Ultra-high-energy-cosmic-ray hot spots from tidal disruption events

Abstract

We consider the possibility that tidal disruption events (TDEs) caused by supermassive black holes (SMBHs) in nearby galaxies can account for the ultra-high-energy cosmic-ray (UHECR) hotspot reported recently by the Telescope Array (TA) and the warm spot by Pierre Auger Observatory (PAO). We describe the expected cosmic-ray signal from a TDE and derive the constraints set by the timescale for dispersion due to intergalactic magnetic fields and the accretion time of the SMBH. We find that TDEs in M82 can explain the hotspot detected by the TA regardless of whether the UHECRs are composed of protons or heavier nuclei. We then check for consistency of the hot and warm spots from M82 and Cen A with the full-sky isotropic signal from all SMBHs within the GZK radius. This analysis applies to any scenario in which the hot/warm spots are real and due to M82 and Cen A, regardless of whether TDEs are the source of UHECRs. We find that the isotropic flux implied by the luminosity density inferred from M82 and Cen A is bigger than that observed by roughly an order of magnitude, but we provide several possible explanations, including the possibility of a local overdensity and the possibility of intermediate-mass nuclei in UHECRs, to resolve the tension.

6 pages; major revisions

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• High-energy cosmic ray nuclei from tidal disruption events: Origin, survival, and implications
• Multiwavelength follow-up of a rare IceCube neutrino multiplet
• Neutrino Emissions from Tidal Disruption Remnants
• Can we observe neutrino flares in coincidence with explosive transients?
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• White paper on EUSO-SPB2
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• Ultrahigh-Energy Cosmic Ray Composition from the Distribution of Arrival Directions
• What is the nature and origin of the highest-energy particles in the universe?
• Exploring the superwind mechanism for generating ultrahigh-energy cosmic rays using large-scale modeling of starbursts
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• Treasure Maps for Detections of Extreme Energy Cosmic Rays
• Case for Centaurus A as the main source of ultrahigh-energy cosmic rays
• Evidence for UHECR origin in starburst galaxies
• Past, Present and Future of UHECR Observations