Low-lying level structure of Cu and its implications on the rp process
arXiv:1704.07941 · doi:10.1103/PhysRevC.95.055806
Abstract
The low-lying energy levels of proton-rich Cu have been extracted using in-beam -ray spectroscopy with the state-of-the-art -ray tracking array GRETINA in conjunction with the S800 spectrograph at the National Superconducting Cyclotron Laboratory at Michigan State University. Excited states in Cu serve as resonances in the Ni(p,)Cu reaction, which is a part of the rp-process in type I x-ray bursts. To resolve existing ambiguities in the reaction Q-value, a more localized IMME mass fit is used resulting in ~keV. We derive the first experimentally-constrained thermonuclear reaction rate for Ni(p,)Cu. We find that, with this new rate, the rp-process may bypass the Ni waiting point via the Ni(p,) reaction for typical x-ray burst conditions with a branching of up to 40. We also identify additional nuclear physics uncertainties that need to be addressed before drawing final conclusions about the rp-process reaction flow in the Ni region.
8 pages, accepted for Phys. Rev. C
References in corpus (5)
- Proton Drip-Line Calculations and the Rp-process
- Evaluated Experimental Isobaric Analogue States from to and associated IMME coefficients
- Statistical Methods for Thermonuclear Reaction Rates and Nucleosynthesis Simulations
- Mass measurements in the vicinity of the doubly-magic waiting point 56Ni
- Observation of the -delayed -proton decay of Zn and its impact on the Gamow Teller strength evaluation
Cited by in corpus (11)
- Nuclear Physics of the Outer Layers of Accreting Neutron Stars
- Dependence of X-ray Burst Models on Nuclear Masses
- Horizons: Nuclear Astrophysics in the 2020s and Beyond
- High-precision mass measurement of Cu and the redirection of the rp-process flow
- The Regulated NiCu Cycles with the new Cu(p,)Zn reaction rate and the Influence on Type-I X-Ray Bursts: GS 182624 Clocked Burster
- On the inversion of isobaric-analogue states in nuclei
- Burning in the tail: implications for a burst oscillation model
- Zn -delayed proton emission establishes the Ni -process waiting point bypass
- Isospin Mixing and the Cubic Isobaric Multiplet Mass Equation in the Lowest T = 2, A = 32 Quintet
- Second T = 3/2 state in B and the isobaric multiplet mass equation
- Exploring Isospin Symmetry Breaking in Exotic Nuclei: High-Precision Mass Measurement of 23Si and Shell-Model Calculations of T = 5/2 Nuclei