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dc.contributor.authorTumasyan, A
dc.contributor.authorAdam, W
dc.contributor.authorAmbrogi, F
dc.contributor.authorBergauer, T
dc.contributor.authorDragicevic, M
dc.contributor.authorErö, J
dc.contributor.authorEscalante Del Valle, A
dc.contributor.authorFrühwirth, R
dc.contributor.authorJeitler, M
dc.contributor.authorKrammer, N
dc.contributor.authorLechner, L
dc.contributor.authorLiko, D
dc.contributor.authorMadlener, T
dc.contributor.authorMikulec, I
dc.contributor.authorPitters, FM
dc.contributor.authorRad, N
dc.contributor.authorSchieck, J
dc.contributor.authorSchöfbeck, R
dc.contributor.authorSpanring, M
dc.contributor.authorTempl, S
dc.contributor.authorWaltenberger, W
dc.contributor.authorWulz, CE
dc.contributor.authorZarucki, M
dc.contributor.authorDarwish, MR
dc.contributor.authorDe Wolf, EA
dc.contributor.authorDi Croce, D
dc.contributor.authorJanssen, T
dc.contributor.authorKello, T
dc.contributor.authorLelek, A
dc.contributor.authorPieters, M
dc.contributor.authorRejeb Sfar, H
dc.contributor.authorVan Haevermaet, H
dc.contributor.authorVan Mechelen, P
dc.contributor.authorVan Putte, S
dc.contributor.authorVan Remortel, N
dc.contributor.authorBlekman, F
dc.contributor.authorBols, ES
dc.contributor.authorChhibra, SS
dc.contributor.authorD’Hondt, J
dc.contributor.authorDe Clercq, J
dc.contributor.authorLontkovskyi, D
dc.contributor.authorLowette, S
dc.contributor.authorMarchesini, I
dc.contributor.authorMoortgat, S
dc.contributor.authorMorton, A
dc.contributor.authorPython, Q
dc.contributor.authorTavernier, S
dc.contributor.authorVan Doninck, W
dc.contributor.authorVan Mulders, P
dc.contributor.authorBeghin, D
dc.contributor.authorBilin, B
dc.contributor.authorClerbaux, B
dc.contributor.authorDe Lentdecker, G
dc.contributor.authorDorney, B
dc.contributor.authorFavart, L
dc.contributor.authorGrebenyuk, A
dc.contributor.authorKalsi, AK
dc.contributor.authorMakarenko, I
dc.contributor.authorMoureaux, L
dc.contributor.authorPétré, L
dc.contributor.authorPopov, A
dc.contributor.authorPostiau, N
dc.contributor.authorStarling, E
dc.contributor.authorThomas, L
dc.contributor.authorVander Velde, C
dc.contributor.authorVanlaer, P
dc.contributor.authorVannerom, D
dc.contributor.authorWezenbeek, L
dc.contributor.authorCornelis, T
dc.contributor.authorDobur, D
dc.contributor.authorGruchala, M
dc.contributor.authorKhvastunov, I
dc.contributor.authorNiedziela, M
dc.contributor.authorRoskas, C
dc.contributor.authorSkovpen, K
dc.contributor.authorTytgat, M
dc.contributor.authorVerbeke, W
dc.contributor.authorVermassen, B
dc.contributor.authorVit, M
dc.contributor.authorBruno, G
dc.contributor.authorBury, F
dc.contributor.authorCaputo, C
dc.contributor.authorDavid, P
dc.contributor.authorDelaere, C
dc.contributor.authorDelcourt, M
dc.contributor.authorDonertas, IS
dc.contributor.authorGiammanco, A
dc.contributor.authorLemaitre, V
dc.contributor.authorMondal, K
dc.contributor.authorPrisciandaro, J
dc.contributor.authorTaliercio, A
dc.contributor.authorTeklishyn, M
dc.contributor.authorVischia, P
dc.contributor.authorWuyckens, S
dc.contributor.authorZobec, J
dc.contributor.authorAlves, GA
dc.contributor.authorHensel, C
dc.contributor.authorMoraes, A
dc.contributor.authorAldá Júnior, WL
dc.contributor.authorBelchior Batista Das Chagas, E
dc.date.accessioned2024-05-14T15:12:02Z
dc.date.available2024-05-14T15:12:02Z
dc.date.issued2023-11-01
dc.identifier.issn2470-0010
dc.identifier.urihttps://qmro.qmul.ac.uk/xmlui/handle/123456789/96871
dc.description.abstractFor the first time at LHC energies, the forward rapidity gap spectra from proton-lead collisions for both proton and lead dissociation processes are presented. The analysis is performed over 10.4 units of pseudorapidity at a center-of-mass energy per nucleon pair of Formula Presented, almost 300 times higher than in previous measurements of diffractive production in proton-nucleus collisions. For lead dissociation processes, which correspond to the pomeron-lead event topology, the epos-lhc generator predictions are a factor of 2 below the data, but the model gives a reasonable description of the rapidity gap spectrum shape. For the pomeron-proton topology, the epos-lhc, qgsjet ii, and hijing predictions are all at least a factor of 5 lower than the data. The latter effect might be explained by a significant contribution of ultraperipheral photoproduction events mimicking the signature of diffractive processes. These data may be of significant help in understanding the high energy limit of quantum chromodynamics and for modeling cosmic ray air showers.en_US
dc.publisherAmerican Physical Societyen_US
dc.relation.ispartofPhysical Review D
dc.rightsPublished by the American Physical Society under the terms of the Creative Commons Attribution 4.0 International license. Further distribution of this work must maintain attribution to the author(s) and the published article’s title, journal citation, and DOI. Funded by SCOAP3.
dc.titleFirst measurement of the forward rapidity gap distribution in Formula Presented collisions at Formula Presenteden_US
dc.typeArticleen_US
dc.rights.holder© 2023 CERN, for the CMS Collaboration
dc.identifier.doi10.1103/PhysRevD.108.092004
pubs.issue9en_US
pubs.notesNot knownen_US
pubs.publication-statusPublisheden_US
pubs.volume108en_US
rioxxterms.funderDefault funderen_US
rioxxterms.identifier.projectDefault projecten_US


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