114 citations · 443 across the 12 of their papers we have counts for
12 papers
The Next Generation Global Gravitational Wave Observatory: The Science Book
Vicky Kalogera, B. S. Sathyaprakash, Matthew Bailes +88
The next generation of ground-based gravitational-wave detectors will observe coalescences of black holes and neutron stars throughout the cosmos, thousands of them with exceptiona…
Gravitational waves from three-dimensional core-collapse supernova models: The impact of moderate progenitor rotation
H. Andresen, E. Müller, H. -Th. Janka +3
We present predictions for the gravitational-wave (GW) emission of three-dimensional supernova (SN) simulations performed for a 15 solar-mass progenitor with the Prometheus-Vertex…
Emission line models for the lowest-mass core collapse supernovae. I: Case study of a 9 one-dimensional neutrino-driven explosion
A. Jerkstrand, T. Ertl, H. -T. Janka +3
A large fraction of core-collapse supernovae (CCSNe), 30-50%, are expected to originate from the low-mass end of progenitors with . However, degeneracy…
Magneto-elastic oscillations modulating the emission of magnetars
Michael Gabler, Pablo Cerdá-Durán, Alexei Mate +3
Magneto-elastic oscillations of neutron stars are believed to explain observed quasi-periodic oscillations (QPOs) in the decaying tail of the giant flares of highly magnetized neut…
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…
On the maximum magnetic field amplification by the magnetorotational instability in core-collapse supernovae
Tomasz Rembiasz, Jérôme Guilet, Martin Obergaulinger +3
Whether the magnetorotational instability (MRI) can amplify initially weak magnetic fields to dynamically relevant strengths in core collapse supernovae is still a matter of active…