Clustering effects in the $^6$Li(p,$^3$He)$^4$He reaction at astrophysical energies

TL;DR

This paper investigates how clustered configurations of $^6$Li influence the reaction cross section at astrophysical energies, revealing that clustering significantly enhances the astrophysical S factor, unlike static deformations.

Contribution

The study provides a theoretical comparison of two- and three-cluster models of $^6$Li and their effects on the $^6$Li(p,$^3$He)$^4$He reaction cross section at low energies.

Findings

Clustered $^6$Li configurations significantly increase the astrophysical S factor.

Static deformations have negligible impact at very low energies.

Three-cluster models reveal the role of $oldsymbol{ extalpha}$-d clustering in reaction observables.

Abstract

Background: The understanding of nuclear reactions between light nuclei at energies below the Coulomb barrier is important for several astrophysical processes, but their study poses experimental and theoretical challenges. At sufficiently low energies, the electrons surrounding the interacting ions affect the scattering process. Moreover, the clustered structure of some of these nuclei may play a relevant role on the reaction observables. Purpose: In this article, we focus on a theoretical investigation of the role of clustered configurations of $^6$Li in reactions of astrophysical interest. Methods: The $^6$Li(p,$^3$He)$^4$He reaction cross section is described considering both the direct transfer of a deuteron as a single point-like particle in Distorted Wave Born Approximation (DWBA), and the transfer of a neutron and a proton in second-order DWBA. A number of two- and three-cluster structure models for $^6$Li are compared. Results: Within the two-cluster structure model, we explore the impact of the deformed components in the $^6$Li wave-function on the reaction of interest. Within the three-cluster structure model, we gauge the degree of $\alpha$-d clustering and explicitly probe its role on specific features of the reaction cross section. We compare the energy trend of the astrophysical $S$ factor deduced in each case. Conclusions: Clustered $^6$Li configurations lead in general to a significant enhancement of the astrophysical factor in the energy region under study. This effect only originates from clustering, whereas static deformations of the ground-state configuration play a negligible role at very low energies.