TY - JOUR
T1 - Chiral symmetry at finite temperature
T2 - Linear versus nonlinear [Formula presented] models
AU - Bochkarev, Alexander
AU - Kapusta, Joseph I
N1 - Copyright:
Copyright 2017 Elsevier B.V., All rights reserved.
PY - 1996
Y1 - 1996
N2 - The linear [Formula presented] [Formula presented] model undergoes a symmetry-restoring phase transition at finite temperature. We show that the nonlinear [Formula presented] [Formula presented] model also undergoes a symmetry-restoring phase transition; the critical temperatures are the same when the linear model is treated in the mean field approximation and the nonlinear model is treated to leading plus subleading order in the [Formula presented] expansion. We also carefully define and study the behavior of [Formula presented] and the scalar condensate at low temperatures in both models, showing that they are independent of field redefinition.
AB - The linear [Formula presented] [Formula presented] model undergoes a symmetry-restoring phase transition at finite temperature. We show that the nonlinear [Formula presented] [Formula presented] model also undergoes a symmetry-restoring phase transition; the critical temperatures are the same when the linear model is treated in the mean field approximation and the nonlinear model is treated to leading plus subleading order in the [Formula presented] expansion. We also carefully define and study the behavior of [Formula presented] and the scalar condensate at low temperatures in both models, showing that they are independent of field redefinition.
UR - http://www.scopus.com/inward/record.url?scp=0000340625&partnerID=8YFLogxK
UR - http://www.scopus.com/inward/citedby.url?scp=0000340625&partnerID=8YFLogxK
U2 - 10.1103/PhysRevD.54.4066
DO - 10.1103/PhysRevD.54.4066
M3 - Article
AN - SCOPUS:0000340625
SN - 1550-7998
VL - 54
SP - 4066
EP - 4079
JO - Physical Review D - Particles, Fields, Gravitation and Cosmology
JF - Physical Review D - Particles, Fields, Gravitation and Cosmology
IS - 6
ER -