Charged-Particle Thermonuclear Reaction Rates: IV. Comparison to Previous Work
arXiv:1004.4150 · doi:10.1016/j.nuclphysa.2010.04.012
Abstract
We compare our Monte Carlo reaction rates (see Paper II of this series) to previous results that were obtained by using the classical method of computing thermonuclear reaction rates. For each reaction, the comparison is presented using two types of graphs: the first shows the change in reaction rate uncertainties, while the second displays our new results normalized to the previously recommended reaction rate. We find that the rates have changed significantly for almost all reactions considered here. The changes are caused by (i) our new Monte Carlo method of computing reaction rates (see Paper I of this series), and (ii) newly available nuclear physics information (see Paper III of this series).
67 pages, 62 figures
References in corpus (5)
- Reaction Rates Uncertainties and the Production of F19 in AGB Stars
- Measurement of the 20 and 90 keV resonances in the N reaction via THM
- The importance of 15O(a,g)19Ne to X-ray bursts and superbursts
- New Cl(p,)Ar reaction rate for astrophysical rp-process calculations
- Thermonuclear Reaction Rate of 23Mg(p,gamma)24$Al
Cited by in corpus (23)
- NACRE II: an update of the NACRE compilation of charged-particle-induced thermonuclear reaction rates for nuclei with mass number
- The s process in asymptotic giant branch stars of low metallicity and the composition of carbon-enhanced metal-poor stars
- The Thermonuclear Runaway and the Classical Nova Outburst
- Radioactive nuclei from cosmochronology to habitability
- Carbon-enhanced metal-poor stars: a window on AGB nucleosynthesis and binary evolution. II. Statistical analysis of a sample of 67 CEMP- stars
- Bayesian Estimation of Thermonuclear Reaction Rates
- New experimental study of low-energy (p,gamma) resonances in magnesium isotopes
- Statistical Methods for Thermonuclear Reaction Rates and Nucleosynthesis Simulations
- Aluminium-26 from massive binary stars I: non-rotating models
- Thermonuclear reaction rate of 18O(p,gamma)19F
- The Status and Future of Direct Nuclear Reaction Measurements for Stellar Burning
- Recommendations for Monte Carlo nucleosynthesis sampling (Research Note)
- Rubidium and zirconium abundances in massive Galactic asymptotic giant branch stars revisited
- Thermonuclear reaction rate of Ne(,)Na from Monte-Carlo calculations
- Recent results in nuclear astrophysics
- Very massive star winds as sources of the short-lived radioactive isotope Al
- Selected topics in the evolution of low-mass stars
- Correlated Uncertainties in Monte Carlo Reaction Rate Calculations
- Thermonuclear 17O(n,gamma)18O reaction rate and its astrophysical implications
- Thermonuclear reaction rate of Si(p,)P
- Hydrogen burning of Si and its impact on presolar stardust grains from classical novae
- Explosive Nucleosynthesis: What we learned and what we still do not understand
- The 2025 Evaluation of Experimental Thermonuclear Reaction Rates (ETR25)