Olaf Massen, Govert Nijs, Mike Sas, Wilke van der Schee, Raimond Snellings
{"title":"热光子和二轻子产生的 QGP 有效温度","authors":"Olaf Massen, Govert Nijs, Mike Sas, Wilke van der Schee, Raimond Snellings","doi":"10.1140/epjc/s10052-025-14072-6","DOIUrl":null,"url":null,"abstract":"<div><p>Thermal electromagnetic radiation is emitted by the quark-gluon plasma (QGP) throughout its space-time evolution, with production rates that depend characteristically on the temperature. We study this temperature using thermal photons and dileptons using the <i>Trajectum</i> heavy ion code, which is constrained by Bayesian analysis. In addition we present the elliptic flow of both the thermal photons and thermal dileptons including systematic uncertainties corresponding to the model parameter uncertainty. We give a comprehensive overview of the resulting effective temperatures <span>\\(T_{\\textrm{eff}},\\)</span> obtained from thermal photon transverse momentum and thermal dilepton invariant mass distributions, as well as the dependence of <span>\\(T_{\\textrm{eff}}\\)</span> on various selection criteria of these probes. We conclude that the <span>\\(T_{\\textrm{eff}}\\)</span> obtained from thermal photons is mostly insensitive to the temperature of the QGP with a value of <span>\\(T_{\\textrm{eff}} \\sim 250\\)</span>–300 MeV depending on their transverse momentum, almost independent of collision centrality. Thermal dileptons are much better probes of the QGP temperature as they do not suffer from a blue shift as their invariant mass is used, allowing for a more precise constraint of the QGP temperature during different stages of the evolution of the system. By applying selection criteria on the dilepton transverse momentum and the invariant mass we are able to extract fluid temperatures on average times ranging from late emission <span>\\((\\langle \\tau \\rangle = 5.6~\\text {fm}/c)\\)</span> to very early emissions <span>\\((\\langle \\tau \\rangle < 1.0~\\text {fm}/c).\\)</span> Furthermore, we show how these selection criteria can be used to map the elliptic flow of the system all throughout its evolution.\n</p></div>","PeriodicalId":788,"journal":{"name":"The European Physical Journal C","volume":"85 4","pages":""},"PeriodicalIF":4.2000,"publicationDate":"2025-04-04","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"https://link.springer.com/content/pdf/10.1140/epjc/s10052-025-14072-6.pdf","citationCount":"0","resultStr":"{\"title\":\"Effective temperatures of the QGP from thermal photon and dilepton production\",\"authors\":\"Olaf Massen, Govert Nijs, Mike Sas, Wilke van der Schee, Raimond Snellings\",\"doi\":\"10.1140/epjc/s10052-025-14072-6\",\"DOIUrl\":null,\"url\":null,\"abstract\":\"<div><p>Thermal electromagnetic radiation is emitted by the quark-gluon plasma (QGP) throughout its space-time evolution, with production rates that depend characteristically on the temperature. We study this temperature using thermal photons and dileptons using the <i>Trajectum</i> heavy ion code, which is constrained by Bayesian analysis. In addition we present the elliptic flow of both the thermal photons and thermal dileptons including systematic uncertainties corresponding to the model parameter uncertainty. We give a comprehensive overview of the resulting effective temperatures <span>\\\\(T_{\\\\textrm{eff}},\\\\)</span> obtained from thermal photon transverse momentum and thermal dilepton invariant mass distributions, as well as the dependence of <span>\\\\(T_{\\\\textrm{eff}}\\\\)</span> on various selection criteria of these probes. We conclude that the <span>\\\\(T_{\\\\textrm{eff}}\\\\)</span> obtained from thermal photons is mostly insensitive to the temperature of the QGP with a value of <span>\\\\(T_{\\\\textrm{eff}} \\\\sim 250\\\\)</span>–300 MeV depending on their transverse momentum, almost independent of collision centrality. Thermal dileptons are much better probes of the QGP temperature as they do not suffer from a blue shift as their invariant mass is used, allowing for a more precise constraint of the QGP temperature during different stages of the evolution of the system. By applying selection criteria on the dilepton transverse momentum and the invariant mass we are able to extract fluid temperatures on average times ranging from late emission <span>\\\\((\\\\langle \\\\tau \\\\rangle = 5.6~\\\\text {fm}/c)\\\\)</span> to very early emissions <span>\\\\((\\\\langle \\\\tau \\\\rangle < 1.0~\\\\text {fm}/c).