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SUMMARY:Particle acceleration observed in gamma-rays
DTSTART;VALUE=DATE-TIME:20151027T073000Z
DTEND;VALUE=DATE-TIME:20151027T075500Z
DTSTAMP;VALUE=DATE-TIME:20260912T235643Z
UID:indico-contribution-942@indico.icrr.u-tokyo.ac.jp
DESCRIPTION:Speakers: Rolf Buehler (DESY\,)\nGamma-rays give us a view on 
 the acceleration some of the most energetic particles in the universe. The
 se particles are usually thought to be accelerated in (relativistic) shock
 s. However\, with the advances in Particle In Cell simulations over the pa
 st years it became clear that magnetic reconnection is also a compelling a
 lternative. In this talk\, I will discuss what gamma-ray observations can 
 tell us about these two options. I will discuss this question for differen
 t gamma-ray source classes\, as Supernova Remnants\, Jets of Active Galact
 ic Nuclei and Pulsar Wind Nebulae.\n\nhttps://indico.icrr.u-tokyo.ac.jp/ev
 ent/23/contributions/942/
LOCATION: Room 5.6
URL:https://indico.icrr.u-tokyo.ac.jp/event/23/contributions/942/
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