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dc.date.accessioned2019-05-28T12:15:28Z
dc.date.available2019-05-28T12:15:28Z
dc.date.created2019-01-08T17:14:25Z
dc.date.issued2018
dc.identifier.citationBravina, Larissa Bleibel, J. Zabrodin, Evgeny . On the origin of forward?backward multiplicity correlations in pp collisions at ultrarelativistic energies. Physics Letters B. 2018, 787, 146-152
dc.identifier.urihttp://hdl.handle.net/10852/68171
dc.description.abstractWe study multiplicity correlations of hadrons in forward and backward hemispheres in pp inelastic interactions at energies 200 GeV ≤ √s ≤ 13 TeV within the microscopic quark–gluon string model. The model correctly describes (i) the almost linear dependence of average multiplicity in one hemisphere on the particle multiplicity in other hemisphere in the centre-of-mass frame; (ii) the increase of the slope parameter bcorr with rising collision energy; (iii) the quick falloff of the correlation strength with increase of the midrapidity gap; (iv) saturation of the forward–backward correlations at very high multiplicities. Investigation of the sub-processes on partonic level reveals that these features can be attributed to shortrange partonic correlations within a single string and superposition of several sub-processes containing different numbers of soft and hard Pomerons with different mean multiplicities. If the number of Pomerons in the event is fixed, no forward–backward correlations are observed. Predictions are made for the top LHC energy √s = 13 TeV.
dc.languageEN
dc.publisherNorth-Holland
dc.rightsAttribution 4.0 International
dc.rights.urihttps://creativecommons.org/licenses/by/4.0/
dc.titleOn the origin of forward?backward multiplicity correlations in pp collisions at ultrarelativistic energies
dc.typeJournal article
dc.creator.authorBravina, Larissa
dc.creator.authorBleibel, J.
dc.creator.authorZabrodin, Evgeny
cristin.unitcode185,15,4,60
cristin.unitnameHøyenergifysikk
cristin.ispublishedtrue
cristin.fulltextoriginal
cristin.qualitycode1
dc.identifier.cristin1652777
dc.identifier.bibliographiccitationinfo:ofi/fmt:kev:mtx:ctx&ctx_ver=Z39.88-2004&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.jtitle=Physics Letters B&rft.volume=787&rft.spage=146&rft.date=2018
dc.identifier.jtitlePhysics Letters B
dc.identifier.volume787
dc.identifier.startpage146
dc.identifier.endpage152
dc.identifier.doihttp://dx.doi.org/10.1016/j.physletb.2018.10.053
dc.identifier.urnURN:NBN:no-71324
dc.type.documentTidsskriftartikkel
dc.type.peerreviewedPeer reviewed
dc.source.issn0370-2693
dc.identifier.fulltextFulltext https://www.duo.uio.no/bitstream/handle/10852/68171/2/1-s2.0-S0370269318308244-main.pdf
dc.type.versionPublishedVersion


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