The 8Li(d,p)9Li Reaction and the Astrophysical 8Li(n,g)9Li Reaction Rate

TL;DR

This study measures the $^8$Li(d,p)$^9$Li reaction to indirectly determine the $^8$Li(n,$$)$^9$Li reaction rate, providing crucial data for astrophysical models of nucleosynthesis and the early universe.

Contribution

First experimental measurement of the $^8$Li(d,p)$^9$Li reaction angular distribution and its use to constrain the $^8$Li(n,$$)$^9$Li reaction rate relevant for astrophysics.

Findings

Determined the $^8$Li(d,p)$^9$Li$\_$g.s. cross section as 7.9 ± 2.0 mb.

Derived the spectroscopic factor $S_{1,3/2}$ as 0.68 ± 0.14.

Calculated the astrophysical $^8$Li(n,$$)$^9$Li reaction rate as 3970 ± 950 cm$^3$ mol$^{-1}$ s$^{-1}$ at $T_9$=1.

Abstract

The $^8$Li($n,\gamma$)$^9$Li reaction plays an important role in both the r-process nucleosynthesis and the inhomogeneous big bang models, its direct capture rates can be extracted from the $^8$Li($d, p$)$^9$Li reaction, indirectly. We have measured the angular distribution of the $^8$Li($d, p$)$^9$Li$_{\textrm{g.s.}}$ reaction at $E_{\textrm{c.m.}}$ = 7.8 MeV in inverse kinematics using coincidence detection of $^{9}\textrm{Li}$ and recoil proton, for the first time. Based on Distorted Wave Born Approximation (DWBA) analysis, the $^{8}\textrm{Li}(d, p)^{9}\textrm{Li}_{\textrm{g.s.}}$ cross section was determined to be 7.9 $\pm$ 2.0 mb. The single particle spectroscopic factor, $S_{1,3/2}$, for the ground state of $^{9}\textrm{Li}$ = $^{8}\textrm{Li} \otimes n$ was derived to be $0.68\pm 0.14$, and then used to calculate the direct capture cross sections for the $^{8}\textrm{Li}(n, \gamma)^{9}\textrm{Li}_{\textrm{g.s.}}$ reaction at energies of astrophysical interest. The astrophysical $^{8}\textrm{Li}(n, \gamma)^{9}\textrm{Li}_{\textrm{g.s.}}$ reaction rate for the direct capture was found to be 3970 $\pm$ 950 $\textrm{cm}^{3}\textrm{mole}^{-1}s^{-1}$ at $T_9$ = 1. This presents the first experimental constraint for the $^{8}\textrm{Li}(n, \gamma)^{9}\textrm{Li}$ reaction rates of astrophysical relevance.