Hans-Thomas Janka

TL;DR: In this paper, relativistic smoothed particle hydrodynamic simulations with conformally flat approximation of the Einstein field equations and a physical, non-zero temperature equation of state are presented.

TL;DR: In this article, the uncertainties involved in supernova dynamics as well as in nuclear data inputs affect the nup-process in the neutrino-driven winds, and the sensitivity to the rates relevant to the breakout from the pp-chain region (A < 12), to the (n, p) rates on heavy nuclei, and to the nuclear masses along the nUP-process pathway is tested.

TL;DR: In this article, the authors examine the flow dynamics in the neighborhood of explosion by means of parametric two-dimensional, time-dependent hydrodynamic simulations for which the linear stability properties are well understood.

TL;DR: In this article, the neutrino emission properties of binary neutron star mergers were investigated using one hydrodynamical simulation. But the authors only considered the neutrinuclear emission properties and did not consider the effect of neutrinos' oscillations on the kilonova lightcurves.

TL;DR: In this paper, the authors performed three-dimensional relativistic hydrodynamical simulations of the coalescence of strange stars and explore the possibility to decide on the strange matter hypothesis by means of gravitational-wave measurements.