dc.contributor.author | ALICE Collaboration | |
dc.date.accessioned | 2017-07-11T06:48:07Z | |
dc.date.available | 2017-07-11T06:48:07Z | |
dc.date.issued | 2017 | |
dc.identifier.citation | ALICE Collaboration. (2017). Production of muons from heavy-flavour hadron decays in p–Pb collisions at √sNN = 5.02 TeV. <i>Physics Letters B</i>, <i>770</i>, 459-472. <a href="https://doi.org/10.1016/j.physletb.2017.03.049" target="_blank">https://doi.org/10.1016/j.physletb.2017.03.049</a> | |
dc.identifier.other | CONVID_27115727 | |
dc.identifier.other | TUTKAID_74421 | |
dc.identifier.uri | https://jyx.jyu.fi/handle/123456789/54908 | |
dc.description.abstract | The production of muons from heavy-flavour hadron decays in p–Pb collisions at √sNN = 5.02 TeV
was studied for 2 < pT < 16 GeV/c with the ALICE detector at the CERN LHC. The measurement was
performed at forward (p-going direction) and backward (Pb-going direction) rapidity, in the ranges of
rapidity in the centre-of-mass system (cms) 2.03 < ycms < 3.53 and −4.46 < ycms < −2.96, respectively.
The production cross sections and nuclear modification factors are presented as a function of transverse
momentum (pT). At forward rapidity, the nuclear modification factor is compatible with unity while
at backward rapidity, in the interval 2.5 < pT < 3.5 GeV/c, it is above unity by more than 2σ. The
ratio of the forward-to-backward production cross sections is also measured in the overlapping interval
2.96 < |ycms| < 3.53 and is smaller than unity by 3.7σ in 2.5 < pT < 3.5 GeV/c. The data are described
by model calculations including cold nuclear matter effects. | |
dc.language.iso | eng | |
dc.publisher | Elsevier BV | |
dc.relation.ispartofseries | Physics Letters B | |
dc.subject.other | hadron decay | |
dc.subject.other | p–Pb collisions | |
dc.title | Production of muons from heavy-flavour hadron decays in p–Pb collisions at √sNN = 5.02 TeV | |
dc.type | article | |
dc.identifier.urn | URN:NBN:fi:jyu-201707103280 | |
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 | 2017-07-10T12:15:08Z | |
dc.type.coar | http://purl.org/coar/resource_type/c_2df8fbb1 | |
dc.description.reviewstatus | peerReviewed | |
dc.format.pagerange | 459-472 | |
dc.relation.issn | 0370-2693 | |
dc.relation.numberinseries | 0 | |
dc.relation.volume | 770 | |
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.subject.yso | hiukkasfysiikka | |
dc.subject.yso | elektronit | |
jyx.subject.uri | http://www.yso.fi/onto/yso/p15576 | |
jyx.subject.uri | http://www.yso.fi/onto/yso/p4030 | |
dc.rights.url | https://creativecommons.org/licenses/by/4.0/ | |
dc.relation.doi | 10.1016/j.physletb.2017.03.049 | |
dc.type.okm | A1 | |