Extracting the speed of sound in quark-gluon plasma with ultrarelativistic lead-lead collisions at the LHC

CMS Collaboration, Emil Sørensen Bols, Jorgen D'Hondt, Soumya Dansana, Alexandre De Moor, Martin Delcourt, Hesham El Faham, Steven Lowette, Inna Makarenko, Denise Müller, Abanti Ranadhir Sahasransu, Stefaan Tavernier, Michael Tytgat, Gerrit Van Onsem, Senne Van Putte, David Vannerom, Nicolas Stylianou

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Ultrarelativistic nuclear collisions create a strongly interacting state of hot and dense quark-gluon matter that exhibits a remarkable collective flow behavior with minimal viscous dissipation. To gain deeper insights into its intrinsic nature and fundamental degrees of freedom, we determine the speed of sound in an extended volume of quark-gluon plasma using lead-lead (PbPb) collisions at a center-of-mass energy per nucleon pair of 5.02 TeV. The data were recorded by the CMS experiment at the CERN LHC and correspond to an integrated luminosity of 0.607 nb$^{-1}$. The measurement is performed by studying the multiplicity dependence of the average transverse momentum of charged particles emitted in head-on PbPb collisions. Our findings reveal that the speed of sound in this matter is nearly half the speed of light, with a squared value of 0.241 $\pm$ 0.002 (stat) $\pm$ 0.016 (syst) in natural units. The effective medium temperature, estimated using the mean transverse momentum, is 219 $\pm$ 8 (syst) MeV. The measured squared speed of sound at this temperature aligns precisely with predictions from lattice quantum chromodynamic (QCD) calculations. This result provides a stringent constraint on the equation of state of the created medium and direct evidence for a deconfined QCD phase being attained in relativistic nuclear collisions.
Originele taal-2English
Artikelnummer77801
Aantal pagina's21
TijdschriftReport on Progress
Volume87
Nummer van het tijdschrift7
DOI's
StatusPublished - 20 jun 2024

Bibliografische nota

Replaced to correct one number in the previous version. All the figures and tables, including additional supplementary figures, can be found at http://cms-results.web.cern.ch/cms-results/public-results/publications/HIN-23-003 (CMS Public Pages)

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