Measurement of very low (alpha,n) cross sections of astrophysical interest

Taín Enríquez, José Luis; Jordan Herrero, Donato; Agramunt Ros, Jorge; Algora, A.; Bandac, I; Bettini, S; Caballero Folch, Roger; Calviño Tavares, Francisco; Cano-Ott, D; Cortés Rossell, Guillem Pere; Domingo-Pardo, C; Fraile, L. M.; Garcia, A.R.; Gomez-Cadenas, J.J.; José Pont, Jordi; Longland, Richard; Mendoza, E

doi:10.1088/1742-6596/665/1/012031

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Document typeArticle

Defense date2016

PublisherInstitute of Physics (IOP)

Rights accessOpen Access

Except where otherwise noted, content on this work is licensed under a Creative Commons license : Attribution-NonCommercial-NoDerivs 3.0 Spain

Abstract

The reactions 13C( ; n)16O and 22Ne( ; n)25Mg are the primary sources of neutrons for the astrophysical s-process. The feasibility of cross section measurements within the respective Gamow windows is discussed in quantitative terms for a 4 neutron counter, based on 3He tubes and a neutron moderator, placed in an underground lab.

CitationTaín, J.L., Jordan, D., Agramunt, J., Algora, A., Bandac, I., Bettini, S., Caballero-Folch, R., Calviño, F., Cano-Ott, D., Cortes, G., Domingo-Pardo, C., Fraile, L., Garcia, A., Gomez-Cadenas, J., Jose, J., Longland, R., Mendoza, E. Measurement of very low (alpha,n) cross sections of astrophysical interest. "Journal of physics: conference series", 2016, vol. 665, núm. 1, p. 012031-1-012031-6.

URIhttp://hdl.handle.net/2117/84952

DOI10.1088/1742-6596/665/1/012031

ISSN1742-6588

Publisher versionhttp://iopscience.iop.org/article/10.1088/1742-6596/665/1/012031/meta

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