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Uncertainties in s −process nucleosynthesis in low mass stars determined from Monte Carlo variations
Autor:
Thomas Rauscher, A. St. J. Murphy, J. W. den Hartogh, Nobuya Nishimura, Sergio Cristallo, Raphael Hirschi, G. Cescutti
Publikováno v:
Monthly Notices of the Royal Astronomical Society
Cescutti, G, Hirschi, R, Nishimura, N, Hartogh, J W D, Rauscher, T, Murphy, A S J & Cristallo, S 2018, ' Uncertainties in s-process nucleosynthesis in low-mass stars determined from Monte Carlo variations ', Monthly Notices of the Royal Astronomical Society, vol. 478, no. 3, pp. 4101-4127 . https://doi.org/10.1093/mnras/sty1185
Cescutti, G, Hirschi, R, Nishimura, N, Hartogh, J W D, Rauscher, T, Murphy, A S J & Cristallo, S 2018, ' Uncertainties in s-process nucleosynthesis in low-mass stars determined from Monte Carlo variations ', Monthly Notices of the Royal Astronomical Society, vol. 478, no. 3, pp. 4101-4127 . https://doi.org/10.1093/mnras/sty1185
The main s-process taking place in low mass stars produces about half of the elements heavier than iron. It is therefore very important to determine the importance and impact of nuclear physics uncertainties on this process. We have performed extensi
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::068cce92523a95e37f9763eb5b5c48d1
https://eprints.keele.ac.uk/4897/1/11052018_hirschi_sty1185.pdf
https://eprints.keele.ac.uk/4897/1/11052018_hirschi_sty1185.pdf