158 citations · 1.8k across the 46 of their papers we have counts for
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Papaloizou-Pringle instability suppression by the magnetorotational instability in relativistic accretion discs
Matteo Bugli, Jérôme Guilet, Ewald Müller +3
Geometrically thick tori with constant specific angular momentum have been widely used in the last decades to construct numerical models of accretion flows onto black holes. Such d…
Magnetorotational Instability in Core-Collapse Supernovae
Tomasz Rembiasz, Martin Obergaulinger, Jérôme Guilet +3
We discuss the relevance of the magnetorotational instability (MRI) in core-collapse supernovae (CCSNe). Our recent numerical studies show that in CCSNe, the MRI is terminated by p…
How to form a millisecond magnetar? Magnetic field amplification in protoneutron stars
Jerome Guilet, Ewald Mueller, Hans-Thomas Janka +4
Extremely strong magnetic fields of the order of are required to explain the properties of magnetars, the most magnetic neutron stars. Such a strong magnetic fie…
Are pulsars spun up or down by SASI spiral modes?
Rémi Kazeroni, Jérôme Guilet, Thierry Foglizzo
Pulsars may either be spun up or down by hydrodynamic instabilities during the supernova explosion of massive stars. Besides rapidly-rotating cases related to bipolar explosions, s…