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  <organization>ICN-UNAM</organization>
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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>
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<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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  <name first="José" middle="" last="Valdés"></name>
  <organization>IGeof-UNAM</organization>
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 <title>A conservative dark matter annihilation bound from the diffuse gamma ray flux</title>
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   <title>Dr.</title>
   <name first="Pasquale Dario" middle="" last="Serpico"></name>
   <organization>Fermilab</organization>
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   <title>Dr.</title>
   <name first="Pasquale Dario" middle="" last="Serpico"></name>
   <organization>Fermilab</organization>
   <emailHash>41ab5f280edb91423ad8e3776a277e81</emailHash>
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   <title>Prof.</title>
   <name first="Michael" middle="" last="Kachelriess"></name>
   <organization>Department of Physics, NTNU - Trondheim, Norway</organization>
   <emailHash>812295aeaa8b50feb9dc7724a9a0a92a</emailHash>
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  <name>Merida, Mexico</name>
  <address></address>
  <room>Kabah (Holiday Inn)</room>
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 <startDate>2007-07-10T08:54:00</startDate>
 <endDate>2007-07-10T09:06:00</endDate>
 <duration>00:12</duration>
 <abstract>We discuss the general observational upper limits on the total annihilation rate of
dark matter derived from the diffuse gamma ray background measured by the EGRET
satellitr. We assume that the dark matter annihilates at tree level in the least
detectable final states in the Standard Model, namely neutrinos. Any other decay
channel would lead to stronger constraints. Electroweak jet cascading imply that, for
masses above ~100 GeV, interesting bounds apply which are much more stringent than
well-known general bounds as the unitarity one and comparable or only a few times
weaker than the bounds recently derived from atmospheric neutrino data.
We briefly discuss the perspectives of improvement of these constraints on the light
of forthcoming GLAST stellite data.</abstract>
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