Näytä suppeat kuvailutiedot

dc.contributor.authorMäntysaari, Heikki
dc.contributor.authorZurita, P.
dc.date.accessioned2018-08-29T09:45:33Z
dc.date.available2018-08-29T09:45:33Z
dc.date.issued2018
dc.identifier.citationMäntysaari, H., & Zurita, P. (2018). In depth analysis of the combined HERA data in the dipole models with and without saturation. <i>Physical Review D</i>, <i>98</i>(3), Article 036002. <a href="https://doi.org/10.1103/PhysRevD.98.036002" target="_blank">https://doi.org/10.1103/PhysRevD.98.036002</a>
dc.identifier.otherCONVID_28225478
dc.identifier.otherTUTKAID_78604
dc.identifier.urihttps://jyx.jyu.fi/handle/123456789/59374
dc.description.abstractWe present an updated impact parameter dependent saturation model determined through a fit to the combined HERA I and I+II reduced cross section data. The same HERA data are used to fit the linearized version of the applied dipole amplitude, which makes it possible to estimate the magnitude of the saturation effects in various experiments. We find that both parametrizations provide comparable descriptions of the considered data when an effective confinement scale dynamics is incorporated with quark masses. Moreover, it is possible to consistently determine the light and charm quark masses. The role of potentially nonperturbatively large dipoles is examined in detail, with the result that, especially in the case of the structure function F2, their contribution is numerically significant. The potential to discriminate between the two models in future e+p and e+A experiments is also illustrated.fi
dc.format.mimetypeapplication/pdf
dc.language.isoeng
dc.publisherAmerican Physical Society
dc.relation.ispartofseriesPhysical Review D
dc.rightsCC BY 4.0
dc.subject.otherquantum chromodynamics
dc.subject.othersaturation
dc.titleIn depth analysis of the combined HERA data in the dipole models with and without saturation
dc.typearticle
dc.identifier.urnURN:NBN:fi:jyu-201808233918
dc.contributor.laitosFysiikan laitosfi
dc.contributor.laitosDepartment of Physicsen
dc.type.urihttp://purl.org/eprint/type/JournalArticle
dc.date.updated2018-08-23T09:15:10Z
dc.type.coarhttp://purl.org/coar/resource_type/c_2df8fbb1
dc.description.reviewstatuspeerReviewed
dc.relation.issn2470-0010
dc.relation.numberinseries3
dc.relation.volume98
dc.type.versionpublishedVersion
dc.rights.copyright© 2018 the Author(s)
dc.rights.accesslevelopenAccessfi
dc.relation.grantnumber681707
dc.relation.grantnumber681707
dc.relation.projectidinfo:eu-repo/grantAgreement/EC/H2020/681707/EU//CGCglasmaQGP
dc.subject.ysoprotonit
dc.subject.ysohiukkasfysiikka
dc.format.contentfulltext
jyx.subject.urihttp://www.yso.fi/onto/yso/p12428
jyx.subject.urihttp://www.yso.fi/onto/yso/p15576
dc.rights.urlhttps://creativecommons.org/licenses/by/4.0/
dc.relation.doi10.1103/PhysRevD.98.036002
dc.relation.funderEuroopan komissiofi
dc.relation.funderEuropean Commissionen
jyx.fundingprogramERC European Research Council, H2020fi
jyx.fundingprogramERC European Research Council, H2020en
jyx.fundinginformationH. M. was supported under DOE Contract No. DE-SC0012704 and European Research Council, Grant No. ERC-2015-CoG-681707, and wishes to thank the Nuclear Theory Group at BNL for hospitality during the preparation of this manuscript. P. Z. acknowledges the support by the U.S. Department of Energy under Contract No. DE-SC0012704.
dc.type.okmA1


Aineistoon kuuluvat tiedostot

Thumbnail

Aineisto kuuluu seuraaviin kokoelmiin

Näytä suppeat kuvailutiedot

CC BY 4.0
Ellei muuten mainita, aineiston lisenssi on CC BY 4.0