Doppler Broadening in Mg()Ne Decay
arXiv:1901.01966 · doi:10.1103/PhysRevC.99.065801
Abstract
Background: The O()Ne bottleneck reaction in Type I x-ray bursts is the most important thermonuclear reaction rate to constrain experimentally, in order to improve the accuracy of burst light-curve simulations. A proposed technique to determine the thermonuclear rate of this reaction employs the Mg()O decay sequence. The key O()Ne resonance at an excitation of 4.03 MeV is now known to be fed in Mg()Ne; however, the energies of the protons feeding the 4.03 MeV state are unknown. Knowledge of the proton energies will facilitate future Mg()O measurements. Purpose: To determine the energy of the proton transition feeding the 4.03 MeV state in Ne. Method: A fast beam of Mg was implanted into a plastic scintillator, which was used to detect particles. 16 high purity germanium detectors were used to detect rays emitted following decay. A Monte Carlo method was used to simulate the Doppler broadening of Ne rays and compare to the experimental data. Results: The center of mass energy between the proton and Ne, feeding the 4.03 MeV state, is measured to be 1.21 MeV, corresponding to a Na excitation energy of 7.44 MeV. Absolute feeding intensities and -decay branching ratios of Ne states were determined including the 1615 keV state. A new decay branch from the 1536 keV state in Ne to the ground state is reported. The lifetime of the 1507 keV state in Ne is measured to be 4.3 ps resolving discrepancies in the literature. Conflicting Mg() decay schemes in published literature are clarified.
11 pages, 13 figures