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On-shell versus curvature mass parameter fixing schemes in the quark-meson model and its phase diagrams

Suraj Kumar Rai and Vivek Kumar Tiwari
Phys. Rev. D 105, 094010 – Published 16 May 2022

Abstract

We compute and compare the effective potential and phase structure for the quark-meson model in an extended mean-field approximation when vacuum one-loop quark fluctuations are included and the model parameters are fixed using different renormalization prescriptions. When the quark one-loop vacuum divergence is regularized under the minimal subtraction scheme, the fixing of the model parameters using the curvature masses of the scalar and pseudoscalar mesons has been termed as the quark-meson model with the vacuum term (QMVT). However, this prescription becomes inconsistent when we notice that the curvature mass is akin to defining the meson mass by the self-energy evaluation at vanishing momentum. In this work, we apply the recently reported exact prescription of the on-shell parameter fixing to that version of quark-meson model where the two quark flavors are coupled to the eight mesons of the SUL(2)×SUR(2) linear sigma model with isosinglet σ (η), isotriplet a0 (π) scalar (pseudoscalar) mesons. The model then becomes the renormalized quark-meson (RQM) model where physical (pole) masses of mesons and pion decay constant are put into the relation of the running mass parameter and couplings by using the on-shell and the minimal subtraction renormalization schemes. The vacuum effective potential plots, the phase diagrams and the order parameter temperature variations for both the RQM model and the QMVT model are exactly identical for the mσ=616MeV. The vacuum effective potential, when the mσ<616MeV, is deepest for the QMVT model. An interesting trend reversal is observed for the mσ>616MeV when the effective potential of the RQM model becomes deepest. We find similar mσ dependent differences in the nature of the RQM and QMVT model phase diagrams and the order parameter temperature variations. Furthermore, SUA(2) chiral and UA(1) axial symmetry breaking/restoration and their interplay can also be investigated in this framework.

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  • Received 24 February 2022
  • Accepted 25 April 2022

DOI:https://doi.org/10.1103/PhysRevD.105.094010

Published by the American Physical Society under the terms of the Creative Commons Attribution 4.0 International license. Further distribution of this work must maintain attribution to the author(s) and the published article’s title, journal citation, and DOI. Funded by SCOAP3.

Published by the American Physical Society

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Authors & Affiliations

Suraj Kumar Rai1,2,* and Vivek Kumar Tiwari1,†

  • 1Department of Physics, University of Allahabad, Prayagraj, India-211002
  • 2Department of Physics, A.N.D. Kisan P.G. College Babhnan Gonda, Dr. R.M.L. Awadh University, Faizabad, India-271313

  • *surajrai050@gmail.com
  • vivekkrt@gmail.com

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Vol. 105, Iss. 9 — 1 May 2022

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