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Infrared behaviour of the pressure in gϕ^3 theory in 6 dimensions

M. E. Carrington·T. J. Hammond·R. Kobes
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Abstract

In an earlier paper Almeida and Frenkel considered the calculation of the pressure in gϕ^3 theory in 6 dimensions via the Schwinger--Dyson equation. They found, under certain approximations, that a finite result ensues in the infrared limit. We find this conclusion to remain true with certain variations of these approximations, suggesting the finiteness of the result to be fairly robust.

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M. E. Carrington, T. J. Hammond, R. Kobes. 2001-11-22. Infrared behaviour of the pressure in gϕ^3 theory in 6 dimensions. https://doi.org/10.1103/physrevd.65.067703

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