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 <user>
  <title></title>
  <name first="Admin" middle="" last="Indico"></name>
  <organization>ICN-UNAM</organization>
  <emailHash>1482bc95ee34f0461176da21871284c8</emailHash>
  <userid>3</userid>
 </user>
</announcer>
<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>
<participants></participants>
<closed>True</closed>
<location>
 <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>
<chair>
 <user>
  <title>Dr.</title>
  <name first="José" middle="" last="Valdés"></name>
  <organization>IGeof-UNAM</organization>
  <emailHash>40af9343b8bb9d18708b4f0252d5f53c</emailHash>
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</chair>
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 <track>OG.1.2</track>
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  <id>0</id>
  <name>Oral</name>
 </type>
 <title>Can solar 6Li abundance really be explained by Galactic cosmic-rays?</title>
 <speakers>
  <user>
   <title>Dr.</title>
   <name first="Tijana" middle="" last="Prodanovic"></name>
   <organization>University of Novi Sad, Serbia</organization>
   <emailHash>e828d258f79fe5daa32f7400ba84920b</emailHash>
  </user>
 </speakers>
 <primaryAuthors>
  <user>
   <title>Dr.</title>
   <name first="Tijana" middle="" last="Prodanovic"></name>
   <organization>University of Novi Sad, Serbia</organization>
   <emailHash>e828d258f79fe5daa32f7400ba84920b</emailHash>
  </user>
 </primaryAuthors>
 <coAuthors>
  <user>
   <title>Prof.</title>
   <name first="Brian D." middle="" last="Fields"></name>
   <organization>University of Illinois at Urbana-Champaign</organization>
   <emailHash>03b9f8bba3df3c7c662f1d630108fbfd</emailHash>
  </user>
 </coAuthors>
 <location>
  <name>Merida, Mexico</name>
  <address></address>
  <room>Uxmal + Tulum (Holiday Inn)</room>
 </location>
 <startDate>2007-07-05T09:18:00</startDate>
 <endDate>2007-07-05T09:30:00</endDate>
 <duration>00:12</duration>
 <abstract>Cosmic-ray interactions are the only known source of the rare isotope 6Li. The
standard picture is that the observed  solar 6Li is produced by galactic cosmic-rays
accelerated in supernova remnants. Thus lithium-6 is a unique probe of the local
Galactic (hadronic) cosmic-ray history. On the other hand, extragalactic gamma-ray
background is a measure of cosmic-ray fluence but for the average star-forming
galaxy. Using the connection between production of lithium and hadronic gamma-rays in
cosmic-ray interactions we tested this assumption and came to a surprising and
alarming result: extragalactic gamma-ray background allows for only ~50% of solar
lithium-6 abundance to be produced by Galactic Cosmic Rays. Although extreme
assumptions yield a consistent picture, more realistic ones indicate that solar 6Li
cannot be produced by standard GCRs alone without overproducing the hadronic gamma rays.</abstract>
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