English (United Kingdom)

https://curated-unify.zendy.io/wp-json/zendy-region/v1/featured_content/oa?rat=en

https://curated-unify.zendy.io/wp-json/zendy-region/v1/highlighted_journal/

Global: Zendy Plus annual

Presents the access of premium content as premium feature

Premium Content

Presents the keyphrase highlighting as premium feature

Keyphrase Highlighting

Presents the summarisation as premium feature

Summarisation

Insights

Presents the pdf analysis as premium feature

PDF Analysis

Presents the zaia usage as premium feature

ZAIA

Global: Zendy Plus monthly

Global: Zendy Tools annual

Global: Zendy Tools monthly

Global: Zendy Free Plan

In an earlier paper Almeida and Frenkel considered the calculation of thepressure in g\phi^3 theory in 6 dimensions via the Schwinger--Dyson equation.They found, under certain approximations, that a finite result ensues in theinfrared limit. We find this conclusion to remain true with certain variationsof these approximations, suggesting the finiteness of the result to be fairlyrobust.Comment: 6 pages, 4 figures, uses revtex

physical review. d. particles, fields, gravitation, and cosmology/physical review. d. particles and fields

Infrared behavior of the pressure in<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mi>g</mml:mi><mml:mrow><mml:msup><mml:mrow><mml:mi>φ</mml:mi></mml:mrow><mml:mrow><mml:mn>3</mml:mn></mml:mrow></mml:msup></mml:mrow></mml:math>theory in 6 dimensions

Infrared behavior of the pressure ingφ3theory in 6 dimensions