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Nucleosynthesis of elements between Sr and Ag in neutron- and proton-rich neutrino-driven winds
A. Arcones, J. Bliss
Neutrino-driven winds that follow core collapse supernovae were thought to be the site where half of the heavy elements are produced by the r-process. Although recent hydrodynamic…
X-ray Decay Lines from Heavy Nuclei in Supernova Remnants as a Probe of the r-Process Origin and the Birth Periods of Magnetars
Justin L. Ripley, Brian D. Metzger, Almudena Arcones +1
The origin of rapid neutron capture (r-process) nuclei remains one of the longest standing mysteries in nuclear astrophysics. Core collapse supernovae (SNe) and neutron star binary…
High resolution simulations of the head-on collision of white dwarfs
D. García-Senz, R. M. Cabezón, A. Arcones +2
The direct impact of white dwarfs has been suggested as a plausible channel for type Ia supernovae. In spite of their (a priori) rareness, in highly populated globular clusters and…
Approaching the precursor nuclei of the third r-process peak with RIBs
C. Domingo-Pardo, R. Caballero-Folch, J. Agramunt +61
The rapid neutron nucleosynthesis process involves an enormous amount of very exotic neutron-rich nuclei, which represent a theoretical and experimental challenge. Two of the main…