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VERSION:2.0
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BEGIN:VEVENT
DTSTAMP:20260523T070713Z
UID:https://www.ipp.mpg.de/events/41811/5593513
DTSTART:20250519T120000Z
DTEND:20250519T133000Z
CLASS:PUBLIC
CREATED:20250509T140559Z
DESCRIPTION:Abstract: Cosmic rays (CRs) with energies below the 'knee' at a
 bout 3 PeV are believed to be of Galactic origin\, but it is still not ful
 ly understood in which astrophysical objects they are produced. The classi
 cal paradigm states that Supernova remnants (SNRs) are the main sources of
  Galactic CRs mainly on the account of their energy budget that is suffici
 ent to explain the energy density of low-energy CRs. But whether SNRs are 
 responsible for all the Galactic CRs or not remains an open question as ma
 ny pieces of the puzzle are still missing. To answer this question it is n
 ecessary to understand whether SNRs can accelerate particles beyond PeV en
 ergies and whether the total yield of CRs from SNRs is compatible with obs
 ervations in terms of the spectral shaper and elemental composition. In th
 is talk I will critically assess the capabilities of SNRs as CR accelerato
 rs by the means of multiwavelength observations and numerical simulations.
 \nVortragende(r): Dr. Iurii Sushch
LAST-MODIFIED:20250509T141629Z
LOCATION:IPP L7A\, Raum: 121
ORGANIZER;CN=Plasma Astrophysics group (TOK):mailto:artem.bohdan@ipp.mpg.de
SUMMARY:Supernova remnants as factories of cosmic rays
URL;VALUE=URI:https://www.ipp.mpg.de/events/41811/5593513
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