Eli Livne

TL;DR: In this article, a 2.5D radiation-hydrodynamics simulation of the accretion-induced collapse (AIC) of white dwarfs is presented, starting from 2D rotational equilibrium configurations of a 1.46-M⊙ model.

TL;DR: In this article, the authors compute stellar evolution models for primordial ∼200 M_⊙ stars, simulating the implosion/explosion due to the pair-production instability, and use them as inputs for detailed non-local thermodynamic equilibrium time-dependent radiative transfer simulations.

TL;DR: In this article, a 2D discrete-ordinate (S_n) method was used to calculate the post-bounce phase of core-collapse supernovae using axisymmetric (2D) multiangle, multigroup neutrino radiation-hydrodynamic calculations.

TL;DR: In this paper, a 2D discrete-ordinate (S_n) method was used to simulate the post-bounce phase of core-collapse supernovae using axisymmetric (2D) multi-angle, multi-group neutrino radiation-hydrodynamic calculations.

TL;DR: In this article, the authors present results from an extensive set of one-and two-dimensional radiation-hydrodynamic simulations of the supernova core-collapse, bounce, and postbounce phases and focus on the proto-neutron star (PNS) spin periods and rotational profiles.