Probing the tidal disruption flares of massive black holes with high-energy neutrinos
Probing the tidal disruption flares of massive black holes with high-energy neutrinos
The recently discovered high-energy transient Swift J164449.3+573451 (Sw J1644+57) is thought to arise from the tidal disruption of a passing star by a dormant massive black hole. Modeling of the broadband emission suggests the presence of a powerful relativistic jet, which contributes dominantly to the observed X-ray emission. Here we …