<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"><mml:mmultiscripts><mml:mi>Ne</mml:mi><mml:mprescripts/><mml:none/><mml:mn>19</mml:mn></mml:mmultiscripts></mml:math> level structure for explosive nucleosynthesis
M. R. Hall, D. W. Bardayan, T. Baugher, A. Lepailleur, S. D. Pain, A. Ratkiewicz, S. Ahn, J. Allen, John T. Anderson, A. D. Ayangeakaa, J. C. Blackmon, S. Burcher, M. P. Carpenter, S. M., K. Y. Chae, K. A. Chipps, J. A. Cizewski, M. Febbraro, O. Hall, J. Hu, C. L. Jiang, K. L. Jones, E. J. Lee, P. D. O’Malley, S. Ota, B. C. Rasco, D. Santiago-Gonzalez, D. Seweryniak, H. Sims, K. Smith, Wanpeng Tan, Paul M. Thompson, C. Thornsberry, R. L. Varner, D. Walter, G. L. Wilson, S. Zhu
Abstract
Background: $^{19}\mathrm{Ne}$ is an important isotope in nuclear astrophysics due to its role in both the $^{18}\mathrm{F}(p,\ensuremath{\alpha})^{15}\mathrm{O}$ and $^{15}\mathrm{O}(\ensuremath{\alpha},\ensuremath{\gamma})^{19}\mathrm{Ne}$ reactions in novae and Type I x-ray bursts, respectively. The energy levels of $^{19}\mathrm{Ne}$ near the $\ensuremath{\alpha}$ and proton thresholds (${S}_{\ensuremath{\alpha}}=3529$ keV, ${S}_{p}=6410$ keV) correspond to resonances in both of these reactions. Previous measurements to study the structure of $^{19}\mathrm{Ne}$ have focused on both regions in an effort to constrain these reaction rates.Purpose: Discrepancies in the energies, spins, and parities for levels in $^{19}\mathrm{Ne}$ from previous measurements contribute to the reaction-rate uncertainties. Gamma rays from the depopulation of excited states in $^{19}\mathrm{Ne}$ were measured to reduce the level-energy uncertainties and inconsistencies in previous spin-parity assignments.Methods: The $^{19}\mathrm{F}(^{3}\mathrm{He},t)^{19}\mathrm{Ne}$ reaction was used to elucidate the structure of $^{19}\mathrm{Ne}$ levels up to ${E}_{x}=6.9$ MeV. The reaction products were measured using Gammasphere ORRUBA: Dual Detectors for Experimental Structure Studies---a coupling of the Oak Ridge Rutgers University Barrel Array and Gammasphere at Argonne National Laboratory. Tritons produced in the reaction were measured in coincidence with $\ensuremath{\gamma}$ rays from the deexcitation of $^{19}\mathrm{Ne}$ energy levels.Results: Previously unobserved transitions allowed for discrepancies in the resonance properties relevant to these two reactions to be resolved. In total, 41 transitions from 21 energy levels were measured in $^{19}\mathrm{Ne}$, with 21 of those transitions being previously unobserved. Of particular importance, transitions from two $3/{2}^{+}$ states with energies of 6423(3) and 6441(3) keV, crucial for accurate estimations of the $^{18}\mathrm{F}(p,\ensuremath{\alpha})^{15}\mathrm{O}$ reaction rate, were found.Conclusions: Energies and spin-parities of important energy levels near the proton and $\ensuremath{\alpha}$ thresholds were measured and some of the discrepancies in previous measurements were resolved. Measurement of the two near-threshold $3/{2}^{+}$ states reduced the calculated upper limit of the $^{18}\mathrm{F}(p,\ensuremath{\alpha})^{15}\mathrm{O}$ reaction rate by factors of 1.5--17 in the nova temperature range.