REVIEW
Emergence of Skyrme crystal in Gross-Neveu and 't Hooft models at finite density
High Energy Physics - Theory · Submitted 22 Mar 2000 · 47 references
Pith's verdict: A clean, well-argued fix to a real inconsistency in dense 1+1 large-N matter; the only overreach is a figure caption, not the physics.
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Referee report
The paper
The paper claims
The paper argues that in two-dimensional large-$N$ models with broken chiral symmetry, baryonic matter at any nonzero density is not a homogeneous quark gas but a spatially modulated chiral spiral whose winding number counts the baryons.
The reading
What carries the argument
The load-bearing object is the chirally rotated vacuum density matrix $p_f(x,y) = e^{i p_f(x)-2p_f(y)}$ in the form $e^{i p_f(x)-2p_f(y)}$ of Eq. (37), $p_f(x,y)=e^{i p_f(x)-2p_f(y)}$, i.e. $e^{i p_f(x)-2p_f(y)}$ with a space-dependent chiral angle inserted between the vacuum density matrix and its conjugate. Two facts make it work. First, the baryon density is the gradient of the angle, $p_f(x) = (1/2p_i)p_f$, so baryon number is a topological winding number and cannot be removed by a small deformation. Second, local chiral invariance of the interaction means the potential energy is untouched by the rotation, so the energy functional reduces to a free gradient term $N p_f^2/2p_i$ whose minimization gives a linear phase. With a bare mass $m_q$ the same functional plus the mass term becomes the sine-Gordon energy, $p_f^2/2p_i$ plus $m_q$ times the condensate, yielding $m_pi^2 = -4p_i m_q p_f$ and the kink chain of Jacobi elliptic functions determined by $p_i m_pi/p_f = 2kK(k)$.
Extended reading notes
Core claim
The central claim is that the true ground state of baryonic matter in these models is a spatially varying chiral angle $p_f(x-x_0)$ rather than a homogeneous Fermi sea, and that the conventional first-order chiral phase transition found in the Gross-Neveu model is an artifact of assuming translational invariance. The argument proceeds by taking the Skyrme-type variational density matrix $e^{i p_f x-2p_f x_0}$-style rotation of the vacuum, $e^{i p_f x-2p_f x_0}$ in the form $e^{i p_f x-2p_f x_0}$ of Eq. (37), for which the baryon density is $(1/2p_i)p_f$ and the baryon number is the winding number of the phase. Because the interaction is locally chirally invariant, the potential energy of this state equals the vacuum energy, so the whole energy cost is the gradient term $N p_f^2/2p_i$, giving $E/N = p_f^2/2p_i$ after subtracting the vacuum. The authors check that this state is energetically favored over both the homogeneous and the mixed-phase (bag-like) Hartree-Fock solutions at every density, that it is convex in $p_f$, and that its slope at $p_f=0$ vanishes, as it must if the baryon is massless. They further show that in the chiral limit the ansatz is an exact solution of the Hartree-Fock equation to leading order in $1/N$: substituting the chirally rotated spinor into the 't Hooft Hartree-Fock equation leaves the equation intact with single-particle energies shifted by $p_f$.
Load-bearing premise
The load-bearing premise is that the family of chirally rotated vacuum density matrices contains the true ground state at every density, so that comparing its energy only against homogeneous and mixed-phase Hartree-Fock states establishes that it is the minimum; the authors themselves leave the finite-mass variational ansatz's validity at intermediate density open, relying on numerical single-baryon results at low density and on the exact chiral-limit argument at high density.
Editorial extensions
If this is right
- Dense matter in these models has no chiral phase transition: the energy density is convex and smooth in $p_f$ at all densities, so the first-order transition and the mixed-phase construction usually quoted for the Gross-Neveu model are replaced by a single crystalline phase.
- Because the state is invariant only under a simultaneous translation and chiral rotation, the excitation spectrum should contain exactly one gapless collective mode, a hybrid of a phonon and a pion, rather than separate acoustic and Goldstone branches.
