dc.contributor.author | Dumitru, Adrian | |
dc.contributor.author | Mäntysaari, Heikki | |
dc.contributor.author | Paatelainen, Risto | |
dc.date.accessioned | 2023-08-21T10:37:48Z | |
dc.date.available | 2023-08-21T10:37:48Z | |
dc.date.issued | 2023 | |
dc.identifier.citation | Dumitru, A., Mäntysaari, H., & Paatelainen, R. (2023). High-energy dipole scattering amplitude from evolution of low-energy proton light-cone wave functions. <i>Physical Review D</i>, <i>107</i>, Article 114024. <a href="https://doi.org/10.1103/PhysRevD.107.114024" target="_blank">https://doi.org/10.1103/PhysRevD.107.114024</a> | |
dc.identifier.other | CONVID_184059310 | |
dc.identifier.uri | https://jyx.jyu.fi/handle/123456789/88599 | |
dc.description.abstract | The forward scattering amplitude of a small dipole at high energies is given in the mean field approximation by the Balitsky-Kovchegov (BK) evolution equation. It requires an initial condition N(r;x0) describing the scattering of a dipole with size r off the target that is probed at momentum fraction x0. Rather than using ad hoc parametrizations tuned to high-energy data at x≪x0, here we attempt to construct an initial scattering amplitude that is consistent with low-energy, large-x properties of the proton. We start from a nonperturbative three quark light-cone model wave function from the literature. We add O(g) corrections due to the emission of a gluon, and O(g2) virtual corrections due to the exchange of a gluon, computed in light-cone perturbation theory with exact kinematics. We provide numerical data as well as analytic parametrizations of the resulting N(r;x0) for x0=0.01–0.05. Solving the BK equation in the leading logarithmic approximation towards lower x, we obtain a fair description of the charm cross section in deeply inelastic scattering measured at HERA by fitting one parameter, the coupling constant αs≃0.2. However, without the option to tune the initial amplitude at x0, the fit of the high precision data results in χ2/Ndof=2.3 at Ndof=38, providing clear statistical evidence for the need of systematic improvement, e.g., of the photon wave function, evolution equation, and initial condition. | en |
dc.format.mimetype | application/pdf | |
dc.language.iso | eng | |
dc.publisher | American Physical Society (APS) | |
dc.relation.ispartofseries | Physical Review D | |
dc.rights | CC BY 4.0 | |
dc.title | High-energy dipole scattering amplitude from evolution of low-energy proton light-cone wave functions | |
dc.type | research article | |
dc.identifier.urn | URN:NBN:fi:jyu-202308214697 | |
dc.contributor.laitos | Fysiikan laitos | fi |
dc.contributor.laitos | Department of Physics | en |
dc.type.uri | http://purl.org/eprint/type/JournalArticle | |
dc.type.coar | http://purl.org/coar/resource_type/c_2df8fbb1 | |
dc.description.reviewstatus | peerReviewed | |
dc.relation.issn | 2470-0010 | |
dc.relation.volume | 107 | |
dc.type.version | publishedVersion | |
dc.rights.copyright | © Funded by SCOAP3. Published by the American Physical Society | |
dc.rights.accesslevel | openAccess | fi |
dc.type.publication | article | |
dc.relation.grantnumber | 338263 | |
dc.relation.grantnumber | 824093 | |
dc.relation.grantnumber | 824093 | |
dc.relation.grantnumber | 835105 | |
dc.relation.grantnumber | 835105 | |
dc.relation.grantnumber | 346567 | |
dc.relation.projectid | info:eu-repo/grantAgreement/EC/H2020/824093/EU//STRONG-2020 | |
dc.relation.projectid | info:eu-repo/grantAgreement/EC/H2020/835105/EU//YoctoLHC | |
dc.subject.yso | hiukkasfysiikka | |
dc.subject.yso | ydinfysiikka | |
dc.format.content | fulltext | |
jyx.subject.uri | http://www.yso.fi/onto/yso/p15576 | |
jyx.subject.uri | http://www.yso.fi/onto/yso/p14759 | |
dc.rights.url | https://creativecommons.org/licenses/by/4.0/ | |
dc.relation.doi | 10.1103/PhysRevD.107.114024 | |
dc.relation.funder | Research Council of Finland | en |
dc.relation.funder | European Commission | en |
dc.relation.funder | European Commission | en |
dc.relation.funder | Research Council of Finland | en |
dc.relation.funder | Suomen Akatemia | fi |
dc.relation.funder | Euroopan komissio | fi |
dc.relation.funder | Euroopan komissio | fi |
dc.relation.funder | Suomen Akatemia | fi |
jyx.fundingprogram | Academy Research Fellow, AoF | en |
jyx.fundingprogram | RIA Research and Innovation Action, H2020 | en |
jyx.fundingprogram | ERC Advanced Grant | en |
jyx.fundingprogram | Research costs of Academy Research Fellow, AoF | en |
jyx.fundingprogram | Akatemiatutkija, SA | fi |
jyx.fundingprogram | RIA Research and Innovation Action, H2020 | fi |
jyx.fundingprogram | ERC Advanced Grant | fi |
jyx.fundingprogram | Akatemiatutkijan tutkimuskulut, SA | fi |
jyx.fundinginformation | This material is based upon work supported by the U.S. Department of Energy, Office of Science, Office of Nuclear Physics, within the framework of the Saturated Glue (SURGE) Topical Theory collaboration. A. D. acknowl edges support by the DOE Office of Nuclear Physics through Grant No. DE-SC0002307, and The City University of New York for PSC-CUNY Research Grant No. 65079-00 53. This work was supported by the Academy of Finland, the Centre of Excellence in Quark Matter and Projects No. 338263 and No. 346567 (H. M.), and Projects No. 347499 and No. 353772 (R.P). H. M. is also supported under the European Union’s Horizon 2020 research and innovation program by the European Research Council (ERC, Grant Agreement No. ERC-2018-ADG 835105 YoctoLHC) and by the STRONG-2020 project (Grant Agreement No. 824093). The content of this article does not reflect the official opinion of the European Union and responsibility for the information and views expressed therein lies entirely with the authors. Computing resources from CSC–IT Center for Science in Espoo, Finland, and from the Finnish Grid and Cloud Infrastructure (persistent identifier urn:nbn:fi:research-infras-2016072533) were used in this work. | |
dc.type.okm | A1 | |