activity
20142024
most citedIntermediate mass black holes in AGN disks II. Model predictions & observational constraints

183 citations · 249 across the 9 of their papers we have counts for

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Showing astro-ph.HEShow all

6 papers · 1 filter

astro-ph.HE2024★ 9 cited

McFACTS II: Mass Ratio--Effective Spin Relationship of Black Hole Mergers in the AGN Channel

Harrison E. Cook, Barry McKernan, K. E. Saavik Ford +6

We use the Monte Carlo For AGN (active galactic nucleus) Channel Testing and Simulation (McFACTS, https://www.github.com/mcfacts/mcfacts) code to study the effect of AGN disk and n…

astro-ph.HE2024★ 17 cited

McFacts III: Compact binary mergers from AGN disks over an entire synthetic universe

Vera Delfavero, K. E. Saavik Ford, Barry McKernan +6

The Active Galactic Nuclei (AGN) channel for the formation of binary black hole (BBH) mergers has been previously studied as a potential formation channel for the merging compact b…

astro-ph.HE2024★ 2 cited

McFACTS I: Testing the LVK AGN channel with Monte Carlo For AGN Channel Testing & Simulation (McFACTS)

Barry McKernan, K. E. Saavik Ford, Harrison E. Cook +6

Active galactic nuclei (AGN) are a promising source of the binary black hole (BBH) mergers observed in gravitational waves with LIGO-Virgo-Kagra (LVK). Constraining the AGN channel…

astro-ph.HE2019★ 4 cited

AGN (and other) astrophysics with Gravitational Wave Events

K. E. Saavik Ford, Imre Bartos, Barry McKernan +14

The stellar mass binary black hole (sBBH) mergers presently detected by LIGO may originate wholly or in part from binary black hole mergers embedded in disks of gas around supermas…

astro-ph.HE2016★ 5 cited

On the resonant detonation of sub-Chandrasekhar mass white dwarfs during binary inspiral

B. McKernan, K. E. S. Ford

White dwarfs (WDs) are believed to detonate via explosive Carbon-fusion in a Type Ia Supernova when their temperature and/or density reach the point where Carbon is ignited in a ru…

astro-ph.HE2014★ 22 cited

Stars as resonant absorbers of gravitational waves

B. McKernan, K. E. S. Ford, B. Kocsis +1

Quadrupole oscillation modes in stars can resonate with incident gravitational waves (GWs), and grow non-linear at the expense of GW energy. Stars near massive black hole binaries…