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dc.contributor.authorALICE Collaboration
dc.date.accessioned2018-11-15T20:11:54Z
dc.date.available2018-11-15T20:11:54Z
dc.date.issued2017-02-16
dc.identifier.citationCollaboration, A. L. I. C. E. (2017). φ-Meson production at forward rapidity in p–Pb collisions at√ sNN= 5. 02 TeV and in pp collisions at. Physics Letters B, 768, 203-217.en_US
dc.identifier.urihttp://hdl.handle.net/1808/27367
dc.description.abstractThe first study of φ-meson production in p–Pb collisions at forward and backward rapidity, at a nucleon–nucleon centre-of-mass energy √sNN=5.02TeV, has been performed with the ALICE apparatus at the LHC. The φ-mesons have been identified in the dimuon decay channel in the transverse momentum (pT) range 1 <pT<7GeV/c, both in the p-going (2.03 <y <3.53) and the Pb-going (−4.46 <y <−2.96) directions — where ystands for the rapidity in the nucleon–nucleon centre-of-mass — the integrated luminosity amounting to 5.01 ±0.19nb−1and 5.81 ±0.20nb−1, respectively, for the two data sam-ples. Differential cross sections as a function of transverse momentum and rapidity are presented. The forward–backward ratio for φ-meson production is measured for 2.96 <|y| <3.53, resulting in a ratio ∼0.5with no significant pTdependence within the uncertainties. The pTdependence of the φnuclear modification factor RpPbexhibits an enhancement up to a factor1.6 at pT=3–4GeV/cin the Pb-going direction. The pTdependence of the φ-meson cross section in pp collisions at √s=2.76TeV, which is used to determine a reference for the p–Pb results, is also presented here for 1 <pT<5GeV/cand 2.5 <y <4, for a 78 ±3nb−1integrated luminosity sample.en_US
dc.description.sponsorshipSCOAP3en_US
dc.publisherElsevieren_US
dc.rights© 2017 The Author(s). Published by Elsevier B.V. This is an open access article under the CC BY license.en_US
dc.rights.urihttps://creativecommons.org/licenses/by/4.0/en_US
dc.titleφ-Meson production at forward rapidity in p–Pb collisions at √sNN=5.02TeVand in pp collisions at √s=2.76TeVen_US
dc.typeArticleen_US
kusw.kudepartmentPhysics and Astronomyen_US
dc.identifier.doi10.1016/j.physletb.2017.01.074en_US
kusw.oaversionScholarly/refereed, publisher versionen_US
kusw.oapolicyThis item meets KU Open Access policy criteria.en_US
dc.rights.accessrightsopenAccessen_US


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© 2017 The Author(s). Published by Elsevier B.V. This is an open access article under the CC BY license.
Except where otherwise noted, this item's license is described as: © 2017 The Author(s). Published by Elsevier B.V. This is an open access article under the CC BY license.