No optical counterpart was found for the black hole merger S231206cc, and the non-detection constrains AGN-disk BBH flare models to SMBH masses around 10^7 to 10^8 solar masses and radii of 0.01 to 0.1 parsec.
The Use of Binary Black Holes Merging in AGN Disks for Hubble Constant Measurements
1 Pith paper cite this work. Polarity classification is still indexing.
1
Pith paper citing it
abstract
We study the impact of environmental effects on the measurement of the Hubble constant ($H_0$) from gravitational wave (GW) observations of binary black hole mergers residing in active galactic nuclei (AGNs) near the central supermassive black hole. Using the potential hierarchical triple merger candidate GW190514-GW190521 in AGN J124942.3+344929 with its electromagnetic counterpart ZTF19abanrhr as a multimessenger case study, we demonstrate that environmental effects can be negligible for mergers at approximately tens to hundreds of Schwarzschild radii from the supermassive black hole. We find $H_0=40.9_{-8.9}^{+19.3}\,{\rm km\,s^{-1}\,Mpc^{-1}}$ (median and 68\% credible interval) under a flat prior and flat $\Lambda$CDM cosmology. Incorporating GW170817 prior information improves constraints to $H_0=68.8_{-6.0}^{+7.7}\,{\rm km\,s^{-1}\,Mpc^{-1}}$. We suggest that in general, AGN environments could serve as viable laboratories for cosmological studies from GW observations where environmental effects remain below detection thresholds.
fields
astro-ph.HE 1years
2025 1verdicts
CONDITIONAL 1representative citing papers
citing papers explorer
-
Long-Term Optical Follow Up of S231206cc: Multi-Model Constraints on BBH Merger Emission in AGN Disks
No optical counterpart was found for the black hole merger S231206cc, and the non-detection constrains AGN-disk BBH flare models to SMBH masses around 10^7 to 10^8 solar masses and radii of 0.01 to 0.1 parsec.