Tidal disruption jets as the source of Ultra-High Energy Cosmic Rays
arXiv:1411.0704
Abstract
Observations of the spectacular, blazar-like tidal disruption event (TDE) candidates Swift J1644+57 and J2058+05 show that the conditions required for accelerating protons to 10^{20} eV appear to be realized in the outer jet, and possibly in the inner jet as well. Direct and indirect estimates of the rate of jetted-TDEs, and of the energy they inject, are compatible with the observed flux of ultra-high energy cosmic rays (UHECRs) and the abundance of presently contributing sources. Thus TDE-jets can be a major source of UHECRs, even compabile with a pure proton composition.
Cited by in corpus (4)
- Ultra-High-Energy Cosmic Rays: The Intersection of the Cosmic and Energy Frontiers
- The Astrophysical Multimessenger Observatory Network (AMON): Performance and Science Program
- Particle Acceleration in Mildly Relativistic Outflows of Fast Energetic Transient Sources
- Multi-messenger signatures of delayed choked jets in tidal disruption events