scholarly journals Fluctuations of conserved charges within a Hadron Resonance Gas approach: chemical freeze-out conditions from net-charge and net-proton fluctuations

2015 ◽  
Vol 97 ◽  
pp. 00019
Author(s):  
V. Mantovani Sarti ◽  
P. Alba ◽  
W. Alberico ◽  
R. Bellwied ◽  
M. Bluhm ◽  
...  
2015 ◽  
Vol 612 ◽  
pp. 012041 ◽  
Author(s):  
M Bluhm ◽  
P Alba ◽  
W Alberico ◽  
R Bellwied ◽  
V Mantovani Sarti ◽  
...  

2012 ◽  
Vol 880 ◽  
pp. 48-64 ◽  
Author(s):  
P. Braun-Munzinger ◽  
B. Friman ◽  
F. Karsch ◽  
K. Redlich ◽  
V. Skokov

2018 ◽  
Vol 171 ◽  
pp. 05002
Author(s):  
Claudia Ratti

The latest lattice QCD results on fluctuations of conserved charges at finite temperature and density are reviewed, and connected to the experimental moments of their net-multiplicity distributions, in order to describe the chemical freeze-out from first principles.


2015 ◽  
Vol 60 (3) ◽  
pp. 181-200 ◽  
Author(s):  
K.A. Bugaev ◽  
◽  
A.I. Ivanytskyi ◽  
D.R. Oliinychenko ◽  
E.G. Nikonov ◽  
...  

2011 ◽  
Vol 8 (8) ◽  
pp. 811-817 ◽  
Author(s):  
D. B. Blaschke ◽  
J. Berdermann ◽  
J. Cleymans ◽  
K. Redlich

Author(s):  
V. Vovchenko ◽  
M. I. Gorenstein ◽  
L. M. Satarov ◽  
H. Stöcker
Keyword(s):  

2020 ◽  
Vol 56 (10) ◽  
Author(s):  
Tom Reichert ◽  
Gabriele Inghirami ◽  
Marcus Bleicher

AbstractWe introduce a novel approach based on elastic and inelastic scattering rates to extract the hyper-surface of the chemical freeze-out from a hadronic transport model in the energy range from E$$_\mathrm {lab}=1.23$$ lab = 1.23  AGeV to $$\sqrt{s_\mathrm {NN}}=62.4$$ s NN = 62.4  GeV. For this study, the Ultra-relativistic Quantum Molecular Dynamics (UrQMD) model combined with a coarse-graining method is employed. The chemical freeze-out distribution is reconstructed from the pions through several decay and re-formation chains involving resonances and taking into account inelastic, pseudo-elastic and string excitation reactions. The extracted average temperature and baryon chemical potential are then compared to statistical model analysis. Finally we investigate various freeze-out criteria suggested in the literature. We confirm within this microscopic dynamical simulation, that the chemical freeze-out at all energies coincides with $$\langle E\rangle /\langle N\rangle \approx 1$$ ⟨ E ⟩ / ⟨ N ⟩ ≈ 1  GeV, while other criteria, like $$s/T^3=7$$ s / T 3 = 7 and $$n_\mathrm {B}+n_{\bar{\mathrm {B}}}\approx 0.12$$ n B + n B ¯ ≈ 0.12 fm$$^{-3}$$ - 3 are limited to higher collision energies.


Sign in / Sign up

Export Citation Format

Share Document