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Cited by 194 publications
(344 citation statements)
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“…This could occur via collective neutrino oscillations [56]. However, the neutrino spectra become very similar for all neutrino flavours during the wind phase [13] and thus no big increase of the electron antineutrino energies is expected in this way. Notice that this high energy could be important in proton-rich conditions for the νp-process [57].…”
Section: Neutrino Oscillationsmentioning
confidence: 99%
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“…This could occur via collective neutrino oscillations [56]. However, the neutrino spectra become very similar for all neutrino flavours during the wind phase [13] and thus no big increase of the electron antineutrino energies is expected in this way. Notice that this high energy could be important in proton-rich conditions for the νp-process [57].…”
Section: Neutrino Oscillationsmentioning
confidence: 99%
“…Improvements in the neutrino reactions have resulted in a reduction of the electron antineutrino energy from the first simulations by Wilson to the modern ones [13,12]. Moreover, all neutrino flavours have very similar energies which leads to proton-rich conditions since the requirement ǫν e − ǫ νe 4∆ ≈ 5 MeV is not fulfilled.…”
Section: Weak Interactions: Electron Fractionmentioning
confidence: 99%
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“…Although the original formulation was quite successful [23], it has been shown [24,25] that the desired conditions of high entropy and neutron-rich composition [4] do not occur in the neutrino energized wind. Nevertheless, it is quite likely that the so-called "weak r-process" occurs in the NDW producing neutron rich nuclei up to about A ∼ 125 [26,27].…”
Section: Current Models For the R-processmentioning
confidence: 99%