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Velocity Dependence of Baryon Screening in a Hot Strongly Coupled Plasma

High Energy Physics - Theory · Submitted 7 Jan 2008

abstract compiled · 2026-09-23 · no language-model review

The authors' main claim We find that in the v -> 1 limit, Ls \propto (1-v^2)^{1/4}/T, and find that corrections to this velocity dependence are small at lower velocities.

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arXiv ID0801.1117 (version 3)
Pith ID27W7XBNP, Pith's permanent record of this paper and its review
CitationChristiana Athanasiou, Hong Liu, Krishna Rajagopal. "Velocity Dependence of Baryon Screening in a Hot Strongly Coupled Plasma." arXiv:0801.1117 (2008). https://pith.science/paper/27W7XBNP
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What the abstract itself states, as probabilities: claims first 0.05 · states limitation 0.85 · human participants 0.01 · controlled comparison 0.14 · randomized assignment 0.01 · states quantitative result 0.81 · compares with prior results 0.92 · mentions code or data availability 0.02.

The abstract, sentence by sentence

arXiv listing abstract v3. Results and the main claim are underlined; .

The L-dependence of the static potential between Nc quarks arranged in a circle of radius L (a "baryon") immersed in the hot plasma of a gauge theory with Nc colors defines a screening length Ls. We use the AdS/CFT correspondence to compute this screening length for the case of heavy quarks in the plasma of strongly coupled N=4 super Yang-Mills theory moving with velocity v relative to the baryon. We find that in the v -> 1 limit, Ls \propto (1-v^2)^{1/4}/T, and find that corrections to this velocity dependence are small at lower velocities. This result provides evidence for the robustness of the analogous behavior of the screening length defined by the static quark-antiquark pair, which has been computed previously and in QCD is relevant to quarkonium physics in heavy ion collisions. Our results also show that as long as the hot wind is not blowing precisely perpendicular to the plane of the baryon configuration that we analyze, the Nc different quarks are not all affected by the wind velocity to the same degree, with those quarks lying perpendicular to the wind direction screened most effectively.

background contribution method result interpretation main claim

What the classifier reports for each sentence. The number is the probability it gave the label.
#sentencerolethe authors' own workstates the main conclusionstrength
s0 The L-dependence of the static potential between Nc quarks arranged in a circle of radius L (a "baryon") immersed in the hot plasma of a gauge theory with Nc colors defines a screening length Ls. background 0.99 0.12 0.03 asserted 0.97
s1 We use the AdS/CFT correspondence to compute this screening length for the case of heavy quarks in the plasma of strongly coupled N=4 super Yang-Mills theory moving with velocity v relative to the baryon. method 0.60 0.94 0.05 asserted 0.97
s2 We find that in the v -> 1 limit, Ls \propto (1-v^2)^{1/4}/T, and find that corrections to this velocity dependence are small at lower velocities. result 1.00 0.97 0.75 asserted 1.00
s3 This result provides evidence for the robustness of the analogous behavior of the screening length defined by the static quark-antiquark pair, which has been computed previously and in QCD is relevant to quarkonium physics in heavy ion collisions. interpretation 1.00 0.32 0.14 hedged possibility 0.69
s4 Our results also show that as long as the hot wind is not blowing precisely perpendicular to the plane of the baryon configuration that we analyze, the Nc different quarks are not all affected by the wind velocity to the same degree, with those quarks lying perpendicular to the wind direction screened most effectively. result 1.00 0.94 0.15 asserted 1.00

What kind of paper the classifier reports this is: theoretical result 0.99 · evidence from proof or derivation 0.65.

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Every quoted sentence on this record is the authors'. Every label is from Pith's closed vocabulary, with the probability shown beside it. Every number in the measurements table is the authors', checked by code. Record as JSON

The paper
Original abstract

The L-dependence of the static potential between Nc quarks arranged in a circle of radius L (a "baryon") immersed in the hot plasma of a gauge theory with Nc colors defines a screening length Ls. We use the AdS/CFT correspondence to compute this screening length for the case of heavy quarks in the plasma of strongly coupled N=4 super Yang-Mills theory moving with velocity v relative to the baryon. We find that in the v -> 1 limit, Ls \propto (1-v^2)^{1/4}/T, and find that corrections to this velocity dependence are small at lower velocities. This result provides evidence for the robustness of the analogous behavior of the screening length defined by the static quark-antiquark pair, which has been computed previously and in QCD is relevant to quarkonium physics in heavy ion collisions. Our results also show that as long as the hot wind is not blowing precisely perpendicular to the plane of the baryon configuration that we analyze, the Nc different quarks are not all affected by the wind velocity to the same degree, with those quarks lying perpendicular to the wind direction screened most effectively.

