p-process fluxes

This tool shows the nucleosynthesis fluxes to and from an isotope of your choice during a Supernova type II.
The sum of all production fluxes is normalized to 100%, and the destruction fluxes are scaled with the same factor.
Fluxes smaller than 1% are not shown.

More details and further references can be found in:

K. Göbel, J. Glorius, A. Koloczek, M. Pignatari, R. Reifarth, R. Schach, K. Sonnabend, and the NuGrid collaboration
"Nucleosynthesis simulations for the production of the p-nuclei ⁹²Mo and ⁹⁴Mo in a Supernova type II model"
Proceedings of the CGS-15, Technische Universität Dresden, August 25-29, 2014.
European Physical Journal Web of Conferences 93, 3006 (2015)

One-dimensional SNII trajectories ("Hashimoto trajectories") as used in
W. Rapp, J. Görres, M. Wiescher, H. Schatz, and F. Käppeler. "Sensitivity of p-Process Nucleosynthesis to Nuclear Reaction Rates in a 25 M_solar Supernova Model."
(The Astrophysical Journal, 653:474–489, December 2006)