scholarly journals The phases of strongly interacting matter in heavy ion collisions

2005 ◽  
Author(s):  
Péter Lévai
2019 ◽  
Vol 204 ◽  
pp. 03009
Author(s):  
Arkadiy Taranenko

Relativistic heavy-ion collisions provide a unique opportunity to study the expansion dynamics and the transport properties of the produced strongly interacting matter. This article reviews the recent results of anisotropic flow measurements for collision energies from $$\sqrt {s{\rm{NN}}} = 200$$ to 2 GeV.


Proceedings ◽  
2019 ◽  
Vol 13 (1) ◽  
pp. 6 ◽  
Author(s):  
Francesco Collaboration

Deconfined strongly interacting QCD matter is produced in the laboratory at the highest energy densities in heavy-ion collisions at the LHC. A selection of recent results from ALICE is presented, spanning observables from the soft sector (bulk particle production and correlations), the hard probes (charmed hadrons and jets) and signatures of possible collective effects in pp and p–Pb collisions with high multiplicity. Finally, the perspectives after the detectors upgrades, taking place in the period 2019–2020, are presented.


2021 ◽  
Author(s):  
Olga Soloveva ◽  
Pierre Moreau ◽  
Elena Bratkovskaya

Abstract We review the transport properties of the strongly interacting quark-gluon plasma (QGP) created in heavy-ion collisions at ultrarelativistic energies, i.e. out-of equilibrium, and compare them to the equilibrium properties. The description of the strongly interacting (non-perturbative) QGP in equilibrium is based on the effective propagators and couplings from the Dynamical QuasiParticle Model (DQPM) that is matched to reproduce the equation-of-state of the partonic system above the deconfinement temperature $T_c$ from lattice QCD. We study the transport coefficients such as the ratio of shear viscosity and bulk viscosity over entropy density, diffusion coefficients, electric conductivity etc. versus temperature and baryon chemical potential. Based on a microscopic transport description of heavy-ion collisions we, furthermore, discuss which observables are sensitive to the QGP formation and its properties.


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