3-10 August 2016
Chicago IL USA
US/Central timezone
There is a live webcast for this event.

Potential Sources of High-Energy Neutrinos (20' + 5')

5 Aug 2016, 11:55
Chicago 8 ()

Chicago 8

Sheraton Grand Chicago 301 East Water Street Chicago IL 60611 USA


Markus Ahlers


The recent observation of TeV-PeV neutrinos by IceCube has opened a new window to the high-energy Universe. These high-energy astrophysical neutrinos are expected to originate from cosmic-ray interactions with gas and radiation. The origin of the IceCube signal is presently unknown and various Galactic and extragalactic source candidates have been proposed. Multi-messenger studies can help to decipher the underlying mechanisms of particle acceleration, propagation and production. I will highlight in my talk various source scenarios and will discuss multi-messenger constraints from cosmic-ray and gamma-ray observations.

Primary author

Markus Ahlers

Presentation Materials

Your browser is out of date!

If you are using Internet Explorer, please use Firefox, Chrome or Edge instead.

Otherwise, please update your browser to the latest version to use Indico without problems.