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20132026
most citedOn stellar-mass black hole mergers in AGN disks detectable with LIGO

296 citations · 753 across the 27 of their papers we have counts for

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19 papers · 1 filter

astro-ph.HE2026

Recoil-regulated extreme mass-ratio inspirals in AGN disks

LingQin Xue, Zoltán Haiman, Hiromichi Tagawa +1

Extreme mass-ratio inspirals (EMRIs) are among the primary targets of future space-based gravitational-wave observatories, such as LISA, TianQin, and Taiji. Active galactic nucleus…

astro-ph.HE2026

High-Spin BBH Subpopulation from AGN Accretion

I. Bartos, Z. Haiman

The formation environments of merging binary black holes remain uncertain. While hierarchical assembly in dense stellar clusters has been widely explored as an explanation for blac…

astro-ph.HE2026

Properties of black hole mergers in disks of active galactic nuclei

Hiromichi Tagawa, Zoltán Haiman, Bence Kocsis

Ground-based gravitational wave (GW) observatories have detected approximately 200 binary black hole (BH) mergers. The astrophysical origin of these events are debated, with eviden…

astro-ph.HE2026

Electromagnetic Flares from Compact-Object Mergers in AGN Disks: Signatures and Predictions

Hiromichi Tagawa, Zoltán Haiman, Shigeo S. Kimura +2

Accretion disks in active galactic nuclei (AGN) are promising sites for mergers of stellar-mass black holes (BHs) detectable via gravitational waves (GWs). These environments facil…

astro-ph.HE2025

Self-lensing flares from black hole binaries V: systematic searches in LSST

Kevin Park, Zoltan Haiman, Chengcheng Xin +3

The Vera C. Rubin Observatory has now seen first light, and over a 10 year duration, LSST is projected to catalogue tens of millions of quasars, many of which are expected to be as…

astro-ph.HE2025

Reconstructing the origin of black hole mergers using sparse astrophysical models

V. Gayathri, Giuliano Iorio, Hiromichi Tagawa +8

The astrophysical origin of binary black hole mergers discovered by LIGO and Virgo remains uncertain. Efforts to reconstruct the processes that lead to mergers typically rely on ei…

astro-ph.HE2025

Triples as Links between Binary Black Hole Mergers, their Electromagnetic Counterparts, and Galactic Black Holes

Smadar Naoz, Zoltan Haiman, Eliot Quataert +1

We propose a formation pathway linking black holes (BHs) observed in gravitational-wave (GW) mergers, wide BH-stellar systems uncovered by Gaia, and accreting low-mass X-ray binari…

astro-ph.HE2025★ 2 cited

Accretion is All You Need: Black Hole Spin Alignment in Merger GW231123 Indicates Accretion Pathway

Imre Bartos, Zoltan Haiman

GW231123 represents the most massive binary-black-hole merger detected to date, lying firmly within, or even above, the pair-instability mass gap. The component spins are both exce…

astro-ph.HE2025★ 11 cited

What Determines the Maximum Mass of AGN-assisted Black Hole Mergers?

LingQin Xue, Hiromichi Tagawa, Zoltan Haiman +1

The origin of merging binary black holes detected through gravitational waves remains a fundamental question in astrophysics. While stellar evolution imposes an upper mass limit of…

astro-ph.HE2025★ 2 cited

Thermal X-ray signatures in late-stage unequal-mass massive black hole binary mergers

Luke Major Krauth, Jordy Davelaar, Zoltán Haiman +3

The multi-messenger combination of gravitational waves (GWs) from merging massive black hole binaries (MBHBs) and the electromagnetic (EM) counterpart from the surrounding circumbi…

astro-ph.HE2024

Self-lensing flares from black hole binaries IV: the number of detectable shadows

Kevin Park, Chengcheng Xin, Jordy Davelaar +1

Sub-parsec supermassive black hole (SMBH) binaries are expected to be common in active galactic nuclei (AGN), as a result of the hierarchical build-up of galaxies via mergers. Whil…

astro-ph.HE2024

Time-dependent models of AGN disks with radiation from embedded stellar-mass black holes

Marguerite Epstein-Martin, Hiromichi Tagawa, Zoltan Haiman +1

The brightest steady sources of radiation in the universe, active galactic nuclei (AGN), are powered by gas accretion onto a central supermassive black hole (SMBH). The large sizes…

astro-ph.HE2023★ 2 cited

Shock cooling and breakout emission for optical flares associated with gravitational wave events

Hiromichi Tagawa, Shigeo S. Kimura, Zoltán Haiman +2

The astrophysical origin of stellar-mass black hole (BH) mergers discovered through gravitational waves (GWs) is widely debated. Mergers in the disks of active galactic nuclei (AGN…

astro-ph.HE2023★ 4 cited

Black Hole Binaries in AGN Accretion Discs II: Gas Effects on Black Hole Satellite Scatterings

Connar Rowan, Henry Whitehead, Tjarda Boekholt +2

The black hole (BH) binaries in active galactic nuclei (AGN) are expected to form mainly through scattering encounters in the ambient gaseous medium. Recent simulations, including…

astro-ph.HE2020★ 35 cited

Cosmic Evolution of Stellar-mass Black Hole Merger Rate in Active Galactic Nuclei

Y. Yang, I. Bartos, Z. Haiman +3

Binary black hole mergers encode information about their environment and the astrophysical processes that led to their formation. Measuring the redshift dependence of their merger…

astro-ph.HE2019★ 41 cited

GW170817A as a Hierarchical Black Hole Merger

V. Gayathri, I. Bartos, Z. Haiman +4

Despite the rapidly growing number of stellar-mass binary black hole mergers discovered through gravitational waves, the origin of these binaries is still not known. In galactic ce…

astro-ph.HE2019★ 283 cited

Hierarchical Black Hole Mergers in Active Galactic Nuclei

Yang Yang, Imre Bartos, V. Gayathri +8

The origins of the stellar-mass black hole mergers discovered by LIGO/Virgo are still unknown. Here we show that, if migration traps develop in the \add{accretion} disks of Active…

astro-ph.HE2017★ 296 cited

On stellar-mass black hole mergers in AGN disks detectable with LIGO

B. McKernan, K. E. S. Ford, J. Bellovary +9

Black hole mergers detectable with LIGO can occur in active galactic nucleus (AGN) disks. Here we parameterize the merger rates, the mass spectrum and the spin spectrum of black ho…

astro-ph.HE2013★ 56 cited

Ripple effects & oscillations in the broad FeKa line as a probe of massive black hole mergers

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

(abridged) When a sufficiently massive satellite (or secondary) black hole is embedded in a gas disk around a (primary) supermassive black hole, it can open an empty gap in the dis…