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<announcer>
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  <title></title>
  <name first="Yves" middle="" last="Schutz"></name>
  <organization>IN2P3 (FR) and CERN</organization>
  <email>yves.roland.schutz@cern.ch</email>
  <userid>16822</userid>
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<supportEmail caption="Support">yves.schutz@cern.ch</supportEmail>
<keywords>
 <keyword>quark-matter, heavy-ion, ultrarelativistic energies, LHC, CERN, ALICE, CMS, ATLAS, RHIC, BNL, PHENIX, STAR</keyword>
</keywords>
<title>QM 2011 - XXII International Conference on Ultrarelativistic Nucleus-Nucleus Collisions</title>
<description>&lt;p&gt;Quark Matter Conference in 2011 at Annecy (&lt;a href="http://qm2011.in2p3.fr"&gt; back to QM2011 home page&lt;/a&gt; )&lt;/p&gt;</description>
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 <name>Centre Bonlieu</name>
 <address>France</address>
 <room>Théâtre National</room>
</location>
<startDate>2011-05-22T08:30:00</startDate>
<endDate>2011-05-28T13:00:00</endDate>
<creationDate>2008-03-04T17:38:10</creationDate>
<modificationDate>2012-03-01T14:02:44</modificationDate>
<timezone>Europe/Zurich</timezone>
<chair>
 <user>
  <title></title>
  <name first="Yves" middle="" last="Schutz"></name>
  <organization>IN2P3/CERN</organization>
  <email>yves.schutz@cern.ch</email>
 </user>
 <user>
  <title></title>
  <name first="Urs" middle="" last="Wiedemann"></name>
  <organization>CERN</organization>
  <email>urs.wiedemann@cern.ch</email>
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 <UnformatedUser>Yves Schutz &amp; Urs Wiedemann</UnformatedUser>
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  <name>Poster</name>
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 <title>Radiative energy loss reduction in a plasma due to damping</title>
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   <title>Dr.</title>
   <name first="Marcus" middle="" last="Bluhm"></name>
   <organization>Laboratoire SUBATECH</organization>
   <email>marcusbluhm@gmx.de</email>
  </user>
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  <user>
   <title>Dr.</title>
   <name first="Marcus" middle="" last="Bluhm"></name>
   <organization>Laboratoire SUBATECH</organization>
   <email>marcusbluhm@gmx.de</email>
  </user>
 </primaryAuthors>
 <coAuthors>
  <user>
   <title>Prof.</title>
   <name first="Pol Bernard" middle="" last="Gossiaux"></name>
   <organization>Laboratoire SUBATECH</organization>
   <email>gossiaux@subatech.in2p3.fr</email>
  </user>
  <user>
   <title>Prof.</title>
   <name first="Joerg" middle="" last="Aichelin"></name>
   <organization>Laboratoire SUBATECH</organization>
   <email>aichelin@subatech.in2p3.fr</email>
  </user>
 </coAuthors>
 <location>
  <name>Imperial Palace</name>
  <address>Allée Impérial 74000 Annecy, France
Tél. : +33 4 50 09 30 00</address>
  <room>Rotonde de l'Europe (150)</room>
 </location>
 <startDate>2011-05-26T15:00:00</startDate>
 <endDate>2011-05-26T15:20:00</endDate>
 <duration>00:20</duration>
 <abstract>The strong quenching of jets and the suppression of hadron spectra 
at high transverse momenta are striking experimental observations 
made in high energy nuclear collisions. Both have been interpreted 
as signature for the formation of a deconfined plasma of QCD 
matter, in which partons suffer a medium-induced energy loss. In 
theoretical studies devoted to a parton's radiative energy loss, 
however, the damping of radiation within the plasma has so far 
widely been neglected. 

We investigate the radiative energy loss per unit distance of a 
relativistic colour charge traversing as probe an infinite 
absorptive plasma. The Landau-Pomeranchuk-Migdal effect is 
incorporated as well as modifications due to the polarization of 
and damping mechanisms in the medium. The latter are 
phenomenologically described by a complex index of refraction, 
while the colour charge dynamics is considered in the Abelian 
approximation. We find a substantial reduction of the medium-
induced mechanical work in addition to the well known Ter-
Mikaelian effect from the polarization of matter. Moreover, the 
formation time of radiated quanta is also drastically reduced, 
both for small frequencies, where damping has a minor additional 
impact besides the polarization effect, and for larger frequencies. 
These effects are more pronounced for larger medium damping 
and/or larger initial energy of the charge. 

Therefore, we expect that our study will have a significant impact 
on the understanding of jet quenching phenomena in ultra-
relativistic heavy-ion collisions at RHIC and even more at LHC.</abstract>
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