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  <name first="Admin" middle="" last="Indico"></name>
  <organization>ICN-UNAM</organization>
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  <userid>3</userid>
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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>
<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>HE.1.5</track>
 <type>
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  <name>Oral</name>
 </type>
 <title>The search for UHECR and Neutrinos from Space: a "Vision" for the next decade</title>
 <speakers>
  <user>
   <title>Dr.</title>
   <name first="Andrea" middle="" last="Santangelo"></name>
   <organization>IAAT University of Tuebingen, Germany</organization>
   <emailHash>a6810057b29222119facec27ed06debf</emailHash>
  </user>
 </speakers>
 <primaryAuthors>
  <user>
   <title>Dr.</title>
   <name first="Andrea" middle="" last="Santangelo"></name>
   <organization>IAAT University of Tuebingen, Germany</organization>
   <emailHash>a6810057b29222119facec27ed06debf</emailHash>
  </user>
  <user>
   <title>Dr.</title>
   <name first="Alessandro" middle="" last="Petrolini"></name>
   <organization>INFN and University of Genova</organization>
   <emailHash>d41d8cd98f00b204e9800998ecf8427e</emailHash>
  </user>
 </primaryAuthors>
 <location>
  <name>Merida, Mexico</name>
  <address></address>
  <room>Yucatan II+III+IV (Fiesta Americana)</room>
 </location>
 <startDate>2007-07-10T11:30:00</startDate>
 <endDate>2007-07-10T11:42:00</endDate>
 <duration>00:12</duration>
 <abstract>Ultra High Energy Cosmic Rays and Neutrinos, with energies from a few  10^18 eV to
beyond the decade of 10^20 eV, and Cosmic Rays with E &gt;= 5 10^19 eV appear to be the
only suitable messengers to explore the Universe at frontier energies, where
radiation is expected to be produced under the most extreme physical conditions.
Observations of these UHE particles will certainly provide new information 1) on the
sources; and 2) on the physical mechanisms able to accelerate these extreme
messengers to macroscopic energies. Moreover, UHE particles may also, provide
evidence of yet unknown physics or of exotic particles, relics of the early Universe.
To reach these
goals, innovative experiments with larger effective aperture (A_eff &gt;= 10^5 km^2 sr)
and good understanding of systematic uncertainties (less than ~10%) must be
developed. Space-based observatories can reach the effective area necessary to
systematically explore the UHE Universe. In the present paper  1.) we present the
Science Rationale behind UHE studies from space; 2.) we briefly discuss the  science
goals, the requirements, the instrument and mission profile of  a  'next-generation"
space-based mission for UHE observations to be  designed and developed in the
framework of the ESA "Cosmic Vision  2015-2025" long term plan.</abstract>
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