paper

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

arXiv:hep-ph/0111293 · doi:10.1103/PhysRevD.65.067703

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.

6 pages, 4 figures, uses revtex4

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