activity
20112015
most citedNeutrino-driven explosion of a 20 solar-mass star in three dimensions enabled by strange-quark contributions to neutrino-nucleon scattering

260 citations · 1.3k across the 10 of their papers we have counts for

collaborators

10 papers

astro-ph.SR2015★ 126 cited

Progenitor-dependent Explosion Dynamics in Self-consistent, Axisymmetric Simulations of Neutrino-driven Core-collapse Supernovae

Alexander Summa, Florian Hanke, Hans-Thomas Janka +3

We present self-consistent, axisymmetric core-collapse supernova simulations performed with the Prometheus-Vertex code for 18 pre-supernova models in the range of 11-28 solar masse…

astro-ph.SR2015★ 260 cited

Neutrino-driven explosion of a 20 solar-mass star in three dimensions enabled by strange-quark contributions to neutrino-nucleon scattering

Tobias Melson, Hans-Thomas Janka, Robert Bollig +3

Interactions with neutrons and protons play a crucial role for the neutrino opacity of matter in the supernova core. Their current implementation in many simulation codes, however,…

astro-ph.SR2014★ 155 cited

Neutrino emission characteristics and detection opportunities based on three-dimensional supernova simulations

Irene Tamborra, Georg Raffelt, Florian Hanke +2

The neutrino emission characteristics of the first full-scale three-dimensional supernova simulations with sophisticated three-flavor neutrino transport for three models with masse…

physics.comp-ph2014★ 1 cited

Towards Petaflops Capability of the VERTEX Supernova Code

Andreas Marek, Markus Rampp, Florian Hanke +1

The VERTEX code is employed for multi-dimensional neutrino-radiation hydrodynamics simulations of core-collapse supernova explosions from first principles. The code is considered s…

astro-ph.SR2014★ 179 cited

Self-sustained asymmetry of lepton-number emission: A new phenomenon during the supernova shock-accretion phase in three dimensions

Irene Tamborra, Florian Hanke, Hans-Thomas Janka +3

During the stalled-shock phase of our 3D hydrodynamical core-collapse simulations with energy-dependent, 3-flavor neutrino transport, the lepton-number flux (nue minus antinue) eme…

astro-ph.SR2013★ 118 cited

Neutrino signature of supernova hydrodynamical instabilities in three dimensions

Irene Tamborra, Florian Hanke, Bernhard Mueller +2

The first full-scale three-dimensional (3D) core-collapse supernova (SN) simulations with sophisticated neutrino transport show pronounced effects of the standing accretion shock i…

astro-ph.SR2013★ 228 cited

SASI Activity in Three-Dimensional Neutrino-Hydrodynamics Simulations of Supernova Cores

F. Hanke, B. Mueller, A. Wongwathanarat +2

The relevance of the standing accretion shock instability (SASI) compared to neutrino-driven convection in three-dimensional (3D) supernova-core environments is still highly contro…

astro-ph.SR2012★ 5 cited

Core-Collapse Supernovae: Reflections and Directions

H. -Thomas Janka, Florian Hanke, Lorenz Huedepohl +3

Core-collapse supernovae are among the most fascinating phenomena in astrophysics and provide a formidable challenge for theoretical investigation. They mark the spectacular end of…

astro-ph.SR2011★ 4 cited

Core-Collapse Supernovae: Explosion Dynamics, Neutrinos and Gravitational Waves

Bernhard Mueller, Hans-Thomas Janka, Andreas Marek +3

The quest for the supernova explosion mechanism has been one of the outstanding challenges in computational astrophysics for several decades. Simulations have now progressed to a s…

astro-ph.SR2011★ 221 cited

Is Strong SASI Activity the Key to Successful Neutrino-Driven Supernova Explosions?

Florian Hanke, Andreas Marek, Bernhard Mueller +1

Following a simulation approach of recent publications we explore the viability of the neutrino-heating explosion mechanism in dependence on the spatial dimension. Our results disa…