Monte Carlo variations as a tool to assess nuclear physics uncertainties in nucleosynthesis studies
@article{Rauscher2019MonteCV, title={Monte Carlo variations as a tool to assess nuclear physics uncertainties in nucleosynthesis studies}, author={Thomas Rauscher}, journal={arXiv: High Energy Astrophysical Phenomena}, year={2019} }
The propagation of uncertainties in reaction cross sections and rates of neutron-, proton-, and $\alpha$-induced reactions into the final isotopic abundances obtained in nucleosynthesis models is an important issue in studies of nucleosynthesis and Galactic Chemical Evolution. We developed a Monte Carlo method to allow large-scale postprocessing studies of the impact of nuclear uncertainties on nucleosynthesis. Temperature-dependent rate uncertainties combining realistic experimental and…
Figures from this paper
References
SHOWING 1-10 OF 15 REFERENCES
Uncertainties in νp-process nucleosynthesis from Monte Carlo variation of reaction rates
- PhysicsMonthly Notices of the Royal Astronomical Society
- 2019
It has been suggested that a νp-process can occur when hot, dense, and proton-rich matter is expanding within a strong flux of antineutrinos. In such an environment, proton-rich nuclides can be…
PHENOMENOLOGICAL STUDY OF INTERACTION BETWEEN SOLAR ACOUSTIC WAVES AND SUNSPOTS FROM MEASURED SCATTERED WAVEFUNCTIONS
- Physics
- 2012
The solar acoustic waves around a sunspot are modified because of the interaction with the sunspot. The interaction can be viewed as that the sunspot, excited by the incident wave, generates the…
VII. Note on regression and inheritance in the case of two parents
- MathematicsProceedings of the Royal Society of London
- 1895
Consider a population in which sexual selection and natural selection may or may not be taking place. Assume only that the deviations from the mean in the case of any organ of any generation follow…
Relationships between Hi Gas Mass, Stellar Mass, and the Star Formation Rate of HICAT+WISE (H i-WISE) Galaxies
- Physics, GeologyThe Astrophysical Journal
- 2018
We have measured the relationships between HI mass, stellar mass and star formation rate using the HI Parkes All Sky-Survey Catalogue (HICAT) and the Wide-field Infrared Survey Explorer (WISE). Of…
Uncertainties in s-process nucleosynthesis in low-mass stars determined from Monte Carlo variations
- Physics
- 2018
© 2018 The Author(s) Published by Oxford University Press on behalf of the Royal Astronomical Society
NEUTRON CROSS SECTIONS FOR NUCLEOSYNTHESIS STUDIES
- Physics
- 2000
Previous compilations of (n, gamma) cross sections of relevance for neutron capture nucleosynthesis in the big bang and in the slow neutron capture process (s process) have been updated to encompass…
Uncertainties in the production of p nuclides in thermonuclear supernovae determined by Monte Carlo variations
- Physics
- 2018
Thermonuclear supernovae originating from the explosion of a white dwarf accreting mass from a companion star have been suggested as a site for the production of p nuclides. Such nuclei are produced…
Uncertainties in s-process nucleosynthesis in massive stars determined by Monte Carlo variations
- Physics
- 2017
The s-process in massive stars produces the weak component of the s-process (nuclei up to A ∼ 90), in amounts that match solar abundances. For heavier isotopes, such as barium, production through…
Uncertainties in the production of p nuclei in massive stars obtained from Monte Carlo variations
- Physics
- 2016
T. Rauscher, N. Nishimura, R. Hirschi, G. Cescutti, A. St. J. Murphy and A. Heger, ‘Uncertainties in the production of p nuclei in massive stars obtained from Monte Carlo variations’, MNRAS Vol 463(…
Challenges in nucleosynthesis of trans-iron elements
- Physics
- 2014
Nucleosynthesis beyond Fe poses additional challenges not encountered when studying astrophysical processes involving light nuclei. Astrophysical sites and conditions are not well known for some of…