The location of the upper edge of the pair-instability supernovae black hole mass gap
Jeremy Sakstein, Djuna Croon
astro-ph.HE, astro-ph.CO, astro-ph.IM, astro-ph.SR, gr-qc
Submitted: 2026-06-30
Comments: Six pages, two figures
License: http://arxiv.org/licenses/nonexclusive-distrib/1.0/
Terminology
Sources
- Find the Gap: Black Hole Population Analysis with an Astrophysically Motivated Mass Function
- The Effect of Pair-Instability Mass Loss on Black Hole Mergers
- Rotating Massive Main-Sequence Stars I: Grids of Evolutionary Models and Isochrones
- Prediction of Multiple Features in the Black Hole Mass Function due to Pulsational Pair-Instability Supernovae
- Missing in Action: New Physics and the Black Hole Mass Gap
- Missing in Axion: where are XENON1T's big black holes?
- Can GW231123 have a stellar origin?
- Weak mixing angle at low energies
- Resolving The Peak Of The Black Hole Mass Spectrum
- Mind the gap: The location of the lower edge of the pair instability supernovae black hole mass gap
- Constraints from gravitational wave detections of binary black hole mergers on the $^{12}\rm{C}\left(\alpha,\gamma\right)^{16}\!\rm{O}$ rate
- The Black Hole Mass Gap as a New Probe of Millicharged Particles
- Minding the gap: GW190521 as a straddling binary
- The Impact of Neutrino Magnetic Moments on the Evolution of Massive Stars
- Modules for Experiments in Stellar Astrophysics (MESA): Time-Dependent Convection, Energy Conservation, Automatic Differentiation, and Infrastructure
- Observing intermediate-mass black holes and the upper--stellar-mass gap with LIGO and Virgo
- Modules for Experiments in Stellar Astrophysics (MESA)
- Modules for Experiments in Stellar Astrophysics (MESA): Giant Planets, Oscillations, Rotation, and Massive Stars
- Modules for Experiments in Stellar Astrophysics (MESA): Binaries, Pulsations, and Explosions
- Modules for Experiments in Stellar Astrophysics (MESA): Convective Boundaries, Element Diffusion, and Massive Star Explosions
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