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Status of Chemical Freeze-Out
High Energy Physics - Phenomenology · Submitted 14 Jul 2006
abstract compiled · 2026-09-23 · no language-model review
The authors' main claim The status of the energy dependence of the chemical freeze-out temperature and chemical potential obtained in heavy ion collisions is presented.
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The paper's own sentences, arranged. 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.
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The abstract, sentence by sentence
The status of the energy dependence of the chemical freeze-out temperature and chemical potential obtained in heavy ion collisions is presented. Recent proposals for chemical freeze-out conditions are compared.
background contribution method result interpretation main claim
| # | sentence | role | the authors' own work | states the main conclusion | strength |
|---|---|---|---|---|---|
| s0 | The status of the energy dependence of the chemical freeze-out temperature and chemical potential obtained in heavy ion collisions is presented. | contribution 0.83 | 0.36 | 0.13 | unclear 0.65 |
| s1 | Recent proposals for chemical freeze-out conditions are compared. | contribution 0.83 | 0.29 | 0.06 | unclear 0.59 |
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The paper
Original abstract
The status of the energy dependence of the chemical freeze-out temperature and chemical potential obtained in heavy ion collisions is presented. Recent proposals for chemical freeze-out conditions are compared.
Human review
References
How the literature uses it
14 arXiv papers cite this in 24 sentences
Papers citing it · 15 sentences without a confident label
Uses its data or values 3 papers
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taken from [ref] and we have parametrized the volume at chemical freeze-out (based on the data summarized in [ref] ) as
Determining the Duration of the Hadronic Stage at RHIC-BES Energies via Resonance Suppression Using a Full Set of Rate Equations · Framework · 0.99
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In absolute chemical equilibrium at highest heavy ion reaction energy one obtains chemical freeze-out temperature $T ∼160-170$ MeV, which goes down to $∼50$ MeV at the lowest reaction energies [ref] .
Resonances and fluctuations in the statistical model · Introduction · 0.88
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In Fig.[ref], chemical freeze-out curve [ref] , [ref] , obtained in statistical model analysis of particle ratios are shown (the red line).
A short course on Relativistic Heavy Ion Collisions · QCD phase diagram at finite baryon density · 0.92
Compares with it 2 papers
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Now, for $N_t=4$ already, the estimated curvature of the pseudo-critical line $T_c(m_0^c,μ)$ was about 3 times less than that of the experimental freeze-out curve [ref] .
A QCD chiral critical point at small chemical potential: is it there or not? · Towards the continuum limit · 0.95
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For comparison, in Fig.[ref], chemical freeze-out curve [ref] , [ref] , obtained in statistical model analysis of particle ratios are shown (the red line).
$J/\psi$ suppression and QCD phase diagram · introduction · 0.90
Cites it as support 1 paper
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That such a model can in fact describe quantitatively the yield of most particles, including multi-strange ones, has in fact been indicated by fits to average particle abundances at AGS,SPS and RHIC energies [ref] .
Phenomenology of Strangeness enhancement in heavy ion collisions · Statistical hadronization phenomenology of strangeness enhancement · 0.97
Cites it as background 2 papers
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Within the framework of the statistical hadronization model (SHM) it can be shown that, under the assumption of a rapid chemical freeze-out of a thermalized medium, particle abundances are described by statistical weights with only a small set of parameters: the chemical freeze-out temperature $$, the baryo-chemical potential $$, and the fireball volume $V$ [ref] .
Influence of modified light-flavor hadron spectra on particle yields in the statistical hadronization model · Introduction · 0.90
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We refer to [ref] for a review of the statistical model.
Statistical hadronization phenomenology in $K/\pi$ fluctuations at ultra-relativistic energies · Introduction · 1.00
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