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PreprintarXiv licencearXiv

Chiral invariant mass and scale symmetry in dense matter from a dilaton compensated parity doublet model

Abstract

In the parity doublet model the nucleon mass includes a chiral invariant part m0, which is conventionally assumed to be medium independent. We promote this assumption to a dynamical question by making the model scale invariant using a dilaton compensator χ, so that the effective chiral invariant mass minv∗ = m0χ̃, with χ̃= χ/fχ, responds to the partial restoration of scale symmetry in the medium. We fit the model parameters by using vacuum spectra, nuclear matter properties, and NICER mass--radius posteriors---with the hadronic equation of state connected to 2+1-flavor Nambu--Jona-Lasinio quark matter by an interpolation. The best fit gives m0 = 657 MeV, a maximum neutron-star mass of 2.30 M⊙ and R1.4 = 12.22 km, with the mass--radius sequence passing through all three NICER credible regions. The resulting tidal deformabilities, Λ1.4 = 387 and Λ̃= 463, are consistent with GW170817 measurements. The in-medium analysis separates the two restorations: at the hadron--quark matching density the chiral condensate falls to 56% of its vacuum value, while the dilaton decreases only to 94%, so the nucleon arrives at the matching density with 90% of its mass carried by the invariant part. The order parameters of chiral and scale symmetries organize the in-medium probes, making the ω an almost pure probe of scale symmetry and the ρ of chiral restoration, which gives us a clue on the origin of hadron mass.

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BibTeX
@misc{ma2026chiral,
  title = {{Chiral invariant mass and scale symmetry in dense matter from a dilaton compensated parity doublet model}},
  author = {Yao Ma and Bikai Gao and Masayasu Harada and Yong-Liang Ma},
  howpublished = {arXiv},
  year = {2026},
  month = nov,
  doi = {10.48550/arxiv.2611.08163},
  eprint = {2611.08163},
  archivePrefix = {arXiv},
  url = {https://arxiv.org/abs/2611.08163},
}
RIS
TY  - UNPB
TI  - Chiral invariant mass and scale symmetry in dense matter from a dilaton compensated parity doublet model
AU  - Yao Ma
AU  - Bikai Gao
AU  - Masayasu Harada
AU  - Yong-Liang Ma
PY  - 2026
DA  - 2026/11/05
PB  - arXiv
DO  - 10.48550/arxiv.2611.08163
UR  - https://arxiv.org/abs/2611.08163
AB  - In the parity doublet model the nucleon mass includes a chiral invariant part m_0, which is conventionally assumed to be medium independent. We promote this assumption to a dynamical question by making the model scale invariant using a dilaton compensator χ, so that the effective chiral invariant mass m_inv^∗ = m_0χ̃, with χ̃= χ/f_χ, responds to the partial restoration of scale symmetry in the medium. We fit the model parameters by using vacuum spectra, nuclear matter properties, and NICER mass--radius posteriors---with the hadronic equation of state connected to 2+1-flavor Nambu--Jona-Lasinio quark matter by an interpolation. The best fit gives m_0 = 657 MeV, a maximum neutron-star mass of 2.30 M_⊙ and R_1.4 = 12.22 km, with the mass--radius sequence passing through all three NICER credible regions. The resulting tidal deformabilities, Λ_1.4 = 387 and Λ̃= 463, are consistent with GW170817 measurements. The in-medium analysis separates the two restorations: at the hadron--quark matching density the chiral condensate falls to 56% of its vacuum value, while the dilaton decreases only to 94%, so the nucleon arrives at the matching density with 90% of its mass carried by the invariant part. The order parameters of chiral and scale symmetries organize the in-medium probes, making the ω an almost pure probe of scale symmetry and the ρ of chiral restoration, which gives us a clue on the origin of hadron mass.
ER  -