TDCCWP calculations with thermal initial states show neutron capture cross sections on 188Os decrease with temperature due to dynamical nuclear couplings neglected in Hauser-Feshbach models.
The above process is carried out using a modified Chebyshev propagation scheme [15–17] to apply the ex- ponential time-evolution operator to the wave-packet
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Thermal effects on stellar neutron capture reactions: a quantum dynamical approach
TDCCWP calculations with thermal initial states show neutron capture cross sections on 188Os decrease with temperature due to dynamical nuclear couplings neglected in Hauser-Feshbach models.