22–25 Jan 2019
Padova
Europe/Rome timezone

Implications of the observation of high-energy neutrinos in the direction of TXS 0506+056

24 Jan 2019, 11:30
30m
Polo di Psicologia - room 3I (3rd floor, building 2) (Padova)

Polo di Psicologia - room 3I (3rd floor, building 2)

Padova

Via Venezia, 12-14 Padova
Talk Main track Connection to neutrinos

Speaker

Dr Foteini Oikonomou (ESO)

Description

The IceCube Collaboration recently announced the detection of a high-energy astrophysical neutrino consistent with arriving from the direction of the blazar TXS 0506+056 during an energetic gamma-ray flare, and a “neutrino flare” from the same direction during 2014-15. I will present some of the inferences drawn from these observations for neutrino emission from TXS 0506+056, in light of the characteristics of this source. Additionally, implications for neutrinos from blazar flares in general will be presented.

Primary author

Dr Foteini Oikonomou (ESO)

Presentation materials