[Bubble] Calculable microscopic theory for 12C(α,γ)16O cross section near Gamow window
Jay Benesch
benesch at jlab.org
Mon Nov 16 06:15:39 EST 2020
seems relevant
https://arxiv.org/abs/2011.06701
Calculable microscopic theory for 12C(α,γ)16O cross section near Gamow
window
Y. Suzuki
12C(α,γ)16O radiative-capture process is a key reaction to produce
the element of oxygen in stars. Measuring the cross section near the
Gamow window is extremely hard because it is too small. To make a
theoretical contribution towards resolving the long-standing problem, I
present a microscopic formulation that aims at providing all materials
needed to calculate the cross section. The states of 12C and 16O
relevant to the reaction are respectively described with fully
microscopic 3 α-particle and 4 α-particle configurations, in which the
relative motion among the α particles is expanded in terms of correlated
Gaussian basis functions. The configuration space has the advantage of
being able to well describe the reduced α-width amplitudes of the states
of 16O. Both electric dipole and electric quadrupole transitions are
responsible for the radiative-capture process. The α particle is
described with a (0s)4 configuration admixed with a small amount of an
isospin T=1 impurity component, which is crucially important to account
for the isovector electric dipole transition. The isoscalar electric
dipole operators are also taken into account up to the first order
beyond the long-wavelength approximation. All the necessary ingredients
are provided to make the paper self-contained and ready for numerical
computations.
Comments: 24 pages, accepted for publication in Few-Body Systems
Subjects: Nuclear Theory (nucl-th); Solar and Stellar Astrophysics
(astro-ph.SR); Nuclear Experiment (nucl-ex)
Cite as: arXiv:2011.06701 [nucl-th]
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