Measurements of the 33S (n, α)30Si cross-section at n_TOF and ILL: Implications in neutron capture therapy

Up to a couple of years ago, the 33S(n, α)30Si cross-section data had been limited and scarce. The origin in the solar system of 36S had been the only motivation to study that cross-section. However, a few years ago, the 33S(n, α)30Si reaction was proposed as a possible target in neutron capture the...

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Main Authors: Praena Javier, L Isabelópez-Casas, Sabat Mariaé-Gilarte, Arias Fernando de Saavedra, Porras Ignacio
Format: Article
Language:English
Published: EDP Sciences 2020-01-01
Series:EPJ Web of Conferences
Online Access:https://www.epj-conferences.org/articles/epjconf/pdf/2020/15/epjconf_nd2019_01020.pdf
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spelling doaj-1d598d148c5448238d89a1d2626cbedd2021-08-02T19:21:52ZengEDP SciencesEPJ Web of Conferences2100-014X2020-01-012390102010.1051/epjconf/202023901020epjconf_nd2019_01020Measurements of the 33S (n, α)30Si cross-section at n_TOF and ILL: Implications in neutron capture therapyPraena Javier0L Isabelópez-Casas1Sabat Mariaé-GilarteArias Fernando de Saavedra2Porras Ignacio3Universidad de GranadaUniversidad de GranadaUniversidad de GranadaUniversidad de GranadaUp to a couple of years ago, the 33S(n, α)30Si cross-section data had been limited and scarce. The origin in the solar system of 36S had been the only motivation to study that cross-section. However, a few years ago, the 33S(n, α)30Si reaction was proposed as a possible target in neutron capture therapy (NCT) due to the excellent bio-properties of 33S and the significant resonance at 13.45 keV of the cross-section for which a high-energy α is emitted. Prior to the experiments carried out at n_TOF-CERN and at the Institut Laue-Langevin (ILL) facilities, the data situation was: no data from the thermal point up to 10 keV; from 10 keV to 300 keV, there was only one (n, α) measurement able to resolve the resonances with a questionable value of the 13.45-keV resonance; and the thermal point did not have a consistent value. Here we summarize three experiments that have been performed covering the whole energy range of interest in NCT and astrophysics. These experiments have solved the most important issues. The data of the present work and the evaluated data are used to calculate the dose rate in the tissue.https://www.epj-conferences.org/articles/epjconf/pdf/2020/15/epjconf_nd2019_01020.pdf
collection DOAJ
language English
format Article
sources DOAJ
author Praena Javier
L Isabelópez-Casas
Sabat Mariaé-Gilarte
Arias Fernando de Saavedra
Porras Ignacio
spellingShingle Praena Javier
L Isabelópez-Casas
Sabat Mariaé-Gilarte
Arias Fernando de Saavedra
Porras Ignacio
Measurements of the 33S (n, α)30Si cross-section at n_TOF and ILL: Implications in neutron capture therapy
EPJ Web of Conferences
author_facet Praena Javier
L Isabelópez-Casas
Sabat Mariaé-Gilarte
Arias Fernando de Saavedra
Porras Ignacio
author_sort Praena Javier
title Measurements of the 33S (n, α)30Si cross-section at n_TOF and ILL: Implications in neutron capture therapy
title_short Measurements of the 33S (n, α)30Si cross-section at n_TOF and ILL: Implications in neutron capture therapy
title_full Measurements of the 33S (n, α)30Si cross-section at n_TOF and ILL: Implications in neutron capture therapy
title_fullStr Measurements of the 33S (n, α)30Si cross-section at n_TOF and ILL: Implications in neutron capture therapy
title_full_unstemmed Measurements of the 33S (n, α)30Si cross-section at n_TOF and ILL: Implications in neutron capture therapy
title_sort measurements of the 33s (n, α)30si cross-section at n_tof and ill: implications in neutron capture therapy
publisher EDP Sciences
series EPJ Web of Conferences
issn 2100-014X
publishDate 2020-01-01
description Up to a couple of years ago, the 33S(n, α)30Si cross-section data had been limited and scarce. The origin in the solar system of 36S had been the only motivation to study that cross-section. However, a few years ago, the 33S(n, α)30Si reaction was proposed as a possible target in neutron capture therapy (NCT) due to the excellent bio-properties of 33S and the significant resonance at 13.45 keV of the cross-section for which a high-energy α is emitted. Prior to the experiments carried out at n_TOF-CERN and at the Institut Laue-Langevin (ILL) facilities, the data situation was: no data from the thermal point up to 10 keV; from 10 keV to 300 keV, there was only one (n, α) measurement able to resolve the resonances with a questionable value of the 13.45-keV resonance; and the thermal point did not have a consistent value. Here we summarize three experiments that have been performed covering the whole energy range of interest in NCT and astrophysics. These experiments have solved the most important issues. The data of the present work and the evaluated data are used to calculate the dose rate in the tissue.
url https://www.epj-conferences.org/articles/epjconf/pdf/2020/15/epjconf_nd2019_01020.pdf
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