专门设计的实验装置,(^{7}Be)的短半衰期和低反应截面所带来的挑战在n_TOF得以克服。两个α粒子之间的符合事件在直接置于中子束中的两个Si - (^{7}Be) - Si阵列中被记录下来。目前的结果在热中子能量下与20世纪60年代在核反应堆上进行的唯一一次先前测量结果一致。这里报道的能量依赖性清楚地表明了目前在大爆炸核合成(BBN)计算中使用的截面估计的不足。尽管可能仍需要在更高中子能量下进行新的测量,但n_TOF的结果暗示了该反应在大爆炸核合成中作用较小,使得长期存在的宇宙锂问题仍未解决。