Abstract
Using the imaginary time formalism in thermal field theory, we derive the running coupling constant and running mass in two loop order. In the process, we express the imaginary time formalism of Feynman diagrams as the summation of nonthermal quantum field theory (QFT) Feynman diagrams with coefficients that depend on temperature and mass. Renormalization constants for thermal ${\ensuremath{\phi}}^{4}$ theory were derived using simple diagrammatic analysis. Our model links the nonthermal QFT and the imaginary time formalism by assuming both have the same mass scale $\ensuremath{\mu}$ and coupling constant $g$. When these results are combined with the renormalization group equations and applied simultaneously to thermal and nonthermal proper vertex functions, the coupling constant and running mass with implicit temperature dependence are obtained. We evaluated pressure for scalar particles in two loop orders at the zero external momentum limit by substituting the running mass result in the quasiparticle model.
Highlights
There are different quasiparticle models [1,2,3,4,5,6,7,8,9] used to describe the state of the quark-gluon plasma (QGP)
Two loop calculation The redefinition of the proper vertex function in one loop order [Eqs. (36) and (40)] to make it finite causes more counterterm diagrams to emerge in the two loop order calculation
The previous results show that no Zφ, Zg, or Zm2 is explicitly temperature dependent, and they agree with the nonthermal field theory
Summary
There are different quasiparticle models [1,2,3,4,5,6,7,8,9] used to describe the state of the quark-gluon plasma (QGP). The concept of thermally dependent RGEs [11,12] considered the mass and the coupling constant as temperature functions. We use the simple diagrammatic analysis [34] in imaginary time formalism (ITF) [35] to derive a coupling constant that obeys RGE for both thermal and nonthermal field theories under the same mass scale μ and coupling constant g. We substitute the running mass on the self-consistent quasiparticle model [5,6,7] pressure relation and check whether it will lead to the StephenBoltzmann limit at the higher temperature approximations Another essential nature is the flexibility of this model. Once we have data points, we can fit running mass, coupling, pressure results to the data points by choosing appropriate values for the integral constants
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