Proton capture on P in novae: On the existence of states at MeV and MeV in S
arXiv:2205.08476 · doi:10.1103/PhysRevC.105.055805
Abstract
We use a high resolution measurement to investigate the claimed existence of a 6401(3) keV state in S that may affect the nuclear reaction rate in oxygen-neon (ONe) novae. Our data are shown to exclude the null hypothesis - that the state does not exist - with high significance. Additionally, the data also suggest the existence of a hitherto unreported state at 6648(4) keV. This state corresponds to a resonance at keV, located below the higher edge of the Gamow window for peak nova temperatures of about 0.4 GK.
References in corpus (16)
- Asymptotic formulae for likelihood-based tests of new physics
- Charged-Particle Thermonuclear Reaction Rates: II. Tables and Graphs of Reaction Rates and Probability Density Functions
- The Effects of Thermonuclear Reaction Rate Variations on Nova Nucleosynthesis: A Sensitivity Study
- Presolar Grains from Novae
- Theoretical Modeling of the Thermal State of Accreting White Dwarfs Undergoing Classical Novae
- Nuclear uncertainties in the NeNa-MgAl cycles and production of 22Na and 26Al during nova outbursts
- Synthesis of intermediate-mass elements in classical novae: from Si to Ca
- Hydrodynamic Models of Type I X-Ray Bursts: Metallicity Effects
- Searching for new physics with profile likelihoods: Wilks and beyond
- Isospin Mixing Reveals P()S Resonance Influencing Nova Nucleosynthesis
- CNO "Breakout" and Nucleosynthesis in Classical Novae
- Benchmarking Xe Neutrinoless Decay Matrix Element Calculations with the Reaction
- Constraining the P(S reaction rate in ONe novae via the weak, low-energy, -delayed proton decay of Cl
- Investigation of pair-correlated states in Ba via the Ba() reaction
- Spectroscopy of states in using the reaction
- Isospin Mixing and the Cubic Isobaric Multiplet Mass Equation in the Lowest T = 2, A = 32 Quintet