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20172019
most citedUncertainties in the production of p nuclides in thermonuclear supernovae determined by Monte Carlo variations

53 citations · 53 across the 2 of their papers we have counts for

collaborators

5 papers

astro-ph.SR2019

Uncertainties in p-process nucleosynthesis from Monte Carlo variation of reaction rates

N. Nishimura, T. Rauscher, R. Hirschi +3

It has been suggested that a p process can occur when hot, dense, and proton-rich matter is expanding within a strong flux of anti-neutrinos. In such an environment, proton-rich…

astro-ph.SR2019

NuGrid stellar data set - III. Updated low-mass AGB models and s-process nucleosynthesis with metallicities Z=0.01, Z=0.02 and Z=0.03

Umberto Battino, Ashley Tattersall, Claudia Lederer-Woods +6

The production of the neutron-capture isotopes beyond iron that we observe today in the solar system is the result of the combined contribution of the r-process, the s- process and…

astro-ph.SR2018

Uncertainties in s-process nucleosynthesis in low mass stars determined from Monte Carlo variations

G. Cescutti, R. Hirschi, N. Nishimura +4

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 nu…

astro-ph.SR201753 cited

Uncertainties in the production of p nuclides in thermonuclear supernovae determined by Monte Carlo variations

N. Nishimura, T. Rauscher, R. Hirschi +3

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 nuclides. Such…

astro-ph.SR2017

The s-process nucleosynthesis: impact of the uncertainties in the nuclear physics determined by Monte Carlo variations

G. Cescutti, N. Nishimura, R. Hirschi +3

We investigated the impact of uncertainties in neutron-capture and weak reactions (on heavy elements) on the s-process nucleosynthesis in low-mass stars and massive stars using a M…