Bernhard Mueller

Associate Professor

MONASH UNIVERSITY

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Articles (17)

Collaborators (6)

Ilya Mandel

MONASH UNIVERSITY

Stuart Sim

The Queen's University Belfast

UNITED KINGDOM

Jose Antonio Font Roda

Full Professor

University of Valencia

Emanuele Berti

Johns Hopkins University

UNITED STATES

Alexander Heger

MONASH UNIVERSITY

Thomas Tauris

Aalborg University

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Bernhard Mueller

Research Interests

Explore related searches

Contact this professor

Articles (17)

Collaborators (6)

Ilya Mandel

Stuart Sim

Jose Antonio Font Roda

Emanuele Berti

Alexander Heger

Thomas Tauris

Make your next move.

Bernhard Mueller

Research Interests

Explore related searches

Contact this professor

Articles (17)

Determining the core-collapse supernova explosion mechanism with current and future gravitational-wave observatories

The gravitational-wave emission from the explosion of a 15 solar mass star with rotation and magnetic fields

Nucleosynthesis in the Innermost Ejecta of Magnetorotational Supernova Explosions in Three Dimensions

Calibration of neutron star natal kick velocities to isolated pulsar observations

Light Curves of Type IIP Supernovae from Neutrino-driven Explosions of Red Supergiants Obtained by a Semianalytic Approach

Simulations of the Progenitors of Black Hole–Neutron Star Gravitational Wave Sources

Synthetic light curves and spectra from a self-consistent 2D simulation of an ultra-strippped supernova

Gravitational Waves from a Core g Mode in Supernovae as Probes of the High-Density Equation of State

3D simulations of magnetoconvection in a rapidly rotating supernova progenitor

Fallback onto kicked neutron stars and its effect on spin-kick alignment

3D simulations of strongly magnetized non-rotating supernovae: explosion dynamics and remnant properties

The role of the hadron-quark phase transition in core-collapse supernovae

Gravitational wave signals from 2D core–collapse supernova models with rotation and magnetic fields

Self-consistent 3D Supernova Models From −7 Minutes to +7 s: A 1-bethe Explosion of a ∼19 M ⊙ Progenitor

Differential rotation in a 3D simulation of oxygen shell burning

3D simulations of oxygen shell burning with and without magnetic fields

The final core collapse of pulsational pair instability supernovae

Collaborators (6)

Ilya Mandel

Stuart Sim

Jose Antonio Font Roda

Emanuele Berti

Alexander Heger

Thomas Tauris

Make your next move.