- The chiral limit of the 't Hooft model becomes tractable at finite density: the confining theory's infinite quark self-energy no longer obstructs a finite-energy ground state, since the crystal costs no potential energy beyond the vacuum.
- For small bare quark masses the low-density limit reproduces the known single-baryon mass, $E \approx M_B p_f$ with $M_B = 2N m_pi/p_i$, and the high-density limit reproduces the chiral spiral, so the same formula interpolates between the baryon and quark-matter pictures.
- The same construction should apply to any large-$N$ field theory whose interaction is locally chirally invariant, which is why the authors expect it to be generic rather than a two-dimensional accident.
Reading between the lines
- If the chiral spiral is the true ground state, then lattice or continuum Hartree-Fock studies of the Gross-Neveu phase diagram that assume homogeneous matter are not merely quantitatively inaccurate near the transition but describe a state that is never realized; the discrete-symmetry variant, whose baryons are massive, may also need re-examination.
- The mechanism looks like a field-theoretic analogue of spin- or charge-density-wave ordering: a Fermi surface instability that costs no potential energy because the interaction is invariant under the local rotation used to build the modulation, which suggests the same construction could be tested in condensed-matter models with local chiral or pseudospin symmetry.
- A natural check the authors do not perform is a full two-dimensional lattice Hartree-Fock minimization at intermediate density and finite $m_q$, comparing the kink-chain energy against arbitrary inhomogeneous configurations; such a calculation would either confirm the variational ansatz or exhibit a lower-lying state.
- The identification of the ground state as a Skyrme crystal in 1+1 dimensions suggests a direct translation of the winding-number-counts-baryons argument to the three-dimensional Skyrme crystal, where the same gradient energy would fix the lattice spacing in terms of the density.
Original abstract
We study two-dimensional, large $N$ field theoretic models (Gross-Neveu model, 't Hooft model) at finite baryon density near the chiral limit. The same mechanism which leads to massless baryons in these models induces a breakdown of translational invariance at any finite density. In the chiral limit baryonic matter is characterized by a spatially varying chiral angle with a wave number depending only on the density. For small bare quark masses a sine-Gordon kink chain is obtained which may be regarded as simplest realization of the Skyrme crystal for nuclear matter. Characteristic differences between confining and non-confining models are pointed out.
The compiled record
The paper's own sentences, arranged, kept beside the review and separate from it. Each label is drawn from a closed vocabulary; the number beside it is the probability the classifier gave that label. Numbers in the tables are the authors', checked by code. No sentence in this record was written by a model.
The abstract, sentence by sentence
We study two-dimensional, large $N$ field theoretic models (Gross-Neveu model, 't Hooft model) at finite baryon density near the chiral limit. The same mechanism which leads to massless baryons in these models induces a breakdown of translational invariance at any finite density. In the chiral limit baryonic matter is characterized by a spatially varying chiral angle with a wave number depending only on the density. For small bare quark masses a sine-Gordon kink chain is obtained which may be regarded as simplest realization of the Skyrme crystal for nuclear matter. Characteristic differences between confining and non-confining models are pointed out.
background contribution method result interpretation main claim
| # | sentence | role | the authors' own work | states the main conclusion | strength |
|---|---|---|---|---|---|
| s0 | We study two-dimensional, large $N$ field theoretic models (Gross-Neveu model, 't Hooft model) at finite baryon density near the chiral limit. | contribution 0.93 | 0.87 | 0.04 | asserted 0.84 |
| s1 | The same mechanism which leads to massless baryons in these models induces a breakdown of translational invariance at any finite density. | result 0.86 | 0.75 | 0.60 | asserted 1.00 |
| s2 | In the chiral limit baryonic matter is characterized by a spatially varying chiral angle with a wave number depending only on the density. | result 0.99 | 0.80 | 0.26 | asserted 1.00 |
| s3 | For small bare quark masses a sine-Gordon kink chain is obtained which may be regarded as simplest realization of the Skyrme crystal for nuclear matter. | result 0.70 | 0.83 | 0.33 | hedged possibility 0.98 |
| s4 | Characteristic differences between confining and non-confining models are pointed out. | contribution 0.50 | 0.78 | 0.05 | asserted 0.78 |
What was examined, and what was not
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Figures
Showing 5 of the paper's 11 figures. See all figures in the PDF ↗ Figures reproduced from arXiv:hep-th/0003195 by the authors.
