Scalar Fields at Zero and Finite Temperature

Author(s):  
Andreas Wipf
1990 ◽  
Vol 05 (02) ◽  
pp. 353-361 ◽  
Author(s):  
PINAKI ROY

We evaluate the finite temperature one-loop effective potential for scalar fields in Kaluza-Klein universe consisting of the product of a space with open Robertson-Walker metric and the N sphere SN. The one-loop effective potential has been computed in both high and low temperature limits.


2015 ◽  
Vol 2015 (8) ◽  
Author(s):  
Yeuk-Kwan E. Cheung ◽  
Marco Drewes ◽  
Jin U Kang ◽  
Jong Chol Kim

2020 ◽  
Vol 44 (5) ◽  
pp. 053103
Author(s):  
Hui Xu ◽  
Lei Ming ◽  
Yeuk-Kwan E. Cheung

2016 ◽  
Vol 31 (40) ◽  
pp. 1650227 ◽  
Author(s):  
T. C. A. Calza ◽  
F. L. Cardoso ◽  
L. G. Cardoso ◽  
C. A. Linhares

The formalism of finite-temperature quantum field theory, as developed by Matsubara, is applied to a Hamiltonian of N scalar fields with a quartic self-interaction at large N. A renormalized expression in the lowest quantum approximation is obtained for the squared mass m2 of the field, as a function of the temperature T, from which we study the process of spontaneous symmetry breaking. We find that in a range of values around the critical temperature Tc, the squared mass can be approximated by a linear relation m2 [Formula: see text] (T − Tc). We thus demonstrate the compatibility of the finite-temperature formalism for scalar fields, in the vicinity of criticality, with respect to the Ginzburg–Landau model. We also discuss the effects caused by the presence of a chemical potential and of an external magnetic field applied to the finite-temperature system, which however do not affect the linearity of the relation between the squared mass and the temperature.


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