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Bump of sound velocity in dense 2-color QCD
High Energy Physics - Lattice · Submitted 25 Oct 2022
abstract compiled · 2026-09-23 · no language-model review
The authors' main claim We obtain the equation of state (EoS) and the sound velocity for 2-color QCD at low temperature and high density and find that in the superfluid phase, $c_s^2/c^2 >1/3$, where $1/3$ is the value at the relativistic limit.
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The abstract, sentence by sentence
We obtain the equation of state (EoS) and the sound velocity for 2-color QCD at low temperature and high density and find that in the superfluid phase, $c_s^2/c^2 >1/3$, where $1/3$ is the value at the relativistic limit. Several independent Monte Carlo studies on 2-color QCD have been conducted intensively in recent years. These works have shown a clear evidence of phase transition between hadronic and superfluid phases. In our paper[1], we have investigated the EoS and sound velocity in both phases. Our result is consistent with chiral perturbation theory in a low $\mu$ regime of the superfluid phase including the Bose-Einstein condensed phase, and shows a peak of sound velocity in the high-density BCS phase. We also give detailed simulation results and a comment on the holography bound in this proceedings.
background contribution method result interpretation main claim
| # | sentence | role | the authors' own work | states the main conclusion | strength |
|---|---|---|---|---|---|
| s0 | We obtain the equation of state (EoS) and the sound velocity for 2-color QCD at low temperature and high density and find that in the superfluid phase, $c_s^2/c^2 >1/3$, where $1/3$ is the value at the relativistic limit. | result 0.98 | 0.97 | 0.87 | asserted 1.00 |
| s1 | Several independent Monte Carlo studies on 2-color QCD have been conducted intensively in recent years. | background 1.00 | 0.04 | 0.02 | asserted 1.00 |
| s2 | These works have shown a clear evidence of phase transition between hadronic and superfluid phases. | background 1.00 | 0.05 | 0.03 | asserted 1.00 |
| s3 | In our paper[1], we have investigated the EoS and sound velocity in both phases. | contribution 0.95 | 0.94 | 0.05 | asserted 0.98 |
| s4 | Our result is consistent with chiral perturbation theory in a low $\mu$ regime of the superfluid phase including the Bose-Einstein condensed phase, and shows a peak of sound velocity in the high-density BCS phase. | result 0.82 | 0.93 | 0.29 | asserted 0.70 |
| s5 | We also give detailed simulation results and a comment on the holography bound in this proceedings. | contribution 0.97 | 0.86 | 0.03 | asserted 0.97 |
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The paper
Original abstract
We obtain the equation of state (EoS) and the sound velocity for 2-color QCD at low temperature and high density and find that in the superfluid phase, $c_s^2/c^2 >1/3$, where $1/3$ is the value at the relativistic limit. Several independent Monte Carlo studies on 2-color QCD have been conducted intensively in recent years. These works have shown a clear evidence of phase transition between hadronic and superfluid phases. In our paper[1], we have investigated the EoS and sound velocity in both phases. Our result is consistent with chiral perturbation theory in a low $\mu$ regime of the superfluid phase including the Bose-Einstein condensed phase, and shows a peak of sound velocity in the high-density BCS phase. We also give detailed simulation results and a comment on the holography bound in this proceedings.
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References
How the literature uses it
6 arXiv papers cite this in 11 sentences
Papers whose main result relates to this one's
States the same result 2 papers
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We find that the velocity of sound exceeds the relativistic limit ($c_s^2/c^2=1/3$) after BEC-BCS crossover in the superfluid phase.
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However, our recent work~\cite{Iida:2022hyy} shows the breaking of this bound in dense QC$_2$D.
Speed of sound exceeding the conformal bound in dense 2-color QCD · 0.90
Papers citing it · 4 sentences without a confident label
Uses its method or tool 2 papers
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At nonzero chemical potential, one can follow a similar strategy to calculate the modifications of pressure and interaction measure using $μ=0$ subtraction (see, e.g., Ref. [ref] and Refs. [ref] ).