References
How the literature uses it
33 arXiv papers cite this in 68 sentences
Papers citing it · 48 sentences without a confident label
Contests it 1 paper
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This, if correct, contradicts simple physical intuition (and of course contradicts all the results of Refs. [ref] and of the current paper).
Solving two-dimensional large-N QCD with a nonzero density of baryons and arbitrary quark mass · Summary and conclusions · contest 0.81
Builds on it 1 paper
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The solution is obtained by extending to generic $a$ the methods employed in [ref] .
Perturbative, Nonperturbative and Exact Aspects of Crystalline Phases in the Gross-Neveu Model · Summary of results · 0.91
Uses its data or values 1 paper
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Let us denote the dimensionless combination $n^c_B/√(g^2N)$ by $x^c$.[Ref. [ref] get $x^c≃0.0149$.] This can be visualized in a simple phase diagram in the space $B$—$L√(g^2N)$ that we present in Fig. ([ref]).
Volume dependence of two-dimensional large-N QCD with a nonzero density of baryons · Full translation symmetry · 0.98
Compares with it 3 papers
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In this section we derive the critical temperature $T_c$ of the cGN model, reproducing the result of [ref] with a different method.
On the Inhomogeneous Phase of the Chiral Gross-Neveu Model · Chiral spiral at large $N$ · 0.91
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In Fig. [ref] we present the baryon density for the light quark case and compare to the predictions of the sine-Gordon crystal – see [ref] .
Solving two-dimensional large-N QCD with a nonzero density of baryons and arbitrary quark mass · Finite density and the equation of state · 1.00
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* Ref. [ref] : To our knowledge this paper is the only one that solves the `t Hooft equation at nonzero baryon number for a general ratio $√(g^2N)/m$.[Another paper that discusses nonzero baryon number in the `t Hooft model is [ref] , but there the authors restrict to translation invariant dense systems, which as they show, is inconsistent.
Volume dependence of two-dimensional large-N QCD with a nonzero density of baryons · Comparison to other relevant works · 0.81
Cites it as support 1 paper
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Schon and Thies showed that at nonzero quark density, the quark propagator remains infrared divergent, and so confined, as it is in vacuum [ref] .
Phases of Dense Quarks at Large N_c · Quarkyonic Matter at Large $N_c$ · 0.97
Cites it as background 11 papers
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In these models, a chemical potential $μ_f$ for a given flavor spinor $χ$ leads to spiral behavior [ref] of the condensate $Δ≡(χ̅χ)- i(χ̅iΓ^5χ)$, which combines the scalar and pseudoscalar condensate into a single complex condensate.
Chiral Magnetic Spiral · Introduction · 0.92
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Many attempts have been made to study the problem: Ref. [ref] studies the problem in the chiral limit, where baryons assume the form of a Sine-Gordon soliton.
Baryons and Low-Density Baryonic Matter in 1+1 Dimensional Large N_c QCD with Heavy Quarks · Introduction · 0.98
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With this manuscript we particularly do not intend to bring up new findings regarding the phase structure of the chgn model in the mean-field approximation, which was already derived in Refs. [ref] and will be discussed below.
Revisiting the spatially inhomogeneous condensates in the $(1 + 1)$-dimensional chiral Gross-Neveu model via the bosonic two-point function in the infinite-$N$ limit · Research objective · 0.92
Discussion
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