Marco Pignatari
0000-0002-9048-6010
University of Hull
187 papers found
Refreshing results…
The reactions [sup 25]Mg(α,n)[sup 28]Si, [sup 26]Mg(α,n)[sup 29]Si and their possible impact on nucleosynthesis
Time-Scales of the s Process: from Minutes to Ages
Difficulties in Probing Nuclear Physics: A Study of $^{44}$Ti and $^{56}$Ni
Nucleosynthesis Calculations from Core-Collapse Supernovae
NuGrid: Toward High Precision Double-Degenerate Merger Simulations with SPH in 3D
Nucleosynthetic Yields from "Collapsars"
The s -Process in Massive Stars at Low Metallicity: The Effect of Primary 14 N from Fast Rotating Stars
Stellar (n, γ) cross sections for Br and Rb: Matching the weak and mains-process components
Mg24(α,γ)Si28resonance parameters at low α-particle energies
Neutron capture cross sections for the weaksprocess in massive stars
NuGrid: Nuclear Burning in 3-D Double Degenerate Merger Simulations
Spatial distribution of nucleosynthesis products in cassiopeia a: Comparison between observations and 3D explosion models
44Ti and 56Ni in core-collapse supernovae
Recent Results at ṉTOF and Future Perspectives
Abundances of Heavy Elements in PNe and AGB Model Predictions
Neutron reactions in massive stars and the origin of 60Fe
NuGrid: S process in massive stars
Complete nucleosynthesis calculations for low-mass stars from NuGrid
Nucleosynthesis simulations for a wide range of nuclear production sites from NuGrid
The hydrodynamic environment for the s process in the He-shell flash of AGB stars
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