The r-process nucleosynthesis in core-collapse supernovae (CC-SNe) is studied, with a
focus on the explosion scenario induced by rotation and strong magnetic fields …

Magnetorotational supernovae are a rare type of core-collapse supernovae where the
magnetic field and rotation play a central role in the dynamics of the explosion. We present …

We calculate nucleosynthesis in core collapse explosions of massive Population III stars and
compare the results with abundances of metal-poor halo stars to constrain the parameters of …

Measurements of high-energy photons from cosmic sources of nuclear radiation through
ESA's INTEGRAL mission have advanced our knowledge: new data with high spectral …

Core-collapse supernovae are among the most energetic explosions in the universe
marking the catastrophic end of massive stars. In spite of rigorous studies for several …

Core‐collapse supernovae are dramatic explosions marking the catastrophic end of
massive stars. The only means to get direct information about the supernova engine is from …

The spatial and velocity distributions of nuclear species synthesized in the innermost
regions of core-collapse supernovae can yield important clues about explosion asymmetries …

We have performed two-dimensional simulations of core collapse supernovae that
encompass shock revival by neutrino heating, neutrino-driven convection, explosive …

We present the results of nucleosynthesis calculations based on multi-dimensional (2D and
3D) hydrodynamical simulations of the thermonuclear burning phase in type Ia supernovae …

Aspherical explosion models for the hypernova (hyperenergetic supernova) SN 1998bw are
presented. Nucleosynthesis in aspherical explosions is examined with a two-dimensional …