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Joint Institute for Nuclear Research Relativistic ... - Index of - JINR

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ADIABATIC CHEMICAL FREEZE-OUT AND WIDE RESONANCE<br />

MODIFICATION IN A THERMAL MEDIA<br />

K.A. Bugaev 1† , D.R. Oliinychenko 2 , E.G. Nikonov 3 , A.S. Sorin 2 and G.M. Zinovjev 1<br />

(1) Bogolyubov <strong>Institute</strong> <strong>for</strong> Theoretical Physics, Metrologichna str. 14 B , Kiev 03680, Ukraine<br />

(2) Bogoliubov Laboratory <strong>of</strong> Theoretical Physics, <strong>JINR</strong>, Joliot-Curie str. 6, Dubna, Russia<br />

(3) Laboratory <strong>for</strong> In<strong>for</strong>mation Technologies, <strong>JINR</strong>, Joliot-Curie str. 6, 141980 Dubna, Russia<br />

† E-mail: Bugaev@th.physik.uni-frankfurt.de<br />

The hadron resonance gas model [1] is a reliable theoretical tool to extract in<strong>for</strong>mation<br />

about the chemical freeze-out (FO) stage <strong>of</strong> the relativistic heavy ion collisions. However,<br />

the question about the reliable chemical FO criterion has a long history [1, 2]. Very<br />

recently this question was thoroughly investigated again [2], using the most sophisticated<br />

version <strong>of</strong> the hadron resonance gas model. Similarly to [1] it was found that none <strong>of</strong><br />

the <strong>for</strong>merly suggested chemical FO criteria is robust, if the realistic particle table with<br />

the hadron masses up to 2.6 GeV is used. However, in [2] the criterion <strong>of</strong> the adiabatic<br />

chemical FO was suggested. In [2] it was also shown that despite an essential difference<br />

with the model <strong>of</strong> [1] the same conclusion on the constant entropy per particle at chemical<br />

FO is reproduced by the chemical FO parameters found in [1]. Thus, it turns out that<br />

the criterion <strong>of</strong> the constant entropy per particle at chemical FO is, indeed, the reliable<br />

one.<br />

Despite the long history <strong>of</strong> this question there was no a single try to understand what<br />

is the physical reason behind any <strong>of</strong> the chemical FO criterion. There<strong>for</strong>e we developed<br />

a simple model equation <strong>of</strong> state which not only well describes the chemical FO thermodynamic<br />

parameters and reproduces the constant value <strong>of</strong> the entropy per particle at<br />

the chemical FO, but which allows us to elucidate the real mass spectra <strong>of</strong> mesons and<br />

baryons that generate such a criterion. Our analysis demonstrates that the real mass<br />

spectrum <strong>of</strong> hadrons is very much different from the Hagedorn mass spectrum which is<br />

traditionally expected to emerge already <strong>for</strong> hadrons with masses above 1.2 GeV [3]. We<br />

argue that the real mass spectrum <strong>of</strong> hadrons is not an exponential, but a power-like<br />

and the reason <strong>for</strong> such a behavior is in the existence <strong>of</strong> many wide resonances. The<br />

main point is that that the presence <strong>of</strong> thermal media essentially modifies the resonance<br />

mass distribution in case <strong>of</strong> large width and leads to the resonance sharpening near the<br />

threshold. The related effect <strong>of</strong> wide resonance enhancement compared to their treatment<br />

as stable particles with the average resonance mass is also discussed. Both effects are<br />

demonstrated in Fig. 2. Based on these findings we suggest that the quark-gluon bags<br />

maybe observed at the NICA energies as the narrow resonances with mass between 2.5<br />

and 4 GeV which are absent in the tables <strong>of</strong> elementary particle properties.<br />

Contacting the non-relativistic Boltzmann distribution in resonance energy φ(m,T) ≃<br />

[ mT<br />

2π 2 ]3<br />

2<br />

exp [ − m T<br />

]<br />

with the cut Gaussian distribution Θ<br />

(<br />

m−M<br />

Th<br />

k<br />

) ]<br />

exp<br />

[− (m k−m) 2<br />

over<br />

the resonance mass m one can easily see that the maximum <strong>of</strong> the resulting mass distribution<br />

is located at m = ˜m k ≡ m k − σ2 k<br />

T<br />

<strong>for</strong> k-th resonance. In addition, the resonance<br />

degeneracy factor g k is changed to an effective value ˜g k = g k exp[<br />

σ 2<br />

k<br />

2T 2 ]. Here m k denotes<br />

the mean mass <strong>of</strong> the resonance k-th in a vacuum, while its Gaussian width in a vacuum is<br />

σ k (note that thetrue width <strong>of</strong> such a resonance is Γ k = Qσ k with Q ≡ 2 √ 2 ln2 ≈ 2.355).<br />

32<br />

2σ 2 k

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