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Measurement of very low (alpha,n) cross sections of astrophysical interest
| dc.contributor.author | Taín Enríquez, José Luis |
| dc.contributor.author | Jordán, D. |
| dc.contributor.author | Agramunt Ros, Jorge |
| dc.contributor.author | Caballero-Folch, R. |
| dc.contributor.author | Calviño Tavares, Francisco |
| dc.contributor.author | Cortés Rossell, Guillem Pere |
| dc.contributor.author | Longland, Richard |
| dc.contributor.author | Parikh, Anuj Ramesh |
| dc.contributor.other | Universitat Politècnica de Catalunya. Departament de Física |
| dc.date.accessioned | 2016-11-04T12:03:16Z |
| dc.date.available | 2016-11-04T12:03:16Z |
| dc.date.issued | 2013 |
| dc.identifier.citation | Taín, J.L., Jordán, D., Agramunt, J., Caballero-Folch, R., Calviño, F., Cortes, G., Longland, R., Parikh, A. Measurement of very low (alpha,n) cross sections of astrophysical interest. A: Nuclear Physics in Astrophysics. "Journal of Physics: Conference Series, vol. 665, no. 1, January 5, 2016". Lisboa: Institute of Physics (IOP), 2013, p. 1-6. |
| dc.identifier.uri | http://hdl.handle.net/2117/91475 |
| dc.description.abstract | The reactions C-13(alpha,n)O-16 and Ne-22(alpha,n)Mg-25 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 pi neutron counter, based on He-3 tubes and a neutron moderator, placed in an underground lab. |
| dc.format.extent | 6 p. |
| dc.language.iso | eng |
| dc.publisher | Institute of Physics (IOP) |
| dc.rights.uri | http://creativecommons.org/licenses/by-nc-nd/3.0/es/ |
| dc.subject | Àrees temàtiques de la UPC::Física |
| dc.subject.lcsh | Neutrons |
| dc.subject.lcsh | Astrophysics |
| dc.subject.other | Cross section |
| dc.subject.other | Neutron |
| dc.subject.other | Astrophysics |
| dc.title | Measurement of very low (alpha,n) cross sections of astrophysical interest |
| dc.type | Conference report |
| dc.subject.lemac | Neutrons |
| dc.subject.lemac | Astrofísica |
| dc.contributor.group | Universitat Politècnica de Catalunya. ANT - Advanced Nuclear Technologies Research Group |
| dc.identifier.doi | 10.1088/1742-6596/665/1/012031 |
| dc.relation.publisherversion | http://iopscience.iop.org/article/10.1088/1742-6596/665/1/012031 |
| dc.rights.access | Open Access |
| local.identifier.drac | 19070824 |
| dc.description.version | Postprint (published version) |
| local.citation.author | Taín, J.L.; Jordán, D.; Agramunt, J.; Caballero-Folch, R.; Calviño, F.; Cortes, G.; Longland, R.; Parikh, A. |
| local.citation.contributor | Nuclear Physics in Astrophysics |
| local.citation.pubplace | Lisboa |
| local.citation.publicationName | Journal of Physics: Conference Series, vol. 665, no. 1, January 5, 2016 |
| local.citation.startingPage | 1 |
| local.citation.endingPage | 6 |
