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1.
Measurement of the $^{235}$U(n,f) cross section relative to the $^{10}$B(n,α) reaction with Micromegas detectors at the CERN n_TOF facility: First results / n_TOF Collaboration
Neutron cross section measurements are often made relative to a neutron cross section standard. Thus, the accuracy of the neutron standards determines the best possible accuracy of the neutron measurements. [...]
2023 - 4 p. - Published in : EPJ Web Conf. 284 (2023) 01030 Fulltext: PDF;
In : 15th International Conference on Nuclear Data for Science and Technology, Online, 21 - 29 Jul 2022, pp.01030
2.
Measurement of $^{92,97,98,100}$Mo(n,$\gamma$) relevant to Astrophysics and Nuclear Technology / Busso, Maurizio (Istituto Nazionale di Fisica Nucleare, INFN and University of Perugia, Italy) ; Castelluccio, Donato Maurizio (Agenzia nazionale per le nuove tecnologie, l'energia e lo sviluppo economico sostenibile (ENEA), Italy) ; Console Camprini, Patrizio (Agenzia nazionale per le nuove tecnologie, l'energia e lo sviluppo economico sostenibile (ENEA), Italy) ; Colonna, Nicola (Istituto Nazionale di Fisica Nucleare, INFN, Italy) ; Cristallo, Sergio (Istituto Nazionale di Fisica Nucleare, INFN, and Istituto Nazionale di Astrofisica - Osservatorio Astronomico d'Abruzzo, Italy) ; Domingo-Pardo, Cesar (Instituto de Fìsica Corpuscular, CSIC - Universidad de Valencia, Spain) ; Guglielmell, Antonio (Agenzia nazionale per le nuove tecnologie, l'energia e lo sviluppo economico sostenibile (ENEA), and European Commission, Joint Research Centre (JRC), Ispra, Italy) ; Heyse, Jan (European Commission, Joint Research Centre (JRC), Geel, Belgium) ; Kopecky, Stefan (European Commission, Joint Research Centre (JRC), Geel, Belgium) ; Lederer-Woods, Claudia (School of Physics and Astronomy, University of Edinburgh, United Kingdom) et al.
CERN-INTC-2024-032 ; INTC-P-569-ADD-1.
- 2024.
Original Document (INTC-P-569) - Full text
3.
Measurement of the $^{14}$N(n,p)$^{14}$C cross section at the CERN n_TOF facility from sub-thermal energy to 800 keV / n_TOF Collaboration
Background: The $^{14}$N(n,p)$^{14}$C reaction is of interest in neutron capture therapy, where nitrogen-related dose is the main component due to low-energy neutrons, and in astrophysics, where 14N acts as a neutron poison in the s-process. Several discrepancies remain between the existing data obtained in partial energy ranges: thermal energy, keV region and resonance region. [...]
arXiv:2212.05128.- 2023-06-29 - 15 p. - Published in : Phys. Rev. C 107 (2023) 064617 Fulltext: 2212.05128 - PDF; Publication - PDF;
4.
$^{7}$ Be(n,p)$^{7}$ Li Cross Section Measurement for the Cosmological Lithium Problem at the n $\_$ TOF Facility at CERN / n_TOF Collaboration
One of the most puzzling problems in Nuclear Astrophysics is the “Cosmological Lithium Problem”, i.e the discrepancy between the primordial abundance of$^{7}$ Li observed in metal poor halo stars (Asplund et al. in Astrophys J 644:229–259, 2006, [1]), and the one predicted by Big Bang Nucleosynthesis (BBN). [...]
2019 - 8 p. - Published in : Springer Proc. Phys. 219 (2019) 25-32
In : Nuclei in the Cosmos XV (NIC XV), Assergi, Italy, 24 - 29 Jun 2018, pp.25-32
5.
Data for the s Process from n_TOF / n_TOF Collaboration
A considerable amount of (n, $\gamma $ ) reactions has been studied, so far, at the neutron time-of-flight facility n_TOF at CERN. The experimental program aims at determining and improving cross sections for a number of isotopes relevant to s-process nucleosynthesis. [...]
2019 - 8 p. - Published in : Springer Proc. Phys. 219 (2019) 63-70
In : Nuclei in the Cosmos XV (NIC XV), Assergi, Italy, 24 - 29 Jun 2018, pp.63-70
6.
First Results of the $^{140}$Ce(n,$\gamma$)$^{141}$Ce Cross-Section Measurement at n_TOF / n_TOF Collaboration
An accurate measurement of the $^{140}$Ce(n,$\gamma$) energy-dependent cross-section was performed at the n_TOF facility at CERN. This cross-section is of great importance because it represents a bottleneck for the s-process nucleosynthesis and determines to a large extent the cerium abundance in stars. [...]
2021 - 11 p. - Published in : Universe 7 (2021) 200 Fulltext: PDF;

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