Evaluation of the $^{35}$K($p$,$\gamma$)$^{36}$Ca reaction rate using the $^{37}$Ca($p$,$d$)$^{36}$Ca transfer reaction
L. Lalanne, O. Sorlin, M. Assi\'e, F. Hammache, N. de S\'er\'eville,, S. Koyama, D. Suzuki, F. Flavigny, D. Beaumel, Y Blumenfeld, B. A. Brown, F., De Oliveira Santos, F. Delaunay, S. Franchoo, J. Gibelin, V. Girard-Alcindor,, J. Guillot, O. Kamalou, N. Kitamura, V. Lapoux

TL;DR
This study refines the $^{35}$K$(p,)$^{36}$Ca reaction rate using transfer reaction data, showing it has minimal impact on X-ray burst light curves and is now well constrained across relevant temperatures.
Contribution
The paper provides new spectroscopic data and reaction rate calculations for $^{35}$K$(p,)$^{36}$Ca, reducing uncertainties and clarifying its influence on astrophysical models.
Findings
Reaction rate is constrained within a factor of 2 at 1 sigma.
New resonances discovered at higher temperatures increase the reaction rate.
The reaction does not significantly affect X-ray burst light curve shape.
Abstract
A recent sensitivity study has shown that the KCa reaction is one of the ten reaction rates that could significantly impact the shape of the calculated X-ray burst light curve. In this work, we propose to reinvestigate the KCa reaction rate, as well as related uncertainties, by determining the energies and decay branching ratios of Ca levels, within the Gamow window, in the 0.5 to 2 GK X-ray burst temperature range. These properties were studied using the one neutron pick-up transfer reaction CaCa in inverse kinematics using a radioactive beam of Ca at 48 MeV nucleon. The experiment performed at GANIL, used the liquid Hydrogen target CRYPTA, the MUST2 detector array for the detection of the light charged particles and a zero degree detection system for the outgoing heavy ions. The atomic…
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