Correlated Energy Uncertainties in Reaction Rate Calculations
arXiv:2007.03802 · doi:10.1051/0004-6361/202038151
Abstract
Context. Monte Carlo methods can be used to evaluate the uncertainty of a reaction rate that arises from many uncertain nuclear inputs. However, until now no attempt has been made to find the effect of correlated energy uncertainties in input resonance parameters. Aims. To investigate the impact of correlated energy uncertainties on reaction rates. Methods. Using a combination of numerical and Monte Carlo variation of resonance energies, the effect of correlations are investigated. Five reactions are considered: two fictional, illustrative cases and three reactions whose rates are of current interest. Results. The effect of correlations in resonance energies depends on the specific reaction cross section and temperatures considered. When several resonances contribute equally to a reaction rate, and are located either side of the Gamow peak, correlations between their energies dilute their effect on reaction rate uncertainties. If they are both located above or below the maximum of the Gamow peak, however, correlations between their resonance energies can increase the reaction rate uncertainties. This effect can be hard to predict for complex reactions with wide and narrow resonances contributing to the reaction rate.
arXiv comment9 pages, 9 figures, accepted to Astronomy and Astrophysics
References in corpus (13)
- STARLIB: A Next-Generation Reaction-Rate Library for Nuclear Astrophysics
- Charged-Particle Thermonuclear Reaction Rates: I. Monte Carlo Method and Statistical Distributions
- Sensitivity of astrophysical reaction rates to nuclear uncertainties
- Uncertainties in the production of nuclei in massive stars obtained from Monte Carlo variations
- Properties of Carbon-Oxygen White Dwarfs From Monte Carlo Stellar Models
- Production of carbon-rich presolar grains from massive stars
- Uncertainties in s-process nucleosynthesis in low mass stars determined from Monte Carlo variations
- The Impact of Nuclear Reaction Rate Uncertainties On The Evolution of Core-Collapse Supernova Progenitors
- CNO "Breakout" and Nucleosynthesis in Classical Novae
- Recommendations for Monte Carlo nucleosynthesis sampling (Research Note)
- Thermonuclear reaction rate of Ne(,)Na from Monte-Carlo calculations
- Correlated Uncertainties in Monte Carlo Reaction Rate Calculations
- Evaluation of the N(,p)O thermonuclear reaction rate and its impact on the isotopic composition of supernova grains