000364106 001__ 364106
000364106 005__ 20260226232649.0
000364106 0247_ $$2doi$$a10.1103/rb78-nmcs
000364106 0247_ $$2ISSN$$a2469-9985
000364106 0247_ $$2ISSN$$a1538-4497
000364106 0247_ $$2ISSN$$a0556-2813
000364106 0247_ $$2ISSN$$a1089-490X
000364106 0247_ $$2ISSN$$a2469-9993
000364106 0247_ $$2ISSN$$a2470-0002
000364106 0247_ $$2datacite_doi$$a10.15120/GSI-2026-00285
000364106 0247_ $$2WOS$$aWOS:001579307100002
000364106 037__ $$aGSI-2026-00285
000364106 041__ $$aEnglish
000364106 082__ $$a530
000364106 088__ $$2arXiv$$a2505.09348
000364106 1001_ $$00009-0004-0826-3726$$aBaker, J. D.$$b0$$eCorresponding author
000364106 245__ $$aPhotonuclear tomography in ultraperipheral heavy-ion collisions
000364106 260__ $$aWoodbury, NY$$bInst.$$c2025
000364106 3367_ $$2DRIVER$$aarticle
000364106 3367_ $$2DataCite$$aOutput Types/Journal article
000364106 3367_ $$0PUB:(DE-HGF)16$$2PUB:(DE-HGF)$$aJournal Article$$bjournal$$mjournal$$s1772117839_1117701
000364106 3367_ $$2BibTeX$$aARTICLE
000364106 3367_ $$2ORCID$$aJOURNAL_ARTICLE
000364106 3367_ $$00$$2EndNote$$aJournal Article
000364106 500__ $$aPublished by the American Physical Society under the terms of the Creative Commons Attribution 4.0 International license. Further distribution of this work must maintain attribution to the author(s) and the published article’s title, journal citation, and DOI.
000364106 520__ $$aWe present a theoretical investigation of photonuclear tomography as a novel technique for probing the internal structure of nuclei. In this approach, ultraperipheral heavy-ion collisions (UPCs) serve as a source of intense fluxes of virtual photons, which induce coherent production of vector mesons. By analyzing the probabilities and cross sections of these photon-induced processes, we propose a methodology for reconstructing the spatial distribution of nucleons within the nucleus. Our framework provides a systematic way to access information on the nuclear geometry probed in UPCs, offering new opportunities for studies of nuclear structure using particle production as a probe. Numerical calculations for selected examples illustrate the feasibility and potential of this method.
000364106 536__ $$0G:(DE-HGF)POF4-612$$a612 - Cosmic Matter in the Laboratory (POF4-612)$$cPOF4-612$$fPOF IV$$x0
000364106 536__ $$0G:(GEPRIS)390831469$$aDFG project G:(GEPRIS)390831469 - EXC 2118: Precision Physics, Fundamental Interactions and Structure of Matter (PRISMA+) (390831469)$$c390831469$$x1
000364106 536__ $$0G:(GEPRIS)491382106$$aDFG project G:(GEPRIS)491382106 - Open-Access-Publikationskosten / 2025-2027 / GSI Helmholtzzentrum für Schwerionenforschung (491382106)$$c491382106$$x2
000364106 588__ $$aDataset connected to CrossRef, Journals: repository.gsi.de
000364106 693__ $$0EXP:(DE-Ds200)no_experiment-20200803$$1EXP:(DE-Ds200)theory-20200803$$5EXP:(DE-Ds200)no_experiment-20200803$$atheory$$eno experiment theory work (theory)$$x0
000364106 7001_ $$00000-0002-4065-6237$$aBertulani, C. A.$$b1$$eCorresponding author
