activity
20072024
most citedElectron-capture supernovae as the origin of elements beyond iron

278 citations · 2.3k across the 23 of their papers we have counts for

collaborators
Showing 2020Show all

6 papers · 1 filter

astro-ph.HE2020★ 40 cited

The chemical signature of jet-driven hypernovae

J. J. Grimmett, Bernhard Müller, Alexander Heger +2

Hypernovae powered by magnetic jets launched from the surface of rapidly rotating millisecond magnetars are one of the leading models to explain broad-lined Type Ic supernovae (SNe…

astro-ph.SR2020★ 11 cited

Stochastic Core Spin-Up in Massive Stars -- Implications of 3D Simulations of Oxygen Shell Burning

L. O. McNeill, B. Müller

It has been suggested based on analytic theory that even in non-rotating supernova progenitors stochastic spin-up by internal gravity waves (IGWs) during the late burning stages ca…

astro-ph.SR2020★ 197 cited

Hydrodynamics of core-collapse supernovae and their progenitors

B. Müller

Multi-dimensional fluid flow plays a paramount role in the explosions of massive stars as core-collapse supernovae. In recent years, three-dimensional (3D) simulations of these phe…

astro-ph.HE2020★ 124 cited

Simple recipes for compact remnant masses and natal kicks

Ilya Mandel, Bernhard Müller

Based on recent results from three-dimensional supernova simulations and semi-analytical parametrised models, we develop analytical prescriptions for the dependence of the mass of…

astro-ph.HE2020★ 24 cited

A Novel Multi-Dimensional Boltzmann Neutrino Transport Scheme for Core-Collapse Supernovae

Conrad Chan, Bernhard Mueller

We introduce a new discrete-ordinate scheme for solving the general relativistic Boltzmann transport equation in the context of core-collapse supernovae. Our algorithm avoids the n…

astro-ph.HE2020★ 125 cited

Three-dimensional core-collapse supernova simulations of massive and rotating progenitors

Jade Powell, Bernhard Müller

We present three-dimensional simulations of the core-collapse of massive rotating and non-rotating progenitors performed with the general relativistic neutrino hydrodynamics code C…