RT Journal Article
T1 Measurement of very low (alpha,n) cross sections of astrophysical interest
A1 Fraile Prieto, Luis Mario
AB 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.
PB IOP Publishing Ltd
SN 1742-6588
YR 2016
FD 2016
LK https://hdl.handle.net/20.500.14352/24368
UL https://hdl.handle.net/20.500.14352/24368
LA eng
NO © 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).
NO Ministerio de Economía y Competitividad
DS Docta Complutense
RD 7 abr 2025