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SUMMARY:Radiation from internal shocks in magnetized flows
DTSTART;VALUE=DATE-TIME:20070706T194500Z
DTEND;VALUE=DATE-TIME:20070706T194500Z
DTSTAMP;VALUE=DATE-TIME:20260615T114624Z
UID:indico-contribution-1141@cern.ch
DESCRIPTION:Speakers: Dr. MASTICHIADIS\, Apostolos (Physics Dpt\, Universi
 ty of Athens)\nWe consider the internal shock formation in magnetized outf
 lows and we\nexamine the plastic collision between such relativistic blobs
  taking\ninto account a possible dissipation of magnetic flux.  We find th
 at\nafter the collision a large amount of energy is released in\nthermal f
 orm and consequently we assume that this is transferred\ninto protons whic
 h obtain a relativistic\nMaxwellian distribution. The relativistic thermal
  proton plasma is dense\nenough to suffer substantial energy losses throug
 h proton-proton\ninteractions and thus to transfer its initial energy into
 \nphotons\, electron-positron pairs and neutrinos. We estimate the radiate
 d\nspectrum by following the evolution of protons\, electrons and photons 
 as they\ninteract with each other and with the magnetic field as well.\n\n
 https://indico.nucleares.unam.mx/event/4/session/39/contribution/1141
LOCATION:Merida\, Mexico Regency (Hyatt)
URL:https://indico.nucleares.unam.mx/event/4/session/39/contribution/1141
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