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Open AccessIdentification of \(\gamma\)-decaying resonant states in 26Mg and their importance for the astrophysical s process
The 22Ne(\( \alpha\)α, n) reaction is expected to provide the dominant neutron source for the weak s process in massive stars and intermediate-mass (IM) Asymptotic Giant Branch (AGB) stars. However, the production ...
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Open AccessAngle-integrated measurements of the 26Al (d, n)27Si reaction cross section: a probe of spectroscopic factors and astrophysical resonance strengths
Measurements of angle-integrated cross sections to discrete states in 27Si have been performed studying the 26Al (d, n) reaction in inverse kinematics by tagging states by their characteristic
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Re-evaluating reaction rates relevant to nova nucleosynthesis from a nuclear structure perspective
Conventionally, reaction rates relevant to nova nucleosynthesis are determined by performing the relevant proton capture reactions directly for stable species, or as has become possible more recently in invers...