\\\\)</span> Furthermore, we show how these selection criteria can be used to map the elliptic flow of the system all throughout its evolution.\\n</p></div>\",\"PeriodicalId\":788,\"journal\":{\"name\":\"The European Physical Journal C\",\"volume\":\"85 4\",\"pages\":\"\"},\"PeriodicalIF\":4.2000,\"publicationDate\":\"2025-04-04\",\"publicationTypes\":\"Journal Article\",\"fieldsOfStudy\":null,\"isOpenAccess\":false,\"openAccessPdf\":\"https://link.springer.com/content/pdf/10.1140/epjc/s10052-025-14072-6.pdf\",\"citationCount\":\"0\",\"resultStr\":null,\"platform\":\"Semanticscholar\",\"paperid\":null,\"PeriodicalName\":\"The European Physical Journal C\",\"FirstCategoryId\":\"4\",\"ListUrlMain\":\"https://link.springer.com/article/10.1140/epjc/s10052-025-14072-6\",\"RegionNum\":2,\"RegionCategory\":\"物理与天体物理\",\"ArticlePicture\":[],\"TitleCN\":null,\"AbstractTextCN\":null,\"PMCID\":null,\"EPubDate\":\"\",\"PubModel\":\"\",\"JCR\":\"Q2\",\"JCRName\":\"PHYSICS, PARTICLES & FIELDS\",\"Score\":null,\"Total\":0}","platform":"Semanticscholar","paperid":null,"PeriodicalName":"The European Physical Journal C","FirstCategoryId":"4","ListUrlMain":"https://link.springer.com/article/10.1140/epjc/s10052-025-14072-6","RegionNum":2,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"Q2","JCRName":"PHYSICS, PARTICLES & FIELDS","Score":null,"Total":0}
Effective temperatures of the QGP from thermal photon and dilepton production
Thermal electromagnetic radiation is emitted by the quark-gluon plasma (QGP) throughout its space-time evolution, with production rates that depend characteristically on the temperature. We study this temperature using thermal photons and dileptons using the Trajectum heavy ion code, which is constrained by Bayesian analysis. In addition we present the elliptic flow of both the thermal photons and thermal dileptons including systematic uncertainties corresponding to the model parameter uncertainty. We give a comprehensive overview of the resulting effective temperatures \(T_{\textrm{eff}},\) obtained from thermal photon transverse momentum and thermal dilepton invariant mass distributions, as well as the dependence of \(T_{\textrm{eff}}\) on various selection criteria of these probes. We conclude that the \(T_{\textrm{eff}}\) obtained from thermal photons is mostly insensitive to the temperature of the QGP with a value of \(T_{\textrm{eff}} \sim 250\)–300 MeV depending on their transverse momentum, almost independent of collision centrality. Thermal dileptons are much better probes of the QGP temperature as they do not suffer from a blue shift as their invariant mass is used, allowing for a more precise constraint of the QGP temperature during different stages of the evolution of the system. By applying selection criteria on the dilepton transverse momentum and the invariant mass we are able to extract fluid temperatures on average times ranging from late emission \((\langle \tau \rangle = 5.6~\text {fm}/c)\) to very early emissions \((\langle \tau \rangle < 1.0~\text {fm}/c).\) Furthermore, we show how these selection criteria can be used to map the elliptic flow of the system all throughout its evolution.
期刊介绍:
Experimental Physics I: Accelerator Based High-Energy Physics
Hadron and lepton collider physics
Lepton-nucleon scattering
High-energy nuclear reactions
Standard model precision tests
Search for new physics beyond the standard model
Heavy flavour physics
Neutrino properties
Particle detector developments
Computational methods and analysis tools
Experimental Physics II: Astroparticle Physics
Dark matter searches
High-energy cosmic rays
Double beta decay
Long baseline neutrino experiments
Neutrino astronomy
Axions and other weakly interacting light particles
Gravitational waves and observational cosmology
Particle detector developments
Computational methods and analysis tools
Theoretical Physics I: Phenomenology of the Standard Model and Beyond
Electroweak interactions
Quantum chromo dynamics
Heavy quark physics and quark flavour mixing
Neutrino physics
Phenomenology of astro- and cosmoparticle physics
Meson spectroscopy and non-perturbative QCD
Low-energy effective field theories
Lattice field theory
High temperature QCD and heavy ion physics
Phenomenology of supersymmetric extensions of the SM
Phenomenology of non-supersymmetric extensions of the SM
Model building and alternative models of electroweak symmetry breaking
Flavour physics beyond the SM
Computational algorithms and tools...etc.