First excited state of the s -process branching nucleus 95 Zr

Astronomy and Astrophysics – Astrophysics

Scientific paper

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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.

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