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SUMMARY:Propagation of Cosmic Rays in Anisotropic Diffusion Models
DTSTART;VALUE=DATE-TIME:20160526T134000Z
DTEND;VALUE=DATE-TIME:20160526T140000Z
DTSTAMP;VALUE=DATE-TIME:20261012T115447Z
UID:indico-contribution-2765@indico.ific.uv.es
DESCRIPTION:Speakers: Annika Reinert (Bethe Center for Theoretical Physics
 \, Universität Bonn)\nOne aim of cosmic ray measurements is to search for
  possible signatures of annihilating or decaying dark matter. The excess o
 f positrons measured at the top of the atmosphere has attracted a lot of a
 ttention in this context. On the other hand it has been proposed that the 
 data might challenge the established diffusion model for cosmic ray propag
 ation. We investigate a modification of the two-zone diffusion model givin
 g rise to changes in the spectral shape of the positron spectrum.\n\nhttps
 ://indico.ific.uv.es/event/2534/contributions/2765/
LOCATION:
URL:https://indico.ific.uv.es/event/2534/contributions/2765/
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