REVIEW 3 major objections 4 minor 1 cited by
From Nuclear Matter with Quenched $g_A$ to Compact-Star Matter with a Signal for Emergent Hidden Scale Symmetry
T0 review · 3 major / 4 minor · reviewed 2026-08-06 · deepseek-v4-flash
Pith's one-line read The paper claims that two longstanding puzzles—why nuclear beta-decay coupling $g_A$ sits near 1 and why neutron-star cores have sound speed near $\sqrt{1/3}\,c$—are two manifestations of a single emergent hidden scale symmetry.
desk verdict A transparent, falsifiable synthesis of the author's own GnEFT program: the low-density g_A^L≈1 anchor is solid and testable, but the claimed link to the pseudo-conformal sound speed is an assumed parallel, not a derived consequence—though the paper openly concedes as much. read the letter →
The pith
A machine-rendered reading of the paper's core claim, the machinery that carries it, and where it could break.
The reading
What carries the argument
The machinery is hidden scale symmetry implemented by a conformal compensator/dilaton field $\hat\chi$ (identified with $f_0(500)$) and hidden local symmetry vector mesons $\rho,\omega$, organized through a renormalization-group description of baryons on the Fermi surface. The chain of reasoning runs from a chiral-scale effective Lagrangian, through the Landau-Fermi-liquid fixed point, to the dilaton-limit fixed point where $g_V\to g_A\to 1$ and $f_\pi\to f_{\hat\chi}\neq 0$; the skyrmion-to-half-skyrmion topology change at $n_{1/2}\approx(2-3)n_0$ provides the hadron-quark continuity that lets the same symmetry operate up to compact-star densities. These ingredients turn the density independence of $\langle\theta^\mu_\mu\rangle$ into the pseudo-conformal sound-speed relation.
What would settle it
Re-measure the superallowed Gamow-Teller strength of $^{100}$Sn with an independent technique: if the extracted $g_A^{\rm eff}$ falls in the RIKEN range $0.74{-}0.88$ rather than near the GSI value $0.96$, the paper's infrared-fixed-point premise and the connection to $v_s^2/c^2\approx 1/3$ are falsified. A complementary check would be a first-principles calculation of $\langle\theta^\mu_\mu\rangle(n)$ at $2{-}7n_0$; a density-dependent trace anomaly would violate Eq. (15).
Extended reading notes
Core claim
The paper's central claim is that the quasiparticle axial coupling $g_A^L$ is not a renormalized coupling that happens to land near 1; it is driven to $g_A^L\approx 1$ by the same dilaton-limit fixed point that produces the pseudo-conformal sound speed in compact stars. In the Landau-Fermi-liquid fixed-point approximation the formula $g_A^L = g_A(1-\tfrac13 \Phi \tilde F_1^\pi)^{-2}$ has a density dependence in the dilaton condensate $\Phi$ and pion Landau parameter $\tilde F_1^\pi$ that cancels, giving $\approx 1$ from light nuclei to nuclear matter and onward to high density. At the dilaton-limit fixed point the constraints $g_V\to g_A\to 1$ and $f_\pi\to f_{\hat\chi}\neq 0$ hold, the $\rho$ meson decouples from pions, and an emergent parity-doubled mass $m_0$ makes the nucleon mass density-independent. The trace of the energy-momentum tensor then satisfies $\partial\langle\theta^\mu_\mu\rangle/\partial n = (\partial\epsilon/\partial n)(1-3v_s^2/c^2)=0$, and with $\partial\epsilon/\partial n\neq 0$ this yields the pseudo-conformal sound speed $v_{\rm pcs}^2/c^2\approx 1/3$. Thus the paper presents quenched $g_A$ and the star-core sound speed as two parallel consequences of one emergent hidden scale symmetry.
Load-bearing premise
The argument stands on the premise that QCD has an infrared fixed point for three or fewer quark flavours, with the $f_0(500)$ as its dilaton, so that $g_A^{\rm eff}\approx 1$ is a symmetry effect rather than ordinary nuclear many-body physics; if that premise is false, or if the RIKEN value in $^{100}$Sn is the true one, the chain of connections collapses.
Editorial extensions
If this is right
- The same mechanism that quenches $g_A$ in nuclei should persist across the whole density range from light nuclei to the dilaton-limit fixed point, making $g_A^{\rm eff}\approx 1$ a symmetry prediction rather than a coincidence.
