Phase structure of NJL model with weak renormalization group

We analyze the chiral phase structure of the Nambu-Jona-Lasinio model at finite temperature and density by using the functional renormalization group (FRG). The renormalization group (RG) equation for the fermionic effective potential V(σ;t) is given as a partial differential equation, where σ:=ψ¯ψ...

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Bibliographic Details
Main Authors: Aoki, Ken-Ichi (Author) , Kumamoto, Shin-Ichiro (Author) , Yamada, Masatoshi (Author)
Format: Article (Journal)
Language:English
Published: 11 April 2018
In: Nuclear physics. B, Particle physics
Year: 2018, Volume: 931, Pages: 105-131
ISSN:1873-1562
DOI:10.1016/j.nuclphysb.2018.04.005
Online Access:Verlag, lizenzpflichtig, Volltext: https://doi.org/10.1016/j.nuclphysb.2018.04.005
Verlag, lizenzpflichtig, Volltext: http://www.sciencedirect.com/science/article/pii/S0550321318300968
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Author Notes:Ken-Ichi Aoki, Shin-Ichiro Kumamoto, Masatoshi Yamada
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Summary:We analyze the chiral phase structure of the Nambu-Jona-Lasinio model at finite temperature and density by using the functional renormalization group (FRG). The renormalization group (RG) equation for the fermionic effective potential V(σ;t) is given as a partial differential equation, where σ:=ψ¯ψ and t is a dimensionless RG scale. When the dynamical chiral symmetry breaking (DχSB) occurs at a certain scale tc, V(σ;t) has singularities originated from the phase transitions, and then one cannot follow RG flows after tc. In this study, we introduce the weak solution method to the RG equation in order to follow the RG flows after the DχSB and to evaluate the dynamical mass and the chiral condensate in low energy scales. It is shown that the weak solution of the RG equation correctly captures vacuum structures and critical phenomena within the pure fermionic system. We show the chiral phase diagram on temperature, chemical potential and the four-Fermi coupling constant.
Item Description:Gesehen am 02.06.2020
Physical Description:Online Resource
ISSN:1873-1562
DOI:10.1016/j.nuclphysb.2018.04.005