Constraints on the dipole photon strength for the odd uranium isotopes

Moreno-Soto, J.; Valenta, S.; Berthoumieux, E.; Chebboubi, A.; Diakaki, Μ.; Dridi, W.; Dupont, E.; Gunsing, F.; Krtička, M.; Litaize, O.; Sérot, O.; Aberle, O.; Alcayne, V.; Amaducci, S.; Andrzejewski, J.; Audouin, L.; Bécares, V.; Babiano-Suárez, V.; Bacak, M.; Barbagallo, M.; Benedikt, Th.; Bennett, S.; Billowes, J.; Bosnar, D.; Brown, A.; Busso, M.; Caamaño, M.; Caballero, 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.; Dietz, M.; Domingo‐Pardo, C.; Dressler, R.; Ducasse, Q.; Durán, I.; Eleme, Z.; Fernández–Domínguez, B.; Ferrari, A.; Finocchiaro, P.; Furman, V.; Göbel, K.; Gawlik-Ramięga, A.; Gilardoni, S.; Gonçalves, I. F.; González‐Romero, E.; Guerrero, C.; Heinitz, S.; Heyse, J.; Jenkins, D. G.; Junghans, A. R.; Käppeler, F.; Kadi, Y.; Kimura, Akira; Knapová, I.; Kokkoris, M.; Kopatch, Y.; Kurtulgil, D.; Ladarescu, I.; Lampoudis, C.; 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, Paolo; Mingrone, F.; Musumarra, A.; Negret, A.; Nolte, R.; Ogállar, F.; Oprea, A.; Patronis, N.; Pavlik, A.; Perkowski, J.; Piersanti, L.; Petrone, C.; Pirovano, E.; Porras, I.; Praena, J.; Quesada, J. M.; Ramos, 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.; Taín, J. L.; Tarifeño-Saldivia, A.; Tassan‐Got, L.; Torres-Sánchez, P.; Tsinganis, A.; Ulrich, J.; Urlaß, S.; Vannini, G.; Variale, V.; Vaz, P.; Ventura, A.; Vescovi, D.; Vlachoudis, V.; Vlastou, R.; Wallner, A.; Woods, P. J.; Wright, T.; Žugec, P.

doi:10.1103/physrevc.105.024618

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2023

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“…References quoted represent examples, where such correction factors were crucial to keep the systematic uncertainty within the level of 2-3% RMS. Finally, this result also highlights the relevance of suitable computing codes and libraries [49], methods and models [50,51,52,53] for simulating the cascade of prompt γ-rays in neutroncapture experiments.…”

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confidence: 79%

Advances and new ideas for neutron-capture astrophysics experiments at CERN n_TOF

et al. 2023

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This article presents a few selected developments and future ideas related to the measurement of $$(n,\gamma )$$ ( n , γ ) data of astrophysical interest at CERN n_TOF. The MC-aided analysis methodology for the use of low-efficiency radiation detectors in time-of-flight neutron-capture measurements is discussed, with particular emphasis on the systematic accuracy. Several recent instrumental advances are also presented, such as the development of total-energy detectors with $$\gamma $$ γ -ray imaging capability for background suppression, and the development of an array of small-volume organic scintillators aimed at exploiting the high instantaneous neutron-flux of EAR2. Finally, astrophysics prospects related to the intermediate i neutron-capture process of nucleosynthesis are discussed in the context of the new NEAR activation area.

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