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SUMMARY:Constraints on cosmic ray propagation and magnetic fields using ga
 mma-ray observations
DTSTART;VALUE=DATE-TIME:20191113T053000Z
DTEND;VALUE=DATE-TIME:20191113T060000Z
DTSTAMP;VALUE=DATE-TIME:20250110T182855Z
UID:indico-contribution-1661@indico.icrr.u-tokyo.ac.jp
DESCRIPTION:Speakers: Rubén López-Coto (INFN Padova)\nThe origin and pro
 pagation of cosmic rays is one of the most important questions in astropar
 ticle physics nowadays. To perform Indirect searches of Dark Matter search
 ing for their products in the local cosmic ray spectra\, we first need to 
 comprehend what is the background coming from astrophysical sources. We ca
 n only model this background by achieving a deep understanding of cosmic r
 ay propagation. Although the transport of these cosmic rays through the ga
 laxy make them lose the information about their origin due to interstellar
  magnetic fields\, we can directly study the properties of their propagati
 on using gamma rays. In this talk\, I will give a review of current measur
 ements of magnetic fields and cosmic ray propagation parameters using gamm
 a rays.\n\nhttps://indico.icrr.u-tokyo.ac.jp/event/259/contributions/1661/
LOCATION:Remote talk
URL:https://indico.icrr.u-tokyo.ac.jp/event/259/contributions/1661/
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