dc.contributor.author | ALICE Collaboration | |
dc.date.accessioned | 2017-08-23T11:49:43Z | |
dc.date.available | 2017-08-23T11:49:43Z | |
dc.date.issued | 2017 | |
dc.identifier.citation | ALICE Collaboration. (2017). Centrality dependence of the pseudorapidity density distribution for charged particles in Pb–Pb collisions at √sNN = 5.02 TeV. <i>Physics Letters B</i>, <i>772</i>, 567-577. <a href="https://doi.org/10.1016/j.physletb.2017.07.017" target="_blank">https://doi.org/10.1016/j.physletb.2017.07.017</a> | |
dc.identifier.other | CONVID_27128915 | |
dc.identifier.uri | https://jyx.jyu.fi/handle/123456789/55159 | |
dc.description.abstract | We present the charged-particle pseudorapidity density in Pb–Pb collisions at √sNN = 5.02 TeV in
centrality classes measured by ALICE. The measurement covers a wide pseudorapidity range from −3.5
to 5, which is sufficient for reliable estimates of the total number of charged particles produced in the
collisions. For the most central (0–5%) collisions we find 21 400 ± 1 300, while for the most peripheral
(80–90%) we find 230 ± 38. This corresponds to an increase of (27 ± 4)% over the results at √sNN =
2.76 TeV previously reported by ALICE. The energy dependence of the total number of charged particles
produced in heavy-ion collisions is found to obey a modified power-law like behaviour. The chargedparticle
pseudorapidity density of the most central collisions is compared to model calculations — none
of which fully describes the measured distribution. We also present an estimate of the rapidity density
of charged particles. The width of that distribution is found to exhibit a remarkable proportionality to
the beam rapidity, independent of the collision energy from the top SPS to LHC energies. | |
dc.language.iso | eng | |
dc.publisher | Elsevier BV | |
dc.relation.ispartofseries | Physics Letters B | |
dc.subject.other | Pb–Pb collisions | |
dc.title | Centrality dependence of the pseudorapidity density distribution for charged particles in Pb–Pb collisions at √sNN = 5.02 TeV | |
dc.type | research article | |
dc.identifier.urn | URN:NBN:fi:jyu-201708163499 | |
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 | 2017-08-16T09:15:07Z | |
dc.type.coar | http://purl.org/coar/resource_type/c_2df8fbb1 | |
dc.description.reviewstatus | peerReviewed | |
dc.format.pagerange | 567-577 | |
dc.relation.issn | 0370-2693 | |
dc.relation.numberinseries | 0 | |
dc.relation.volume | 772 | |
dc.type.version | publishedVersion | |
dc.rights.copyright | © 2017 The Author(s). Published by Elsevier B.V. This is an open access article under the CC BY license. Funded by SCOAP3. | |
dc.rights.accesslevel | openAccess | fi |
dc.type.publication | article | |
dc.subject.yso | hiukkasfysiikka | |
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.2017.07.017 | |
dc.type.okm | A1 | |