- The compact-star equation of state should be pseudo-conformal from roughly $2n_0$ to $5{-}7n_0$, with $v_s^2/c^2\approx 1/3$, a maximum mass near $2.05M_\odot$, and radii near 12.8 km for both $1.44M_\odot$ and $2.0M_\odot$ stars.
- Anomaly-induced quenching of $g_A$ is absent if $\beta'_{\rm IR}=0$; the GSI value $g_A^{\rm eff}\approx 0.96$ is consistent with this, while the RIKEN value $0.74{-}0.88$ would invalidate the IR-fixed-point assumption and break the chain.
- The density-independent trace anomaly implies that scale symmetry is not restored in compact stars but is hidden: $\langle\theta^\mu_\mu\rangle$ stays non-zero yet flat in density.
Reading between the lines
- Editorial inference: if the symmetry picture is right, deviations of $g_A^{\rm eff}$ from 1 should track density in a computable way across many nuclei, so a campaign of precise Gamow-Teller measurements in medium-mass nuclei would map the approach to the dilaton-limit fixed point.
- Editorial inference: the density-independent mass $m_0$ behind the flat trace anomaly should leave observable imprints beyond the sound speed, for instance in neutron-star cooling, neutrino emissivity, or tidal deformability, predictions the paper does not work out.
- Editorial inference: the GSI-versus-RIKEN discrepancy in $^{100}$Sn is not a detail of one nucleus; it is the cheapest decisive experiment for the whole framework, since the two values lead to opposite conclusions about the infrared fixed point.
Editorial analysis
A structured set of objections, weighed in public.
Referee Report
Summary. The paper develops the proposal that the long-standing puzzle of the effective axial coupling g_A^eff ≈ 1 in nuclei and the approximate sound speed v_s^2/c^2 ≈ 1/3 in compact-star matter are two manifestations of one emergent hidden scale symmetry. The formalism is a generalized nuclear EFT (GnEFT) that combines hidden local symmetry (vector mesons) and hidden scale symmetry (a dilaton identified with f0(500)), anchored on a Landau-Fermi-liquid fixed-point description of baryons on the Fermi surface and on a skyrmion-to-half-skyrmion topology change at a density n1/2. The low-density anchor is Eq. (5), which yields g_L^A ≈ 1 and reproduces the gyromagnetic ratio δg_l; the high-density anchor is Eq. (15), which gives the pseudo-conformal sound speed Eq. (16) when the trace anomaly is density-independent. The paper also discusses the GSI vs. RIKEN discrepancy for the 100Sn Gamow-Teller transition, and lists predictions for neutron-star masses, radii, and tidal deformability as a function of n1/2.
Significance. If the proposed connection holds, it would unify two seemingly unrelated phenomena in nuclear and astrophysics and would provide a concrete signal for an emergent scale symmetry in dense QCD matter. The paper is commendably honest about its fragility: it explicitly states that re-confirmation of the RIKEN quenching would break the entire chain of connections, and it identifies the 1/N̄ corrections as not fully worked out. The low-density relation Eq. (5) is a concrete, testable result anchored in the Landau-Migdal framework, and the paper cites a quantitative estimate of the 1/N̄ correction to g_L^A. The main weakness is that the central link between quenched g_A and the pseudo-conformal sound speed is presented as an analogy rather than derived; in particular, Eq. (15) is an identity whose physical content resides entirely in the premise ∂⟨θ_μ^μ⟩/∂n = 0, a premise that is asserted rather than demonstrated.
major comments (3)
- [§Pseudo-Conformal Sound Speed, Eq. (15)-(16)] The derivation of the pseudo-conformal sound speed is not self-contained. Equation (15) is a thermodynamic identity; the conclusion v_s^2/c^2 ≈ 1/3 follows only if ∂⟨θ_μ^μ⟩/∂n = 0, and the paper does not derive this density independence from the underlying GnEFT. The text justifies it by asserting that ⟨χ̂⟩* tends to a density-independent m0 in the half-skyrmion phase, but no calculation of ⟨χ̂⟩* as a function of density is shown. The scale invariance of normalized field configurations in Eq. (1) and Fig. 2 does not imply ∂⟨χ̂⟩*/∂n = 0, because the normalization by the maximum field value can absorb an overall density-dependent rescaling. This is a load-bearing step: without a derivation of ∂⟨χ̂⟩*/∂n = 0, Eq. (16) is an assumption, not a consequence of the IR fixed point.
