Analogy of QCD hadronization and Hawking-Unruh radiation at NICA
dc.Affiliation | October University for modern sciences and Arts (MSA) | |
dc.contributor.author | Tawfik, Abdel Nasser | |
dc.date.accessioned | 2019-11-23T10:22:16Z | |
dc.date.available | 2019-11-23T10:22:16Z | |
dc.date.issued | 2016 | |
dc.description | Accession Number: WOS:000382168700011 | en_US |
dc.description.abstract | The proposed analogy of particle production from high-energy collisions and Hawking-Unruh radiation from black holes is extended to finite density (collisions) and finite electric charge (black holes). Assuming that the electric charge is directly proportional to the density (or the chemical potential), it becomes clear that for at least two freezeout conditions; constant s/T-3 and E/N, the proposed analogy works very well. Dependence of radiation (freezeout) temperature on finite electric charge leads to an excellent estimation for kaon-to-pion ratio, for instance, especially in the energy range covered by NICA. The precise and complete measurements for various light-flavored particle yields and ratios are essential in characterizing Hawing-Unruh radiation from charged black holes and the QCD hadronization at finite density, as wel | en_US |
dc.description.sponsorship | SPRINGER | en_US |
dc.identifier.citation | Cited References in Web of Science Core Collection: 34 | en_US |
dc.identifier.doi | https://doi.org/10.1140/epja/i2016-16254-3 | |
dc.identifier.issn | 1434-6001 | |
dc.identifier.other | https://doi.org/10.1140/epja/i2016-16254-3 | |
dc.identifier.uri | https://cutt.ly/VeVy80E | |
dc.language.iso | en | en_US |
dc.publisher | SPRINGER | en_US |
dc.relation.ispartofseries | EUROPEAN PHYSICAL JOURNAL A;Volume: 52 Issue: 8 Article Number: 254 | |
dc.relation.uri | https://cutt.ly/weVy8jE | |
dc.subject | University for CHEMICAL FREEZE-OUT | en_US |
dc.subject | BLACK-HOLES | en_US |
dc.subject | ENTROPY | en_US |
dc.subject | THERMODYNAMICS | en_US |
dc.subject | LATTICE | en_US |
dc.title | Analogy of QCD hadronization and Hawking-Unruh radiation at NICA | en_US |
dc.type | Article | en_US |
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