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The impact of non-dipolar magnetic fields in core-collapse supernovae
M. Bugli, J. Guilet, M. Obergaulinger +2
The magnetic field is believed to play an important role in at least some core-collapse supernovae if its magnitude reaches , which is a typical value for a magnet…
Model comparison from LIGO-Virgo data on GW170817's binary components and consequences for the merger remnant
The LIGO Scientific Collaboration, the Virgo Collaboration, B. P. Abbott +1191
GW170817 is the very first observation of gravitational waves originating from the coalescence of two compact objects in the mass range of neutron stars, accompanied by electromagn…
Non-linear dynamics of spinning bosonic stars: formation and stability
N. Sanchis-Gual, F. Di Giovanni, M. Zilhão +4
We perform numerical evolutions of the fully non-linear Einstein-(complex, massive)Klein-Gordon and Einstein-(complex)Proca systems, to assess the formation and stability of spinni…
Universal relations for gravitational-wave asteroseismology of proto-neutron stars
Alejandro Torres-Forné, Pablo Cerdá-Durán, Martin Obergaulinger +2
State-of-the-art numerical simulations of core-collapse supernovae reveal that the main source of gravitational waves is the excitation of proto-neutron star modes during post-boun…