- [§g_A^eff = 1 to Pseudo-Conformality] The central claim that quenched g_A and v_pcs^2/c^2 ≈ 1/3 are two manifestations of one symmetry is asserted as a 'parallel' rather than derived. The paper itself concedes, in the 'Quenching of g_A and Trace Anomaly' section, that 'I cannot give a simple and fully satisfactory answer' to how the g_A connection relates to pseudo-conformality. Equation (5) is a low-density Fermi-liquid result, while g_A → 1 at the dilaton-limit fixed point is a separate high-density constraint; the paper provides no operator relation or calculation showing that the same emergent scale symmetry controls both, nor that the mechanism behind Eq. (5) continues into the half-skyrmion phase. As written, the unity of the two phenomena is an interpretation, not a demonstrated consequence.
- [§Hadron-Quark Continuity and §Results] The paper relies on the large-N_c skyrmion-crystal description being valid up to compact-star densities of (5–7)n0, an extrapolation far beyond any direct test, and it treats the density independence of the dilaton VEV in the half-skyrmion phase as established by the skyrmion-crystal machinery. This is a legitimate framework choice, but it makes the pseudo-conformal prediction contingent on a set of non-perturbative assumptions that are not independently verified. A more explicit account of how the half-skyrmion phase yields ∂⟨χ̂⟩*/∂n = 0—beyond the scaling of normalized field shapes—would be needed to make Eq. (16) a quantitative prediction rather than a restatement of the premise.
minor comments (4)
- [Abstract and Footnote 4] The p parameter in the Grassmannian model is stated as p = 2 in the abstract and as p = 3 in footnote 4; this inconsistency should be resolved.
- [Preamble and Abstract] There are several typographical errors, including 'HQC)' in the abstract, 'obvoius' in the Preamble, and 'supperallowed' in the section on 100Sn; these should be corrected.
- [§Results] The statement that 'the only parameter in the calculation is the half-skyrmion phase density n1/2' is hard to reconcile with the earlier introduction of c_A, F_1^π, F_1^ω, m_L, and β'_IR; the paper should clarify which parameters are fixed by low-density data and which remain free in the compact-star calculation.
- [Figure 3] The discussion of the left and right panels of Fig. 3 refers to the role of the ρ–π decoupling, but the precise parameterization used for the density dependence of the ρ and ω couplings is not given; a brief statement of the model inputs would help the reader judge the sensitivity of the sound-speed curve.
Circularity Check
Sound-speed 1/3 is the density-independent trace-anomaly premise restated, and high-density g_A→1 is the DLFP constraint restated; the g_A–v_s^2 unification relies on same-author citations and is an interpretation rather than a derived consequence.
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self definitional
[Section 'Pseudo-Conformal Sound Speed at High Density', Eqs. (14)-(16)]
"The crucial point in the formalism is that ⟨θμ μ⟩ may not be zero but its derivative with respect to density could be zero because of the density-independent m0 to which ⟨χ̂⟩∗ tends to [29]. Thus ∂/∂n ⟨θμ μ⟩ = ∂ϵ(n)/∂n (1 − 3 v_s^2/c^2) = 0 (15) ... Now taking that there are no Lee-Wick states in the density range involved, i.e., ∂ϵ(n)/∂n ̸= 0, one arrives at the pseudo-conformal sound speed v_pcs^2/c^2 ≈ 1/3. (16)"
Eq. (15) is the exact thermodynamic identity ∂(ε−3P)/∂n = (∂ε/∂n)(1−3v_s^2), so setting the left side to zero and dividing by nonzero ∂ε/∂n gives Eq. (16) tautologically. The only physical input is the premise ∂⟨θ⟩/∂n = 0, which the paper asserts from the half-skyrmion m0 picture but does not derive here. Thus the 'prediction' v_s^2 ≈ 1/3 is a restatement of the assumed density-independence of the trace anomaly, not an independent consequence of the IR fixed point.
