Spin-parities of sub-threshold resonances in the ${}^{18}$F(p, $\alpha$)${}^{15}$O reaction

Abstract

The ${}^{18}$F(p, $\alpha$)${}^{15}$O reaction is key to determining the ${}^{18}$F abundance in classical novae. However, the cross section for this reaction has large uncertainties at low energies largely caused by interference effects. Here, we resolve a longstanding issue with unknown spin-parities of sub-threshold states in ${}^{19}$Ne that reduces these uncertainties. The ${}^{20}$Ne(${}^3$He, ${}^4$He)${}^{19}$Ne neutron pick-up reaction was used to populate ${}^{19}$Ne excited states, focusing on the energy region of astrophysical interest ($\approx$ 6 - 7 MeV). The experiment was performed at the Triangle Universities Nuclear Laboratory using the high resolution Enge split-pole magnetic spectrograph. Spins and parities were found for states in the astrophysical energy range. In particular, the state at 6.133 MeV (E${}_r^{\text{c.m.}}=-278$ keV) was found to have spin and parity of $3/2^{+}$ and we confirm the existence of an unresolved doublet close to 6.288 MeV (E${}_r^{\text{c.m.}}=-120$ keV) with J${}^{\pi }$ = $1/2^{+}$ and a high-spin state. Using these results, we demonstrate a significant factor of two decrease in the reaction rate uncertainties at nova temperatures.

arXiv comment15 pages, 6 figures, accepted in Phys. Rev. C. Corrected typos and references

References in corpus (9)

• New Constraints on the 18F(p,alpha) 15O Rate in Novae from the (d,p) Reaction
• Particle decay branching ratios for states of astrophysical importance in 19Ne
• Is γ-ray emission from novae affected by interference effects in the 18F(p,α)15O reaction?
• Resonances in 19Ne with relevance to the astrophysically important 18F(p,α)15O reaction
• Subthreshold resonances and resonances in the $R$-matrix method for binary reactions and in the Trojan Horse method
• Spectroscopy of ${}^{19}$Ne for the thermonuclear ${}^{15}$O($\alpha ,\gamma$)${}^{19}$Ne and ${}^{18}$F($p,\alpha$)${}^{15}$O reaction rates
• Key ${}^{19}$Ne states identified affecting $\gamma$-ray emission from ${}^{18}$F in novae
• Uncertainties in the ${}^{18}$F(p,$\alpha$)${}^{15}$O reaction rate in classical novae
• Sub-threshold states in ${}^{19}$Ne relevant to ${}^{18}$F(p,$\alpha$)${}^{15}$O