Search for High Energy Neutrinos from Infrared Flares
Teresa Pernice, Giacomo Sommani (for the IceCube Collaboration)

TL;DR
This study investigates whether infrared flares from accreting supermassive black holes are associated with high-energy neutrinos, using extensive WISE data and IceCube observations to assess potential correlations and detectability.
Contribution
It provides a comprehensive analysis of a large IR flare catalog against IceCube data, exploring neutrino emission potential and reevaluating previous correlations with improved datasets.
Findings
No significant neutrino excess found in stacking analysis.
Extended IR flare catalog increases sensitivity for neutrino detection.
Revised analysis of nuclear flares with updated IceCube alerts.
Abstract
IceCube has detected a diffuse flux of high-energy neutrinos, whose origin still remains uncertain. Accreting supermassive black holes (SMBHs) have been proposed as plausible sources of neutrinos. Candidate sources include AT2019dsg, which is likely a stellar tidal disruption event (TDE), and AT2019dfr, an AGN flare. Both present delayed emission in the IR band with respect to the optical signal. This emission can be interpreted as the reprocessing of X-rays to optical light of the flare by dust located in a torus around the SMBH. An additional study using an optically detected sample of 63 accretion flares revealed another candidate as a potential high-energy neutrino counterpart: AT2019aalc, which is also accompanied by a dust echo. However, follow-up stacking analysis of the 63 nuclear flares using the full IceCube data sample did not show any significant excess over background.…
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