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self definitional
[Section 'Pseudo-Conformality: Manifestation in Crystal Lattice', bullet 'Dilaton-limit fixed point', Eq. (2)]
"The elimination of these singular terms gives what is referred to as 'dilaton-limit-fixed-point (DLFP)' constraints gV → gA → 1, fπ → fχ̄ ̸= 0. (2) ... The constraints (2) support two important predictions of the theory: 1. gA → 1 as density approaches n ≈ nDLFP."
The 'prediction' that g_A → 1 at the DLFP is literally one of the constraints in Eq. (2), imposed by the fixed-point construction ('elimination of these singular terms'), not a consequence derived from QCD or from the Landau calculation. The low-density g_A^L ≈ 1 from Eq. (5) carries independent content, but the high-density end of the claimed chain restates the DLFP assumption as a prediction.
1 more flagged steps
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self citation load bearing
[Section 'Pseudo-Conformal Sound Speed at High Density', bullet 'Emergent parity doubling and vpcs']
"As detailed in these articles, in half-skyrmion phase at high density, the interplay between the diltaon χ̂ and the vector meson ω after the charged vector mesons get decoupled forces the VEV of the χ̂ field tend to go to density-independent m0 in the nucleon mass which renders the VEV of the trace of energy-momentum tensor θμ μ independent of density in the range of density relevant to compact stars."
This sentence supplies the entire physical premise behind Eq. (16), but it is delegated to [32,43] (and [29] just above), prior work by the same author/group. The density-independent ⟨χ̂⟩*, and hence density-independent ⟨θ⟩, is not demonstrated in this paper; the compact-star sound-speed 'prediction' is an imported assumption from the author's own skyrmion/DLFP framework rather than a consequence worked out here.
full rationale
The paper's two headline quantitative outputs reduce partly to their own inputs. Eq. (15) is the exact thermodynamic identity ∂(ε−3P)/∂n = (∂ε/∂n)(1−3v_s^2); setting it to zero and dividing by nonzero ∂ε/∂n yields Eq. (16), so v_s^2 ≈ 1/3 is the assumed density-independence of the trace anomaly rewritten. The paper imports that density-independence from same-author prior work ([29], [32], [43]) rather than deriving it in this manuscript, and the scale invariance of normalized field configurations in Eq. (1) does not by itself imply ∂⟨χ̂⟩*/∂n = 0 because the normalization may absorb an overall density-dependent scale. Similarly, the high-density prediction g_A → 1 is one of the DLFP constraints in Eq. (2), so it is the fixed-point ansatz restated as a prediction. The low-density g_A^L ≈ 1 result from the Landau Fermi-liquid formula (5) does have independent calculational content, and the explicit RIKEN/GSI confrontation gives the scenario a genuine falsifier, which prevents a higher score. Nevertheless, the central claim that quenched g_A and v_s^2 ≈ 1/3 are two manifestations of one emergent hidden scale symmetry is an interpretation built on premises that are, in the key equations, identical to the outputs. Score 6 reflects this partial circularity: some predictions reduce by construction, while the low-density Landau calculation and external QCD IR-fixed-point literature remain independent.
Assumptions & free parameters
free parameters (4)
- n1/2, the skyrmion-to-half-skyrmion (HQC) transition density =
2.0-3.5 n0
- c_A (coefficient in q_ssb, Eq. (8)) =
not given ('incalculable')
- Landau(-Migdal) parameters F_1^π, F_1^ω, and m_L =
not tabulated here; from ref. [23] and Vlowk RG fits
- β'_IR =
0
assumptions (8)
- domain assumption QCD with N_f ≤ 3 has an infrared fixed point with a genuine (QCD-conformal) dilaton
- domain assumption f0(500) is the dilaton σ̂ of hidden scale symmetry
- domain assumption Nucleons in dense matter are described by the large-N_c skyrmion crystal down to compact-star densities
- domain assumption β'_IR = 0, the slope of the QCD beta function at the infrared fixed point vanishes
- domain assumption The GSI 100Sn measurement (g_A^eff ≈ 0.96) is the correct reference for the quasiparticle axial coupling
- domain assumption No Lee-Wick states in the density range of compact stars, so ∂ε(n)/∂n ≠ 0
- standard math Landau Fermi-liquid theory and Shankar-Polchinski RG apply to baryons on the Fermi surface
- domain assumption The large-N' Grassmannian model fixes the HLS parameter a = 2
