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<supportEmail caption="Support">icrc2007@icrc2007.unam.mx</supportEmail>
<title>30th International Cosmic Ray Conference</title>
<description>The 30th International Cosmic Ray Conference will be held from July 3, 2007 to July 11, 2007 in Merida, Yucatan, Mexico.</description>
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 <name>Merida, Mexico</name>
 <address></address>
 <room></room>
</location>
<startDate>2007-07-03T08:00:00</startDate>
<endDate>2007-07-11T19:00:00</endDate>
<creationDate>2005-09-26T05:04:53</creationDate>
<modificationDate>2024-04-12T17:46:55</modificationDate>
<timezone>Mexico/General</timezone>
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 <title>Simulation of cosmic ray propagation in the Galactic center ridge in accordance with observed VHE γ-ray emissions.</title>
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   <name first="Stavros" middle="" last="Dimitrakoudis"></name>
   <organization>National and Kapodistrian University of Athens</organization>
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   <title>Mr.</title>
   <name first="Stavros" middle="" last="Dimitrakoudis"></name>
   <organization>National and Kapodistrian University of Athens</organization>
   <emailHash>cc5acb5e06bb956198e8b55a92e80942</emailHash>
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  <name>Merida, Mexico</name>
  <address></address>
  <room>Uxmal + Tulum (Holiday Inn)</room>
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 <startDate>2007-07-05T11:42:00</startDate>
 <endDate>2007-07-05T11:54:00</endDate>
 <duration>00:12</duration>
 <abstract>Diffuse VHE γ radiation from the Galactic center ridge observed by the H.E.S.S.
telescope has been convincingly linked with the propagation of recently accelerated
cosmic rays that interact with molecular hydrogen clouds during their diffusion.
Through a series of time-dependent simulations of that diffusion for different
propagation parameters we have obtained the most probable values of the diffusion
coefficient for the galactic center region. Assuming that the diffusion coefficient
is of the form κ(E) = κ0(E/E0)^δ, then for different optimal combinations of κ0 and δ
its value is obtained for cosmic rays originating from a central point (possibly Sgr
A East) 10 kyr ago.</abstract>
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