dc.contributor.author | PHENIX Collaboration | |
dc.date.accessioned | 2018-09-17T09:36:49Z | |
dc.date.available | 2018-09-17T09:36:49Z | |
dc.date.issued | 2018 | |
dc.identifier.citation | PHENIX Collaboration. (2018). Measurement of emission-angle anisotropy via long-range angular correlations with high-pT hadrons in d+Au and p+p collisions at √sNN = 200 GeV. <i>Physical Review C</i>, <i>98</i>(1), Article 014912. <a href="https://doi.org/10.1103/PhysRevC.98.014912" target="_blank">https://doi.org/10.1103/PhysRevC.98.014912</a> | |
dc.identifier.other | CONVID_28212660 | |
dc.identifier.uri | https://jyx.jyu.fi/handle/123456789/59543 | |
dc.description.abstract | We present measurements of two-particle angular correlations between high-transverse-momentum (2 < pT <
11 GeV/c) π0 observed at midrapidity (|η| < 0.35) and particles produced either at forward (3.1 <η< 3.9)
or backward (−3.7 <η< −3.1) rapidity in d + Au and p + p collisions at √sNN = 200 GeV. The azimuthal
angle correlations for particle pairs with this large rapidity gap in the Au-going direction exhibit a characteristic
structure that persists up to pT ≈ 6 GeV/c and which strongly depends on collision centrality, which is a similar
characteristic to the hydrodynamical particle flow in A + A collisions. The structure is absent in the d-going
direction as well as in p + p collisions, in the transverse-momentum range studied. The results indicate that
the structure is shifted in the Au-going direction toward more central collisions, similar to the charged-particle
pseudorapidity distributions. | fi |
dc.format.mimetype | application/pdf | |
dc.language.iso | eng | |
dc.publisher | American Physical Society | |
dc.relation.ispartofseries | Physical Review C | |
dc.rights | CC BY 4.0 | |
dc.subject.other | heavy-ion collisions | |
dc.subject.other | p+p collisions | |
dc.subject.other | hadrons | |
dc.title | Measurement of emission-angle anisotropy via long-range angular correlations with high-pT hadrons in d+Au and p+p collisions at √sNN = 200 GeV | |
dc.type | research article | |
dc.identifier.urn | URN:NBN:fi:jyu-201808163850 | |
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 | 2018-08-16T12:15:17Z | |
dc.type.coar | http://purl.org/coar/resource_type/c_2df8fbb1 | |
dc.description.reviewstatus | peerReviewed | |
dc.relation.issn | 2469-9985 | |
dc.relation.numberinseries | 1 | |
dc.relation.volume | 98 | |
dc.type.version | publishedVersion | |
dc.rights.copyright | © 2018 American Physical Society. Funded
by SCOAP3. | |
dc.rights.accesslevel | openAccess | fi |
dc.type.publication | article | |
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 | 10.1103/PhysRevC.98.014912 | |
dc.type.okm | A1 | |