REVIEW
The Condensed Matter Physics of QCD
High Energy Physics - Phenomenology · Submitted 27 Nov 2000 · 146 references
Pith's verdict: The 2000 Handbook survey that fixed the vocabulary of color superconductivity: the symmetry analysis has held up, the gap numbers were always provisional, and the paper says so itself.
Why Pith says this
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Referee report
The paper
The paper claims
At high enough density, three-flavor quark matter locks color to flavor, gaps every quark and gluon, and may connect continuously to hypernuclear matter.
The reading
What carries the argument
Two tools carry the argument. First, renormalization toward the Fermi surface: integrating out modes in a shell around the Fermi surface shows that four-fermion couplings in the color-antitriplet, flavor-antitriplet, scalar diquark channel grow without bound as $dG/dln delta = -kappa G^2$, so any attractive interaction, however weak, produces a pairing instability. Second, BCS/Nambu-Jona-Lasinio gap equations, solved variationally and diagrammatically, turn that instability into a gap. The paper also shows that the asymptotic gap is not $exp(-c/g^2)$ as a contact interaction would give, but $Delta/mu sim b,g^5 exp(-3pi^2/(sqrt{2},g))$, because near-forward magnetic gluon exchange is logarithmically enhanced and cut off by dynamical screening rather than by the Meissner effect.
Extended reading notes
Core claim
The central claim is that in QCD with three colors and three massless flavors, the high-density ground state carries a diquark condensate $langle psi^{a}_{alpha i L}(p), psi^{b}_{beta j L}(-p), epsilon_{ab} rangle = Delta(p^2), epsilon_{alpha beta A}, epsilon_{ijA}$, with an equal and opposite right-handed piece, so that the state is a parity-preserving scalar. This is color-flavor locking: neither color nor chiral flavor rotations alone leave the condensate invariant, but simultaneous rotations of color, left-handed flavor, and right-handed flavor do. The consequences the paper draws are that all nine quarks acquire gaps (an octet gap and a larger singlet gap), all eight gluons acquire masses by the Meissner-Anderson-Higgs mechanism, and a linear combination of the photon and the $T_8$ gluon, $tilde Q = Q + eta T_8$ with $eta = 1/sqrt{3}$, remains massless, so every elementary excitation carries an integer charge in units of a slightly reduced electron charge. Because the surviving symmetries match those expected of three-flavor hypernuclear matter, the paper advances a quark-hadron continuity conjecture: no phase transition need separate nuclear matter from the color-flavor locked phase in the three-flavor world.
Load-bearing premise
The tens-of-MeV gap estimates at accessible densities come from a four-fermion coupling fixed to reproduce a 400 MeV constituent quark mass in vacuum and then carried unchanged to the dense phase, and the paper itself shows the gap shrinking roughly in proportion when that coupling is halved.
Editorial extensions
If this is right
- All colored excitations are gapped and all gluons massive in the three-flavor phase, so weak-coupling perturbation theory around the true ground state is free of the infrared divergences that spoil perturbation theory around the naive ground state.
- The low-energy spectrum contains a pseudoscalar octet of Nambu-Goldstone bosons whose masses and decay constant are computable from first principles at high density; the kaon comes out lighter than the pion by a factor of $m_d/(m_u+m_d)$.
- A rotated photon remains massless and all excitations carry integer charge, reproducing a defining feature of confinement inside a controlled weak-coupling calculation.
- The three-flavor phase has the same symmetries as hypernuclear matter, so in a world of three degenerate quarks there need be no phase transition between nuclear and quark matter.
- Any quark matter in a neutron star more than a few seconds old must be color superconducting, since the critical temperature is of order tens of MeV while star interiors are at tens of keV.
Reading between the lines
- The continuity conjecture suggests a practical search strategy: if the transition is smooth, the pseudoscalar meson masses and decay constants should evolve continuously across the density where quarks replace baryons as the convenient variables, which is in principle checkable by comparing hypernuclear models with high-density effective-theory results.
- The paper's own numbers show the gap scales roughly linearly with the model coupling: halving $G$ takes $Delta_8$ from 80 MeV to 16 MeV at $mu = 500$ MeV, so the quoted tens-of-MeV gaps are really a statement about the assumed strength of the attraction, not a first-principles prediction at accessible density.
- Because the asymptotic result makes $Delta$ grow logarithmically with $mu$ while $m_s^2/(2mu)$ falls, the color-flavor locked phase wins over the two-flavor phase at sufficiently high density for any finite strange quark mass, which turns the phase-diagram question into a quantitative one about where the unlocking transition sits.
- The rotated-photon construction is a template: whenever a condensate breaks a gauge group and a global flavor group together, the unbroken combination can be found by the same generator-mixing calculation, which suggests analogous mixed symmetries in other dense or condensed systems with multiple simultaneous broken symmetries.
