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Fast ejecta as a potential way to distinguish black holes from neutron stars in high-mass gravitational-wave events
Elias R. Most, L. Jens Papenfort, Samuel Tootle +1
High-mass gravitational-wave events in the neutron-star mass range, such as GW190425, have recently started to be detected by the LIGO/Virgo detectors. If the masses of the two bin…
A lower bound on the maximum mass if the secondary in GW190814 was once a rapidly spinning neutron star
Elias R. Most, L. Jens Papenfort, Lukas R. Weih +1
The recent detection of GW190814 featured the merger of a binary with a primary having a mass of and a secondary with a mass of . While th…
The heavier the better: how to constrain mass ratios and spins of high-mass neutron-star mergers
Elias R. Most, Lukas R. Weih, Luciano Rezzolla
The first binary neutron-star merger event, GW170817, and its bright electromagnetic counterpart have provided a remarkable amount of information. By contrast, the second event, GW…
Electromagnetic precursors to gravitational wave events: Numerical simulations of flaring in pre-merger binary neutron star magnetospheres
Elias R. Most, Alexander A. Philippov
The detection of gravitational waves from neutron star merger events has opened up a new field of multi-messenger astronomy linking gravitational waves events to short-gamma ray bu…