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Pressure and Spectral Density of Fermions at Finite Temperature

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摘要 The pressure of a fermion system is expressed as a mass integral over the full two-point spectral densities within the real time formalism by use of the Keldysh representation for the propagators.This simpliSes the calculation significantly and allows a Dyson resummation.The expression is used to demonstrate that potential infrared divergences are rendered harmless.We apply it to check the pressures of an ideal fermion gas and of a chemically non-equilibrated quantum chromodynamics plasma.
作者 侯德富 U.Heinz 李家荣 HOU De-fu;U.Heinz;LI Jia-rong(Institute of Particle Physics,Huazhong Normal University,Wuhan 430079;Institut fur Theoretische Physik,Universitat Regensburg,D-93040 Regensburg,Germany)
出处 《Chinese Physics Letters》 SCIE CAS CSCD 1999年第10期709-711,共3页 中国物理快报(英文版)
基金 Supported by the Deutsche Forschungsgemeinschaft(DFG) the Bundesministerium fur Bildung und Forschung(BMBF) the National Natural Science Foundation of China under Grant No.19775017 the Gesellschaft fur Schwerionenforschung(GSI).
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