Astronomy and Astrophysics – Astrophysics
Scientific paper
Oct 2003
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003phrvc..68d8802s&link_type=abstract
Physical Review C, vol. 68, Issue 4, id. 048802
Astronomy and Astrophysics
Astrophysics
5
Transfer Reactions, 90<=A<=149, Hydrostatic Stellar Nucleosynthesis
Scientific paper
The transfer reaction 94 Zr (d,p) 95 Zr has been studied to check the existence of a low-lying first excited level at 23 keV in 95 Zr . This level—if it exists—might have significant influence on the branching of the astrophysical s process at the branching nucleus 95 Zr . Our experimental spectra, measured with very good energy resolution, do not show any evidence for the existence of such a low-lying level. This is in agreement with experimental results from several reactions and contradicts the only claim for evidence of such a low-lying level which was also derived from 94 Zr (d,p) 95 Zr data, however with moderate resolution, but still the best of the previous experiments.
Faestermann Th.
Graw G.
Hertenberger Ralf
Mohr Paul
Sonnabend Kerstin
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