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Nuclear Input for Core-collapse Models
G. Martinez-Pinedo, M. Liebendoerfer, D. Frekers
We review the nuclear physics input necessary for the study of the collapse of massive stars as precursor to supernova explosions. Recent theoretical advances for the calculation o…
The Innermost Ejecta of Core Collapse Supernovae
C. Fröhlich, P. Hauser, M. Liebendoerfer +5
We ensure successful explosions (of otherwise non-explosive models) by enhancing the neutrino luminosity via reducing the neutrino scattering cross sections or by increasing the he…
Parity-Dependence in the Nuclear Level Density
D. Mocelj, T. Rauscher, G. Martinez-Pinedo +4
Astrophysical reaction rates are sensitive to the parity distribution at low excitation energies. We combine a formula for the energy-dependent parity distribution with a microscop…
Neutral-current neutrino-nucleus cross-sections for A~50-65 nuclei
A. Juodagalvis, K. Langanke, G. Martinez-Pinedo +3
We study neutral current neutrino-nucleus reaction cross-sections for Mn, Fe, Co and Ni isotopes. An earlier study for a few selected nuclei has shown that in the supernova environ…
The Shell Model as Unified View of Nuclear Structure
E. Caurier, G. Martínez-Pinedo, F. Nowacki +2
The last decade has witnessed both quantitative and qualitative progresses in Shell Model studies, which have resulted in remarkable gains in our understanding of the structure of…
Supernova Inelastic Neutrino-Nucleus Cross Sections from High-Resolution Electron Scattering Experiments and Shell-Model Calculations
K. Langanke, G. Martínez-Pinedo, P. von Neumann-Cosel +1
Highly precise data on the magnetic dipole strength distributions from the Darmstadt electron linear accelerator for the nuclei 50Ti, 52Cr and 54Fe are dominated by isovector Gamow…