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

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dc.contributor.authorFraile Prieto, Luis Mario
dc.date.accessioned2023-06-18T06:50:27Z
dc.date.available2023-06-18T06:50:27Z
dc.date.issued2016
dc.description© Iop Publishing Ltd. Articulo firmado por más de 10 autores. Nuclear Physics in Astrophysics Conference (NPA) (6 .2013. Lisboa, Portugal). This work was supported by the Spanish Ministerio de Economía y Competitividad under Grants CONSOLIDER-Ingenio 2010 CSD2008-0037 (CUP), PRI-PIMNUP-2011-1348, FPA2011-28770-C03-03, FPA2011-24553, FPA2010-17142 and CSD-2007-00042 (CPAN).
dc.description.abstractThe 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.description.departmentDepto. de Estructura de la Materia, Física Térmica y Electrónica
dc.description.facultyFac. de Ciencias Físicas
dc.description.refereedTRUE
dc.description.sponsorshipMinisterio de Economía y Competitividad
dc.description.statuspub
dc.eprint.idhttps://eprints.ucm.es/id/eprint/36089
dc.identifier.doi10.1088/1742-6596/665/1/012031
dc.identifier.issn1742-6588
dc.identifier.officialurlhttp://dx.doi.org/10.1088/1742-6596/665/1/012031
dc.identifier.relatedurlhttp://iopscience.iop.org/
dc.identifier.urihttps://hdl.handle.net/20.500.14352/24368
dc.journal.titleJournal of physics: Conference series
dc.language.isoeng
dc.publisherIOP Publishing Ltd
dc.relation.projectIDCONSOLIDER-Ingenio 2010
dc.relation.projectIDCSD2008-0037 (CUP)
dc.relation.projectIDPRI-PIMNUP-2011-1348
dc.relation.projectIDFPA2011-28770- C03-03
dc.relation.projectIDFPA2011-24553
dc.relation.projectIDFPA2010-17142
dc.relation.projectIDCSD-2007-00042 (CPAN)
dc.rightsAtribución 3.0 España
dc.rights.accessRightsopen access
dc.rights.urihttps://creativecommons.org/licenses/by/3.0/es/
dc.subject.cdu539.1
dc.subject.keywordAstronomy & Astrophysics
dc.subject.keywordPhysics
dc.subject.keywordNuclear
dc.subject.ucmFísica nuclear
dc.subject.unesco2207 Física Atómica y Nuclear
dc.titleMeasurement of very low (alpha,n) cross sections of astrophysical interest
dc.typejournal article
dc.volume.number665
dcterms.references[1] Kaeppeler F et al 2011 Rev. Mod. Phys. 83 157 [2] Fraile L M et al 2012 Letter of Intent to LSC: A nuclear astrophysics facility for LSC: the sources of neutrons in the stars and other reactions of astrophysical interest [3] Davids C N 1968 Nucl. Phys. A 110 619 [4] Ashery D 1969 Nucl. Phys. A 136 481 [5] Haas F X and Bair J K 1973 Phys. Rev. C 7 2432 [6] Harms F X et al 1991 Phys. Rev. C 43 2849 [7] Drotle H W et al 1993 Astroph. J. 414 735 [8] Jaeger M et al 2001 Phys. Rev. Lett. 87 202501 [9] Heil M et al 2008 Phys. Rev. C 78 025803 [10] Gomez-Hornillos M B et al 2011 J. Phys. Conf. Ser. 312 052008 [11] Jordan D et al 2013 Astrop. Phys. 42 1 [12] Bramblett R L et al 1960 Nucl. Instrum. Methods 9 1. [13] D. Pelowitz (Ed.), MCNPX Users Manual Version 2.5.0, Los Alamos National Laboratory, Report LA-CP-05-0369, April 2005. [14] McDonald A B 2009 J. Phys. Conf. Ser. 173 012002
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relation.isAuthorOfPublicationec83106c-33f4-426c-afd6-68c5d859f9d4
relation.isAuthorOfPublication.latestForDiscoveryec83106c-33f4-426c-afd6-68c5d859f9d4

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