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References
How the literature uses it

19 arXiv papers cite this in 46 sentences

Each citing sentence is taken from the citing paper's LaTeX source and typed by Pith's classifier. A label appears at probability 0.8 or more (0.95 for support), a contest at 0.7 or more; the quoted words are the citing authors'. How each label was checked · JSON

Papers whose main result relates to this one's

Found among the papers closest to this one by title and main claim. Pith's classifier compared each pair's main results and a second model family confirmed the relation; checked against two further families, shown conflicts agreed 118 times in 120 and shown same results 218 times in 239. The quoted sentence is the other paper's main claim.

States the same result 1 paper
  • Related results that we find include the observation that the screening length formula L_s T ~ (1-v^2)^{1/4} obtained previously for other color singlet configurations, is robust for circular baryons as well.

    Baryon Dissociation in a Strongly Coupled Plasma · 0.86

Papers citing it · 26 sentences without a confident label

Uses its method or tool 2 papers
Compares with it 3 papers
Cites it as support 1 paper
  • If we assume that the configuration experiences no drag[ This assumption is supported by the computations involving meson configurations [ref] as well as previously considered baryon configurations [ref] .

    Baryon Dissociation in a Strongly Coupled Plasma · Baryon Screening and the AdS Black Hole · 1.00

Cites it as background 9 papers

What it cites · 51 sentences without a confident label

Builds on 1 paper
  • For example, following a line of reasoning developed in Ref. [ref] for the meson sector, it can be shown that in a certain class of gauge theories whose gravity duals are asymptotically AdS, as $v→1$ the baryon screening length scales as $L_s ∝(1-v^2)^1/4/^1/4$, where $$ is the energy density of the plasma. $$ is proportional to $T^4$ for the specific theory that we have analyzed, at any $v$, in this Section.

    Screening length in plasma winds · Wind parallel to the baryon configuration · 0.95

Uses the method or tool of 4 papers
  • As in Refs. [ref] , we regularize the baryon energy by subtracting the energy of (in this case $N_c$) disjoint quarks in a hot plasma wind of velocity $v$, whose strings are dragging behind them in the $x_3$ direction according to the solution found in [ref] .

    An AdS/CFT Calculation of Screening in a Hot Wind · Wind perpendicular to the baryon configuration · 0.93

  • As in Refs. [ref] , we regularize the baryon energy by subtracting the energy of (in this case $N_c$) disjoint quarks in a hot plasma wind of velocity $v$, whose strings are dragging behind them in the $x_3$ direction according to the solution found in [ref] .

    Wilson loops in heavy ion collisions and their calculation in AdS/CFT · Wind perpendicular to the baryon configuration · 0.93

  • As in Refs. [ref] , we regularize the baryon energy by subtracting the energy of (in this case $N_c$) disjoint quarks in a hot plasma wind of velocity $v$, whose strings are dragging behind them in the $x_3$ direction according to the solution found in [ref] .

    Energy loss of a heavy quark moving through N=4 supersymmetric Yang-Mills plasma · Wind perpendicular to the baryon configuration · 0.93

Uses data or values from 4 papers
Compares with 2 papers
  • The only feature in our Fig. [ref] that does not have a direct, almost quantitative, analogue in Ref. [ref] is the very small difference between the curves for the two cases in which the wind direction is perpendicular to the line between the quark and the D5-brane, namely the case in which the wind is parallel to the plane of the baryon configuration and the quark is at $ϕ=π/2$ and the case in which the wind is perpendicular to the plane of the baryon configuration.

    Wilson loops in heavy ion collisions and their calculation in AdS/CFT · Wind parallel to the baryon configuration · 0.99

  • Their curved shapes are strikingly similar to the shapes of the projections of strings joining a static quark-antiquark in the meson configurations analyzed in Refs. [ref] , although they are not precisely the same.

    An AdS/CFT Calculation of Screening in a Hot Wind · Wind parallel to the baryon configuration · 1.00

Cites as background 5 papers
  • The simplest example of the AdS/CFT correspondence is provided by the duality between $N=4$ supersymmetric Yang-Mills (SYM) theory and classical gravity in $AdS_5×S_5$ [ref] . $N=4$ super Yang-Mills theory is a conformally invariant theory with two parameters: the rank of the gauge group $N_c$ and the 't Hooft coupling $λ= g_YM^2 N_c$.

    The Large N Limit of Superconformal Field Theories and Supergravity · Introduction and Summary · 1.00

  • The IR/UV relationship that characterizes the AdS/CFT correspondence [ref] tells us that smaller values of the fifth-dimension coordinate $r$ correspond to larger length scales $R^2/r$ in the (3+1)-dimensional field theory, where $R$ is the curvature of the AdS space.

    The Holographic Bound in Anti-de Sitter Space · Introduction and Summary · 0.82

  • Many have been considered in lattice investigations [ref] .

    Heavy quark free energies for three quark systems at finite temperature · Introduction and Summary · 0.89

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