Original abstract
Important progress in understanding the behavior of hadronic matter at high density has been achieved recently, by adapting the techniques of condensed matter theory. At asymptotic densities, the combination of asymptotic freedom and BCS theory make a rigorous analysis possible. New phases of matter with remarkable properties are predicted. They provide a theoretical laboratory within which chiral symmetry breaking and confinement can be studied at weak coupling. They may also play a role in the description of neutron star interiors. We discuss the phase diagram of QCD as a function of temperature and density, and close with a look at possible astrophysical signatures.
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
Important progress in understanding the behavior of hadronic matter at high density has been achieved recently, by adapting the techniques of condensed matter theory. At asymptotic densities, the combination of asymptotic freedom and BCS theory make a rigorous analysis possible. New phases of matter with remarkable properties are predicted. They provide a theoretical laboratory within which chiral symmetry breaking and confinement can be studied at weak coupling. They may also play a role in the description of neutron star interiors. We discuss the phase diagram of QCD as a function of temperature and density, and close with a look at possible astrophysical signatures.
background contribution method result interpretation main claim
| # | sentence | role | the authors' own work | states the main conclusion | strength |
|---|---|---|---|---|---|
| s0 | Important progress in understanding the behavior of hadronic matter at high density has been achieved recently, by adapting the techniques of condensed matter theory. | background 0.93 | 0.11 | 0.13 | asserted 1.00 |
| s1 | At asymptotic densities, the combination of asymptotic freedom and BCS theory make a rigorous analysis possible. | method 0.49 | 0.08 | 0.07 | asserted 0.99 |
| s2 | New phases of matter with remarkable properties are predicted. | result 0.91 | 0.23 | 0.24 | asserted 0.73 |
| s3 | They provide a theoretical laboratory within which chiral symmetry breaking and confinement can be studied at weak coupling. | interpretation 0.95 | 0.13 | 0.12 | asserted 0.97 |
| s4 | They may also play a role in the description of neutron star interiors. | interpretation 0.93 | 0.08 | 0.07 | hedged possibility 1.00 |
| s5 | We discuss the phase diagram of QCD as a function of temperature and density, and close with a look at possible astrophysical signatures. | contribution 0.98 | 0.75 | 0.14 | asserted 0.48 |
What was examined, and what was not
- arXiv listing abstract v2
- full text
- figures and tables
- references and citing sentences
- relations to other papers
- P abstract
- S sections
- T body sentences
- C citations
- R cross-paper relations
Figures
Figures reproduced from arXiv:hep-ph/0011333 by the authors.
References
How the literature uses it
236 arXiv papers cite this in 319 sentences
Papers citing it · 111 sentences without a confident label
Uses its method or tool 1 paper
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To resolve this problem, in this section we describe vortices in the CFL phase in a gauge-invariant manner [ref] using diquarks in Eqs. [ref] and [ref] as building blocks.
Continuity of vortices from the hadronic to the color-flavor locked phase in dense matter · Gauge-invariant description · 0.90
Uses its data or values 1 paper
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They show some agreement and suggest $Δ∼20-100 MeV$ [ref] for $μ_q≈400-500 MeV$.
Superconducting phases of strongly-interacting matter in large magnetic fields · The $μ_B$-$T$ plane at $B=0$ · 0.86
Compares with it 2 papers
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For completeness, however, we add that the functional form of the expansion [ref] at LO/LO agrees with the one obtained for the pressure in Nambu-Jona-Lasinio-type model calculations at that order, see, e.g., Refs. [ref] .] In all cases, the overall scale of the gap is fixed to be $Δ_∗ = 100$.
Pressure and speed of sound in two-flavor color-superconducting quark matter at next-to-leading order · Pressure · 0.83
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There is a similar dip in the phase diagram of QCD (see for example [ref] ).
Holographic Nuclear Physics · phase diagram · 0.97
Cites it as background 174 papers
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The condensation pattern that is considered here is the color-flavor-locked (CFL) phase [ref] where quarks of all colors and flavors pair together to form Cooper pairs.
The Meissner Effect and Vortex Expulsion in Color-Superconducting Quark stars, and its Role for Re-heating of Magnetars · The Vortex Expulsion Mechanism · 0.92
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At asymptotic densities, where the up, down and strange quarks can be treated on an equal footing and effects due to the strange quark mass can be neglected, quark matter is in the color flavor locked (CFL) phase [ref] .
Collective modes in the color flavor locked phase · Introduction · 0.80
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At asymptotic densities, where the up ($u$), down ($d$) and strange ($s$) quarks can all be treated as massless, quark matter is in the Color Flavor Locked (CFL) phase [ref] .
The rigidity of three flavor quark matter · Introduction · 0.91
Discussion
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