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Multi-section fission ionization chamber for measurement of 239Pu(n,γ) reaction in fission tagging method

Nuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment, ISSN: 0168-9002, Vol: 1067, Page: 169649
2024
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Article Description

The 239Pu(n,γ) reaction cross section is very important for operation of both thermal and fast reactors, when loaded with MOX fuels. According to the NEA/OECD High Priority Request List the precision of cross section data for this reaction should be improved. The cross section of (n,f) reaction is much higher compared to (n,γ) for this isotope. In such conditions the fission tagging technique could be applied to identify the fission background. In the past, this technique was successfully used for capture measurements at the n_TOF facility at CERN. The multi-section fission ionization chamber was constructed and used in the combination with Total Absorption Calorimeter (TAC) for detecting gamma rays for the precise measurement of 239Pu(n,γ) reaction cross section at the n_TOF facility.

Bibliographic Details

J. Perkowski; J. Andrzejewski; A. Gawlik-Ramięga; V. Alcayne; D. Cano-Ott; E. Mendoza; A. Sánchez-Caballero; E. González-Romero; T. Martínez; A. Pérez de Rada Fiol; J. Plaza del Olmo; G. Sibbens; D. Vanleeuw; J. Heyse; P. Schillebeeckx; O. Aberle; M. Bacak; A. P. Bernardes; M. Calviani; F. Cerutti; E. Chiaveri; M. Di Castro; S. Fargier; F. García-Infantes; S. Gilardoni; Y. Kadi; G. Lerner; A. Masi; N. Patronis; J. A. Pavón-Rodríguez; C. Rubbia; M. Sabaté-Gilarte; M. E. Stamati; V. Vlachoudis; S. Altieri; C. Beltrami; S. Amaducci; L. Cosentino; P. Finocchiaro; G. Vecchio; V. Babiano-Suarez; J. Balibrea Correa; C. Domingo-Pardo; I. Ladarescu; J. Lerendegui-Marco; S. Bennett; W. Hillman; A. Sekhar; A. G. Smith; T. Wright; E. Berthoumieux; E. Dupont; F. Gunsing; G. Kaur; R. Beyer; A. Junghans; A. Wallner; M. Boromiza; A. Negret; C. Petrone; D. Bosnar; P. Žugec; M. Caamaño; I. Durán; B. Fernández-Domínguez; F. Calviño; A. Casanovas; G. Cortés; A. Tarifeño-Saldivia; D. M. Castelluccio; P. Console Camprini; S. Fiore; A. Mengoni; A. Manna; C. Massimi; R. Zarrella; G. Cescutti; P. M. Milazzo; S. Chasapoglou; M. Diakaki; K. Kaperoni; M. Kokkoris; N. Kyritsis; V. Michalopoulou; R. Vlastou; P. Colombetti; G. Gervino; A. Sturniolo; N. Colonna; M. Mastromarco; A. Mazzone; G. Tagliente; V. Variale; M. A. Cortés-Giraldo; B. Fernández; C. Guerrero; P. Pérez-Maroto; J. M. Quesada; S. Cristallo; R. Mucciola; S. Dellmann; R. Reifarth; D. Vescovi; S. Di Maria; Y. Romanets; P. Vaz; M. Dietz; E. Pirovano; R. Dressler; E. A. Maugeri; D. Rochman; D. Schumann; Z. Eleme; E. Vagena; C. Gustavino; V. Furman; Y. Kopatch; I. Porras; J. Praena; P. Torres-Sánchez; D. G. Jenkins; E. Jericha; A. Kimura; I. Knapová; M. Krtička; S. Valenta; C. Lederer-Woods; N. V. Sosnin; P. J. Woods; P. Mastinu; E. Musacchio-Gonzalez; F. Murtas; A. Musumarra; M. G. Pellegriti; S. Pomp; D. Tarrío

Elsevier BV

Physics and Astronomy

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