activity
19942026
most cited2PI effective action and gauge invariance problems

54 citations · 1.1k across the 82 of their papers we have counts for

collaborators

82 papers

hep-th2026

The gauge invariance of non-perturbative vertex prescriptions

M. E. Carrington, A. R. Frey, B. A. Meggison

We study the gauge invariance of different continuum methods to include non-perturbative effects in gauge theories. We work with three dimensional quantum electrodynamics and imple…

hep-th2026

supersymmetric Yang-Mills thermodynamics to order

Margaret E. Carrington, Gabor Kunstatter, Ubaid Tantary

We calculate the resummed perturbative free energy of supersymmetric Yang-Mills in four spacetime dimensions (SYM) to order in the 't Hooft coupling…

hep-ph2024

The effect of anisotropy on the formation of heavy quarkonium bound states

Margaret E. Carrington, Gabor Kunstatter, Arghya Mukherjee

We study the real part of the static potential of a heavy quark-antiquark system in an anisotropic plasma medium. We use a quasi-particle approach where the collective dynamics of…

hep-th2024

Evidence for universal flow and characteristics of early time thermalization in a scalar field model for heavy ion collisions

Margaret E. Carrington, Wade N. Cowie, Gabor Kunstatter +1

We study numerically the evolution of an expanding strongly self-coupled real scalar field. We use a conformally invariant action that gives a traceless energy-momentum tensor and…

nucl-th2023

Glasma properties in small proper time expansion

Margaret E. Carrington, Wade N. Cowie, Bryce T. Friesen +2

In a series of works by two of us, various characteristics of the glasma from the earliest phase of relativistic heavy-ion collisions have been studied using a proper time expansio…

astro-ph.SR2022★ 1 cited

Spin-down and reduced mass loss in early-type stars with large-scale magnetic fields

Z. Keszthelyi, A. de Koter, Y. Götberg +12

Magnetism can greatly impact the evolution of stars. In some stars with OBA spectral types there is direct evidence via the Zeeman effect for stable, large-scale magnetospheres, wh…