Equation of state and speed of sound of isospin-asymmetric QCD on the lattice · The EoS from an interpolation of the isospin density · 0.91
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We use the same lattice setup as that used in our previous works [ref] .
Chemical potential (in)dependence of hadron scatterings in the hadronic phase of QCD-like theories and its applications · Lattice Setups · 0.98
Compares with it 3 papers
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The non-monotonic profile of $C^2_S$ [ref] becomes apparent and visible as $κ→1$ , similar to inferred in numerous works for cold NS matter [ref] and contrary to the results in Ref. [ref] .
Observables and conformal properties of dark matter admixed isentropic neutron stars · Speed of Sound · 0.83
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We note that our finding of $c_s^2>1/3$, as well as the development of a peak is in good agreement with recent results obtained in two-color QCD [ref] (see also [ref] ).
Equation of state and speed of sound of isospin-asymmetric QCD on the lattice · Speed of sound at vanishing temperature · 0.98
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Our findings are in good agreement with recent results obtained in two-color QCD [ref] .
Equation of state and Taylor expansions at nonzero isospin chemical potential · The speed of sound · 0.99
Cites it as background 1 paper
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In recent years, lattice Monte Carlo studies on dense QC$_2$D have been conducted independently and intensively by several groups [ref] .
Lattice study on finite density QC$_2$D towards zero temperature · Introduction · 0.95
What it cites · 15 sentences without a confident label
Uses the method or tool of 2 papers
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Now, we utilize a fixed scale method to obtain the EoS at finite density [ref] .
Deconfinement in dense 2-color QCD · Equation of state and velocity of sound at finite $μ$ · 1.00
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To obtain the extrapolated value at $j=0$, we perform the reweighting of $j$ and take the linear extrapolation (see Fig.8 in Ref. [ref] ).
Two-colour QCD phases and the topology at low temperature and high density · Simulation results · 0.97
Uses data or values from 1 paper
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phase structure in Fig. [ref] and summarize the definition of each phase in Table [ref], which is an extract from Ref. [ref] .
Two-colour QCD phases and the topology at low temperature and high density · Phase structure at $T=79$ MeV · 0.84
Compares with 4 papers
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First of all, our results are consistent with the prediction of ChPT [ref] , which is given by $c_s^2/c^2=(1-μ_c^4/μ^4)/(1+3μ_c^4/μ^4)$, in the BEC phase.
Deconfinement in dense 2-color QCD · Simulation results · 0.93
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On the other hand, a result based on the resummed perturbation theory suggests that $c_s^2/c^2$ approaches the limit from above [ref] .
Equation of state of cold and dense QCD matter in resummed perturbation theory · Summary and discussion · 0.92
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For example, in the finite temperature case, the sound velocity monotonically increases in $T>T_c$ and approaches the relativistic limit as the temperature increases [ref] .
Full result for the QCD equation of state with 2+1 flavors · Simulation results · 0.93
Cites as support 2 papers
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It supports the predictions from several effective models based on the presence of the quark Fermi sea [ref] .
Stiffening of matter in quark-hadron continuity · Summary and discussion · 0.96
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It supports the predictions from several effective models based on the presence of the quark Fermi sea [ref] .
Peaks of sound velocity in two color dense QCD: quark saturation effects and semishort range correlations · Summary and discussion · 0.96
Cites as background 2 papers
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Based on this motivation, several Monte Carlo studies on $2$-color QCD have been conducted independently and intensively in recent years (see references in Ref. [ref] ).
Velocity of Sound beyond the High-Density Relativistic Limit from Lattice Simulation of Dense Two-Color QCD · Introduction · 0.93
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Several early works based on a phenomenological quark-hadron crossover picture of neutron star matter [ref] suggested that the zero-temperature sound velocity squared, $c_s^2=∂p/∂e$, peaks in $n_B = 1$–$10n_o$ to be consistent with various observational constraints.
From hadrons to quarks in neutron stars: a review · Introduction · 0.91
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