Isospin-forbidden electric-dipole capture and the $\alpha(d,\gamma)^6$Li reaction
Daniel Baye, E.M. Tursunov

TL;DR
This paper investigates the isospin-forbidden electric-dipole (E1) capture in the $ ext{ }^2$H($ ext{ }^4$He,$ ext{ }^6$Li) reaction, analyzing theoretical contributions and comparing calculations with recent experimental data, emphasizing the role of isovector E1 transitions.
Contribution
The study provides a microscopic analysis of isoscalar and isovector E1 contributions, deriving the dominant operators and confirming the importance of small isospin admixtures in explaining experimental data.
Findings
The calculated astrophysical S factor agrees with recent LUNA data.
The exact-masses prescription is not justified microscopically and should be avoided.
Capture from initial S-wave scattering states significantly impacts the reaction.
Abstract
At the long-wavelength approximation, transitions are forbidden between isospin-zero states. Hence radiative capture is strongly hindered in reactions involving nuclei but the astrophysical factor may remain comparable to, or larger than, the one. Theoretical expressions of the isoscalar and isovector contributions to capture are analyzed in microscopic and three-body approaches in the context of the Li reaction. The lowest non-vanishing terms of the operators are derived and the dominant contributions to matrix elements are discussed. The astrophysical factor computed with some of these contributions in a three-body model is in agreement with the recent low-energy experimental data of the LUNA collaboration. This confirms that a correct treatment of the isovector transitions involving small isospin-one…
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