299 citations · 839 across the 8 of their papers we have counts for
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The process in the light of an improved understanding of supernova neutrino spectra
A. Sieverding, G. Martínez-Pinedo, L. Huther +2
We study the neutrino-induced production of nuclides in explosive supernova nucleosynthesis for progenitor stars with solar metallicity including neutrino nucleus reactions for all…
Expected impact from weak reactions with light nuclei in core-collapse supernova simulations
T. Fischer, G. Martínez-Pinedo, M. Hempel +4
We study the role of light nuclear clusters in simulations of core-collapse supernovae. Expressions for the reaction rates are developed for a large selection of charged current ab…
Neutrino Nucleosynthesis of radioactive nuclei in supernovae
A. Sieverding, L. Huther, K. Langanke +2
We study the neutrino-induced production of nuclides in explosive supernova nucleosynthesis for progenitor stars with solar metallicity and initial main sequence masses between 15…
Effects of neutrino oscillations on nucleosynthesis and neutrino signals for an 18 M supernova model
Meng-Ru Wu, Yong-Zhong Qian, Gabriel Martinez-Pinedo +2
In this paper, we explore the effects of neutrino flavor oscillations on supernova nucleosynthesis and on the neutrino signals. Our study is based on detailed information about the…
Supernova neutrinos and nucleosynthesis
G. Martínez-Pinedo, T. Fischer, L. Huther
Observations of metal-poor stars indicate that at least two different nucleosynthesis sites contribute to the production of r-process elements. One site is responsible for the prod…
Impact of active-sterile neutrino mixing on supernova explosion and nucleosynthesis
Meng-Ru Wu, Tobias Fischer, Lutz Huther +2
We show that for the active-sterile flavor mixing parameters suggested by the reactor neutrino anomaly, substantial \ν_e-\ν_s and \bar \ν_e-\bar \ν_s conversion occurs in regions w…
Charged-current weak interaction processes in hot and dense matter and its impact on the spectra of neutrinos emitted from proto-neutron star cooling
G. Martínez-Pinedo, T. Fischer, A. Lohs +1
We have performed three-flavor Boltzmann neutrino transport radiation hydrodynamics simulations covering a period of 3 s after the formation of a protoneutron star in a core-collap…