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Cited article:

Proton vs. neutron captures in the neutrino winds of core-collapse supernovae

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The decompression of the outer neutron star crust and r-process nucleosynthesis

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Astronomy & Astrophysics 531 A78 (2011)
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What are the astrophysical sites for the r-process and the production of heavy elements?

F.-K. Thielemann, A. Arcones, R. Käppeli, et al.
Progress in Particle and Nuclear Physics 66 (2) 346 (2011)
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Formation of quark phases in protoneutron stars: The transition from the two-flavor color-superconducting phase to the normal quark phase

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Analysis of matter suppression in collective neutrino oscillations during the supernova accretion phase

Sovan Chakraborty, Tobias Fischer, Alessandro Mirizzi, Ninetta Saviano and Ricard Tomàs
Physical Review D 84 (2) (2011)
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No Collective Neutrino Flavor Conversions during the Supernova Accretion Phase

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Physical Review Letters 107 (15) (2011)
https://doi.org/10.1103/PhysRevLett.107.151101

TYPE Ia SUPERNOVAE AS SITES OF THEp-PROCESS: TWO-DIMENSIONAL MODELS COUPLED TO NUCLEOSYNTHESIS

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IMPACTS OF COLLECTIVE NEUTRINO OSCILLATIONS ON CORE-COLLAPSE SUPERNOVA EXPLOSIONS

Yudai Suwa, Kei Kotake, Tomoya Takiwaki, Matthias Liebendörfer and Katsuhiko Sato
The Astrophysical Journal 738 (2) 165 (2011)
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The influence of collective neutrino oscillations on a supernovarprocess

Huaiyu Duan, Alexander Friedland, Gail C McLaughlin and Rebecca Surman
Journal of Physics G: Nuclear and Particle Physics 38 (3) 035201 (2011)
https://doi.org/10.1088/0954-3899/38/3/035201

Neutrino Radiation-Hydrodynamics: General Relativistic versus Multidimensional Supernova Simulations

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Progress of Theoretical Physics Supplement 186 87 (2010)
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