[SEMINARI]: Dr. Kalashnikov: Infrared Properties of Hot Gauge Theories 
    Arcadi Santamaria 
    Arcadi.Santamaria en uv.es
       
    Mar Feb 23 18:51:29 CET 1999
    
    
  
 
------------ próxima parte ------------
  ------------------------------------------------------------------------
                              S E M I N A R I
            [Image]    Departament de Física Teòrica     [Image]
                          Universitat de València
                      46100 Burjassot (València) Spain
  ------------------------------------------------------------------------
                    Infrared Properties of Hot Gauge Theories
                              Oleg Kalashnikov
                           (Lebedev Inst., Moscow)
  ------------------------------------------------------------------------
                     Aula de Seminaris de Física Teòrica
                Thursday 25 of February of 1999 at 12:00 AM
  ------------------------------------------------------------------------
                                    Resum
  The infrared limits of the gluon polarization tensor are analyzed in hot
  non-Abelian theories using perturbative and nonperturbative calculations.
The calculations performed within the lowest one-loop order lead to the very
  important result: to the infrared fictitious pole of the gluon propagator
   which spoils the selfconsistency within any perturbative scheme. Within
    nonperturbative calculations there are two different possibilities to
eliminate this difficulty: the nonanalytical logarithmic behaviour for small
  momenta and the finite limit of the order of g^2 T that is the so-called
  gluon magnetic mass. Both possibilities are analyzed. The next-to-leading
  order calculations are reviewed to present the nonperturbative screening
   potential within hot non-Abelian QCD and the Debye mass. The screening
  potential being calculating nonperturbatively does not correspond to the
   usual attractive QCD-Debye one and instead of that it is repulsive and
 power-behaved like 1/r^6 at large distance. The more exact calculations of
                 the Debye mass are also reviewed briefly.
  ------------------------------------------------------------------------
    
    
Más información sobre la lista de distribución Seminari