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<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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<startDate>2007-07-03T08:00:00</startDate>
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 <title>Cosmic Ray Acceleration by Stochastic Fields</title>
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   <title>Dr.</title>
   <name first="Hector Javier" middle="" last="Durand-Manterola"></name>
   <organization>Departamento de Fisica Espacial, Instituto de Geofisica, Universidad Nacional Autonoma de Mexico</organization>
   <emailHash>ae815ef43e63c295748edb23e18b8937</emailHash>
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   <title>Dr.</title>
   <name first="Hector Javier" middle="" last="Durand-Manterola"></name>
   <organization>Departamento de Fisica Espacial, Instituto de Geofisica, Universidad Nacional Autonoma de Mexico</organization>
   <emailHash>ae815ef43e63c295748edb23e18b8937</emailHash>
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  <name>Merida, Mexico</name>
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 <abstract>In 1949 Fermi proposed the stochastic acceleration as a particle acceleration 
mechanism.  Fermi spoke of large clouds magnetized that were the responsible 
for this acceleration.  In this work I have focused in the stochastic acceleration 
due to fluctuations of the magnetic field of small scale that show to be 
extremely efficient accelerating.  I show that with a force of 10e-16 N a proton 
can be accelerated from 0 to 10e9 eV in only 70 days and from 0 to 10e12 eV in 
90,000 years.  The limit of this mechanism is smaller to 10e15 eV since more 
energy than that requires of more time than the age of the universe. Since the 
time in which this mechanism accelerates depends on the average force 
exercised by the fluctuations then is possible that in very turbulent zones of the 
universe, greater energies can be reached in smaller time.  For example if the 
average force is 10e-11 N energy of 10e19 eV is reached in 893 million years.</abstract>
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