dc.contributor.author | ALICE Collaboration | |
dc.date.accessioned | 2019-01-07T09:09:31Z | |
dc.date.available | 2019-01-07T09:09:31Z | |
dc.date.issued | 2019 | |
dc.identifier.citation | ALICE Collaboration. (2019). Transverse momentum spectra and nuclear modification factors of charged particles in Xe–Xe collisions at √sNN = 5.44 TeV. <i>Physics Letters B</i>, <i>788</i>, 166-179. <a href="https://doi.org/10.1016/j.physletb.2018.10.052" target="_blank">https://doi.org/10.1016/j.physletb.2018.10.052</a> | |
dc.identifier.other | CONVID_28828299 | |
dc.identifier.other | TUTKAID_80139 | |
dc.identifier.uri | https://jyx.jyu.fi/handle/123456789/60928 | |
dc.description.abstract | Transverse momentum (pT) spectra of charged particles at mid-pseudorapidity in Xe–Xe collisions at
√sNN = 5.44 TeV measured with the ALICE apparatus at the Large Hadron Collider are reported. The
kinematic range 0.15 < pT < 50 GeV/c and |η| < 0.8 is covered. Results are presented in nine classes
of collision centrality in the 0–80% range. For comparison, a pp reference at the collision energy of
√s = 5.44 TeV is obtained by interpolating between existing pp measurements at √s = 5.02 and 7 TeV.
The nuclear modification factors in central Xe–Xe collisions and Pb–Pb collisions at a similar center-ofmass energy of √sNN = 5.02 TeV, and in addition at 2.76 TeV, at analogous ranges of charged particle
multiplicity density dNch/dη show a remarkable similarity at pT > 10 GeV/c. The centrality dependence
of the ratio of the average transverse momentum (pT) in Xe–Xe collisions over Pb–Pb collision at
√s = 5.02 TeV is compared to hydrodynamical model calculations. | fi |
dc.format.mimetype | application/pdf | |
dc.language.iso | eng | |
dc.publisher | Elsevier B.V. | |
dc.relation.ispartofseries | Physics Letters B | |
dc.rights | CC BY 4.0 | |
dc.subject.other | Xe–Xe collisions | |
dc.subject.other | transverse momentum spectra | |
dc.title | Transverse momentum spectra and nuclear modification factors of charged particles in Xe–Xe collisions at √sNN = 5.44 TeV | |
dc.type | article | |
dc.identifier.urn | URN:NBN:fi:jyu-201901031026 | |
dc.contributor.laitos | Fysiikan laitos | fi |
dc.contributor.laitos | Department of Physics | en |
dc.type.uri | http://purl.org/eprint/type/JournalArticle | |
dc.date.updated | 2019-01-03T10:15:18Z | |
dc.type.coar | http://purl.org/coar/resource_type/c_2df8fbb1 | |
dc.description.reviewstatus | peerReviewed | |
dc.format.pagerange | 166-179 | |
dc.relation.issn | 0370-2693 | |
dc.relation.numberinseries | 0 | |
dc.relation.volume | 788 | |
dc.type.version | publishedVersion | |
dc.rights.copyright | © 2018 The Author. | |
dc.rights.accesslevel | openAccess | fi |
dc.subject.yso | hiukkasfysiikka | |
dc.format.content | fulltext | |
jyx.subject.uri | http://www.yso.fi/onto/yso/p15576 | |
dc.rights.url | https://creativecommons.org/licenses/by/4.0/ | |
dc.relation.doi | 10.1016/j.physletb.2018.10.052 | |
dc.type.okm | A1 | |