High-energy Neutrinos from Choked Gamma-Ray Bursts in Active Galactic Nucleus Accretion Disks

Both long-duration gamma-ray bursts (LGRBs) from core collapse of massive stars and short-duration GRBs (SGRBs) mergers binary neutron star (BNS) or star--black hole (NSBH) are expected to occur in the accretion disk active galactic nuclei (AGNs). We show that GRB jets embedded migration traps AGN disks promised be choked by dense material. Efficient shock acceleration cosmic rays at reverse is expected, high-energy neutrinos would produced. find these sources can effectively produce detectable TeV--PeV through $p\gamma$ interactions. From a LGRB jet with isotropic equivalent energy $10^{53}\,{\rm erg}$ $100\,{\rm Mpc}$, one expects $\sim2\,(7)$ neutrino events IceCube (IceCube-Gen2). The contribution LGRBs observed diffuse background depends on unknown local event rate density disks. For example, if $\sim5\%$ low-luminosity $(\sim10\,{\rm Gpc}^{-3}\,{\rm yr}^{-1})$, contribute $\sim10\%$ background. Choked SGRBs potential for future joint electromagnetic, neutrino, gravitational wave multi-messenger observations.