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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…
Optimal neutron-star mass ranges to constrain the equation of state of nuclear matter with electromagnetic and gravitational-wave observations
Lukas R. Weih, Elias R. Most, Luciano Rezzolla
Exploiting a very large library of physically plausible equations of state (EOSs) containing more than members and yielding more than stellar models, we conduct a…
Using gravitational-wave observations and quasi-universal relations to constrain the maximum mass of neutron stars
Luciano Rezzolla, Elias R. Most, Lukas R. Weih
Combining the GW observations of merging systems of binary neutron stars and quasi-universal relations, we set constraints on the maximum mass that can be attained by nonrotating s…