invented entities (3)
-
'Quarkish' quasi-quark degrees of freedom at HQC
-
Half-skyrmions confined by monopoles
-
Emergent chiral-invariant nucleon mass m0 (parity-doubling partner)
Cite this review
Pith. "Pith review of From Nuclear Matter with Quenched $g_A$ to Compact-Star Matter with a Signal for Emergent Hidden Scale Symmetry." pith.science (2026). https://pith.science/paper/TVBASILF
@misc{pith2026250704939,
author = {Pith},
title = {Pith review of: From Nuclear Matter with Quenched $g_A$ to Compact-Star Matter with a Signal for Emergent Hidden Scale Symmetry},
year = {2026},
howpublished = {\url{https://pith.science/paper/TVBASILF}},
note = {Machine review of arXiv:2507.04939}
}
abstract
An ``unorthodox" idea is developed that the long-standing mystery in nuclear physics of the effective axial-current coupling constant in nuclei, $g_A^{\rm eff}\approx 1$, could be interpreted in terms of an emerging hidden scale symmetry in dense compact-star matter. Arguments are presented using an effective field theory anchored on a renormalization-group approach to interacting baryons on the Fermi surface coupled with hidden symmetric heavy mesonic degrees of freedom that enables one to go beyond Weinberg's nuclear effective field theory involving nucleon and pion fields only, referred hereon to as $\chi$EFT$_\pi$. Both hidden local and scale symmetries, the former involving the vector mesons $\rho$ and $\omega$ and the latter the hidden scalar meson, a dilaton $\hat{\sigma}$ (i.e., $f_0(500)$), play the crucial role. Going beyond the density regime applicable to normal nuclear matter $n_0$, the notion of ``hadron-quark continuity HQC)" is brought in via the skyrmion structure of the nucleon argued to be valid in QCD at large $N_c$ limit and the large $N^\prime$ limit of the Grassmannian model $G/H= [O(N^\prime)/O(N^\prime-p) \times O(p)]$ where $N^\prime=4$ and $p=2$ for hidden local symmetry and the IR fixed point in QCD for $N_f \leq 3$ involving ``genuine/QCD-conformal dilaton" for hidden scale symmetry. The connection between the quenched $g_A$ and the sound speed $v^2_{s}/c^2\approx 1/3$ inside dense compact stars could be interpreted as a signal for emergent ``pseudo-conformal" symmetry.
Figures
Forward citations
Cited by 1 Pith paper
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Half-life of $^{136}$Xe for neutrinoless double-$\beta$ decay calculated with effective axial-vector current coupling unified for two-neurtino and neutrinoless double-$\beta$ decay modes
For 136Xe, the predicted 0νββ half-life is (1.3-3.0)×10^31 y at ⟨mν⟩=1 meV, roughly ten times longer than the standard compilation, based on unifying the effective axial coupling of the 2ν and 0ν modes.
Reference graph
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This means that the effective quasiparticle geff A ≈ 1 in baryonic matter at some high density
gA → 1 as density approaches n ≈ nDLF P. This means that the effective quasiparticle geff A ≈ 1 in baryonic matter at some high density. At what density this sets in will be addressed later in con- nection with the proposed pseudo-conformal sound speed in compact stars
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H. K. Lee, “Parity doubling in dense baryonic matter as an emergent phenomenon and pseudo-conformal phase,” Symmetry 16, no.12, 1598 (2024)
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Axial currents in nuclei,
K. Kubodera, J. Delorme and M. Rho, “Axial currents in nuclei,” Phys. Rev. Lett. 40, 755-758 (1978)
1978
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Chiral symmetry and effective field theories for hadronic, nuclear and stellar matter,
J. W. Holt, M. Rho and W. Weise, “Chiral symmetry and effective field theories for hadronic, nuclear and stellar matter,” Phys. Rept. 621, 2-75 (2016) [arXiv:1411.6681 [nucl-th]]
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Nowak, M
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1996
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Anomaly-induced quenching of gA in nuclear matter and impact on search for neutrinoless ββ decay,
M. Rho, “Anomaly-induced quenching of gA in nuclear matter and impact on search for neutrinoless ββ decay,” Symmetry 15, no.9, 1648 (2023)
2023
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C.B. Henke et al. , “Superallowed Gamow-Teller decay of the doubly magic nucleus 100Sn,” Nature 486, 341 (2012)
