Abstract
The transfer reaction Zr-94(d,p)Zr-95 has been studied to check the
existence of a low-lying first excited level at 23 keV in Zr-95. This
level-if it exists-might have significant influence on the branching of
the astrophysical s process at the branching nucleus Zr-95. 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 Zr-94(d,p)Zr-95 data, however with moderate
resolution, but still the best of the previous experiments.
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