New $\alpha$ ANC measurement of the 1/2$^+$ state in $^{17}$O at 6.356 MeV, that dominates the $^{13}$C($\alpha$,n)$^{16}$O reaction rate at temperatures relevant for the s-process
M. L. Avila, G. V. Rogachev, E. Koshchiy, L. T. Baby, J. Belarge, K., W. Kemper, A. N. Kuchera, D. Santiago-Gonzalez

TL;DR
This study provides a new measurement of the alpha Asymptotic Normalization Coefficient (ANC) for the 1/2+ state in $^{17}$O at 6.356 MeV, clarifying previous experimental discrepancies and refining the reaction rate relevant for the s-process in stars.
Contribution
The paper introduces a novel alpha transfer measurement technique to accurately determine the ANC of the 1/2+ state in $^{17}$O, resolving prior experimental inconsistencies.
Findings
Discrepancies between previous alpha transfer experiments are resolved.
The measured ANC value is $( ilde C^{^{17} ext{O}(1/2+)}_{ ext{α-}^{13} ext{C}})^2=3.6 extpm0.7$ fm$^{-1}$.
Some disagreement remains with the Trojan Horse method measurement.
Abstract
Background: Accurate knowledge of the C(,)O reaction cross section is important for the understanding of the s-process in AGB stars, since it is considered to be the main source of neutrons. The sub-threshold 1/2 state at excitation energy of 6.356 MeV in O has a strong influence on the reaction cross section at energies relevant for astrophysics. Several experiments have been performed to determine the contribution of this state to the C(O reaction rate. Nevertheless, significant discrepancies between different measurements remain. Purpose: The aim of this work is to investigate these discrepancies. Method: An 8 MeV C beam (below the Coulomb barrier) was used to study the -transfer reaction Li(C,)O. Results: The squared Coulomb modified ANC of the 1/2 state in O measured in…
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