Cut from a different cloth: Binary black holes in the mass gap
Gravitational-wave observations of black holes with rare masses may reveal their unique origin stories.
Gravitational-wave observations of black holes with rare masses may reveal their unique origin stories.
Black hole mergers may have more dance moves than we thought—recoil kicks create intricate spin distributions for black holes from hierarchical mergers.
Stars of various temperatures and sizes slow down at different rates– and to different extents. The authors of this paper address this distinction in a regime never before addressed observationally.
The latest pair of merging black holes announced by LIGO-Virgo, the first made public from their latest observing run, is unlike any seen before.
All of the black hole mergers we’ve seen so far with LIGO/Virgo have surprised us with their mass-spin relationship. Are we misunderstanding stellar collapse? Or is there something even more exotic going on?
A variety of mechanisms cause stars to experience spin evolution. Can we learn about planet formation by pushing spin measurements down to substellar masses?