000364106 7001_ $$00000-0003-4943-9973$$aGonçalves, Victor P.$$b2$$eCorresponding author
000364106 773__ $$0PERI:(DE-600)2844098-5$$a10.1103/rb78-nmcs$$gVol. 112, no. 3, p. 034911$$n3$$p034911$$tPhysical review / C$$v112$$x2469-9985$$y2025
000364106 8564_ $$uhttps://repository.gsi.de/record/364106/files/rb78-nmcs.pdf$$yOpenAccess
000364106 8564_ $$uhttps://repository.gsi.de/record/364106/files/rb78-nmcs.pdf?subformat=pdfa$$xpdfa$$yOpenAccess
000364106 8767_ $$92025$$d2026-02-26$$eHybrid-OA$$jFlatrate$$zAPS und DFG
000364106 8767_ $$92025$$d2026-02-26$$eHybrid-OA$$jStorniert$$zDFG OAPK
000364106 8767_ $$92025$$d2026-02-26$$eHybrid-OA$$jZahlung erfolgt$$zDFG OAPK
000364106 909CO $$ooai:repository.gsi.de:364106$$popenaire$$popen_access$$pOpenAPC$$pdriver$$pVDB$$popenCost$$pdnbdelivery
000364106 9101_ $$0I:(DE-Ds200)20121206GSI$$60000-0002-4065-6237$$aGSI Helmholtzzentrum für Schwerionenforschung GmbH$$b1$$kGSI
000364106 9131_ $$0G:(DE-HGF)POF4-612$$1G:(DE-HGF)POF4-610$$2G:(DE-HGF)POF4-600$$3G:(DE-HGF)POF4$$4G:(DE-HGF)POF$$aDE-HGF$$bForschungsbereich Materie$$lMatter and the Universe$$vCosmic Matter in the Laboratory$$x0
000364106 9141_ $$y2025
000364106 915__ $$0StatID:(DE-HGF)0200$$2StatID$$aDBCoverage$$bSCOPUS$$d2025-01-06
000364106 915__ $$0StatID:(DE-HGF)0300$$2StatID$$aDBCoverage$$bMedline$$d2025-01-06
000364106 915__ $$0StatID:(DE-HGF)1230$$2StatID$$aDBCoverage$$bCurrent Contents - Electronics and Telecommunications Collection$$d2025-01-06
000364106 915__ $$0LIC:(DE-HGF)CCBY4$$2HGFVOC$$aCreative Commons Attribution CC BY 4.0
000364106 915__ $$0StatID:(DE-HGF)0600$$2StatID$$aDBCoverage$$bEbsco Academic Search$$d2025-01-06
000364106 915__ $$0StatID:(DE-HGF)1150$$2StatID$$aDBCoverage$$bCurrent Contents - Physical, Chemical and Earth Sciences$$d2025-01-06
000364106 915__ $$0StatID:(DE-HGF)0113$$2StatID$$aWoS$$bScience Citation Index Expanded$$d2025-01-06
000364106 915__ $$0StatID:(DE-HGF)0150$$2StatID$$aDBCoverage$$bWeb of Science Core Collection$$d2025-01-06
000364106 915__ $$0StatID:(DE-HGF)9900$$2StatID$$aIF < 5$$d2025-01-06
000364106 915__ $$0StatID:(DE-HGF)0510$$2StatID$$aOpenAccess
000364106 915__ $$0StatID:(DE-HGF)0030$$2StatID$$aPeer Review$$bASC$$d2025-01-06
000364106 915__ $$0StatID:(DE-HGF)0100$$2StatID$$aJCR$$bPHYS REV C : 2022$$d2025-01-06
000364106 915__ $$0StatID:(DE-HGF)0160$$2StatID$$aDBCoverage$$bEssential Science Indicators$$d2025-01-06
000364106 915__ $$0StatID:(DE-HGF)0199$$2StatID$$aDBCoverage$$bClarivate Analytics Master Journal List$$d2025-01-06
000364106 915pc $$0PC:(DE-HGF)0000$$2APC$$aAPC keys set
000364106 915pc $$0PC:(DE-HGF)0001$$2APC$$aLocal Funding
000364106 915pc $$0PC:(DE-HGF)0002$$2APC$$aDFG OA Publikationskosten
000364106 915pc $$0PC:(DE-HGF)0133$$2APC$$aTIB: American Physical Society 01.01.2025
000364106 920__ $$lno
000364106 9201_ $$0I:(DE-Ds200)EXM-20080818OR100$$kEXM$$lExtreMe Matter Institute, EMMI$$x0
000364106 9801_ $$aFullTexts
000364106 980__ $$ajournal
000364106 980__ $$aVDB
000364106 980__ $$aI:(DE-Ds200)EXM-20080818OR100
000364106 980__ $$aUNRESTRICTED
000364106 980__ $$aAPC