Shu-Rui Zhang, Yu Wang, Ye-Fei Yuan, Hiromichi Tagawa, Yun-Feng Wei, Liang Li, Rong-Gen Cai

Recently, the gravitational wave (GW) event for black hole (BH)-BH mergers, S241125n, has been reported to be associated with a short gamma-ray burst (GRB) and X-ray afterglow emission. Such an association could potentially unveil the environments of mergers and provide attractive targets for multi-messenger observations. We summarize these observations and model it as a binary BH merger occurring within an active galactic nucleus (AGN), where the merger remnant accretes disk material at hyper-Eddington rates. The resulting jet could lead to the GRB associated with the GW event. The GRB, detected by Swift-BAT, exhibits a Comptonized spectrum with an unusually soft photon index, which is consistent with emission from the jet interacting the emission associated with the dense AGN disk environment. Its X-ray afterglow shows an unusually hard spectrum, indicating possible strong absorption by a high column density typical of AGN disks. We highlight the importance of identifying the host galaxy and conducting more sensitive infrared observations to test the model.