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Measurement and analysis of the Am-243 neutron capture cross section at the n_TOF facility at CERN
TOF Collaboration, E. Mendoza, D. Cano-Ott +129
Background:The design of new nuclear reactors and transmutation devices requires to reduce the present neutron cross section uncertainties of minor actinides. Purpose: Reduce the $…
High accuracy determination of the U/U fission cross section ratio up to 1 GeV at n_TOF (CERN)
C. Paradela, M. Calviani, D. Tarrío +104
The U to U fission cross section ratio has been determined at n_TOF up to 1 GeV, with two different detection systems, in different geometrical configurations…
Measurement of the C()B cross section at n_TOF (CERN) by in-beam activation analysis
P. Žugec, N. Colonna, D. Bosnar +101
The integral cross section of the C()B reaction has been determined for the first time in the neutron energy range from threshold to several GeV at the n_TOF fac…
The Karlsruhe Astrophysical Database of Nucleosynthesis in Stars Project - Status and Prospects
Iris Dillmann, Tamas Szücs, Zsolt Fülöp +3
The KADoNiS (Karlsruhe Astrophysical Database of Nucleosynthesis in Stars) project is an astrophysical online database for cross sections relevant for nucleosynthesis in the pr…
GEANT4 simulation of the neutron background of the CD set-up for capture studies at n_TOF
TOF collaboration, P. Žugec, N. Colonna +104
The neutron sensitivity of the CD detector setup used at n_TOF for capture measurements has been studied by means of detailed GEANT4 simulations. A realistic software repli…
s-Processing in AGB Stars Revisited. I. Does the Main Component Constrain the Neutron Source in the 13C-Pocket?
O. Trippella, M. Busso, E. Maiorca +2
Slow neutron captures at A 85 are mainly guaranteed by the reaction 13C(,n)16O in AGB stars, requiring proton injections from the envelope. These were so far assumed to…
Neutron Reactions in Astrophysics
R. Reifarth, C. Lederer, F. Käppeler
The quest for the origin of matter in the Universe had been the subject of philosophical and theological debates over the history of mankind, but quantitative answers could be foun…
Galactic Chemical Evolution and solar s-process abundances: dependence on the 13C-pocket structure
S. Bisterzo, C. Travaglio, R. Gallino +2
We study the s-process abundances (A > 90) at the epoch of the solar-system formation. AGB yields are computed with an updated neutron capture network and updated initial solar abu…
Experimental neutron capture data of Ni from the CERN n_TOF facility
TOF collaboration, P. Žugec, M. Barbagallo +99
The Ni cross section has been measured at the neutron time of flight facility n_TOF at CERN, in the energy range from 27 meV up to 400 keV. In total, 51 resonances h…