2012
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Improved value for the Gamow-Teller strength of the 100Sn beta decay,
D. Lubos et al. , “Improved value for the Gamow-Teller strength of the 100Sn beta decay,” Phys. Rev. Lett. 122, 222502 (2019)
2019
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Chiral effective field theory calculations of weak transitions in light nuclei,
G. B. King, L. Andreoli, S. Pastore, M. Piarulli, R. Schi- avilla, R. B. Wiringa, J. Carlson and S. Gandolfi, “Chiral effective field theory calculations of weak transitions in light nuclei,” Phys. Rev. C 102, no.2, 025501 (2020)
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J.T. Suhonen, “Value of the axial-vector coupling strength in β and ββ decays: A Review,” Front. in Phys. 5, 55 (2017); J. Engel and J. Men` endez, “Status and fu- ture of nuclear matrix elements for neutrinoless double- beta decay: A review,” Rept. Prog. Phys. 80, 046301 (2017)
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Corrections to Landau Fermi- liquid fixed-point approximation in nonlinear bosonized theory: An application to gL A in nuclei,
L. Q. Shao and M. Rho, “Corrections to Landau Fermi- liquid fixed-point approximation in nonlinear bosonized theory: An application to gL A in nuclei,” Phys. Rev. C 110, no.1, 015204 (2024). 12
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Nuclear matter and finite nuclei: Recent studies based on parity doublet model,
Y. K. Kong, Y. Kim and M. Harada, “Nuclear matter and finite nuclei: Recent studies based on parity doublet model,” Symmetry 16, no.9, 1238 (2024)
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Inter- play between ω-nucleon interaction and nucleon mass in dense baryonic matter,
W. G. Paeng, H. K. Lee, M. Rho and C. Sasaki, “Inter- play between ω-nucleon interaction and nucleon mass in dense baryonic matter,” Phys. Rev. D 88, 105019 (2013)
2013
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Scale-invariant hidden local symmetry, topology change and dense baryonic matter,
W. G. Paeng, T. T. S. Kuo, H. K. Lee and M. Rho, “Scale-invariant hidden local symmetry, topology change and dense baryonic matter,” Phys. Rev. C 93, no.5, 055203 (2016)
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The equation of state of nucleon matter and neutron star structure,
A. Akmal, V. R. Pandharipande and D. G. Ravenhall, “The equation of state of nucleon matter and neutron star structure, ”Phys. Rev. C 58, 1804-1828 (1998)
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Dense baryonic matter predicted in “pseudo- conformal model
M. Rho, “Dense baryonic matter predicted in “pseudo- conformal model”,” Symmetry 15, no.6, 1271 (2023)
2023
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Implications of latest NICER data for the neutron star equation of state,
L. Brandes and W. Weise, “Implications of latest NICER data for the neutron star equation of state,” Phys. Rev. D 111, no.3, 034005 (2025); “Constraints on phase tran- sitions in neutron star matter,” Symmetry 16, no.1, 111 (2024)
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Perturbative QCD reveals the soften- ing of matter in the cores of massive neutron stars,
O. Komoltsev, “Perturbative QCD reveals the soften- ing of matter in the cores of massive neutron stars,” [arXiv:2506.06465 [astro-ph.HE]]; E. Finch, I. Legred, K. Chatziioannou, R. Essick, S. Han and P. Landry, “Unified nonparametric equation-of-state inference from the neutr...
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Pseudo-conformal sound speed in the core of compact stars,
M. Rho, “Pseudo-conformal sound speed in the core of compact stars,” Symmetry 14, no.10, 2154 (2022), [arXiv:2209.02327 [nucl-th]]
2022 arXiv
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Evidence for quark-matter cores in massive neutron stars,
E. Annala, T. Gorda, A. Kurkela, J. N¨ attil¨ a and A. Vuorinen, “Evidence for quark-matter cores in massive neutron stars,” Nature Phys. 16, no.9, 907-910 (2020)
2020
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Qualitons at high density,
D. K. Hong, M. Rho and I. Zahed, “Qualitons at high density,” Phys. Lett. B 468, 261-269 (1999) [arXiv:hep- ph/9906551 [hep-ph]]
1999
Reviewed August 6, 2026 · model on record in the stance chip above.
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