000594048 001__ 594048 000594048 005__ 20250715170713.0 000594048 0247_ $$2doi$$a10.1103/PhysRevD.109.016010 000594048 0247_ $$2INSPIRETeX$$aFieg:2023kld 000594048 0247_ $$2inspire$$ainspire:2698221 000594048 0247_ $$2ISSN$$a2470-0010 000594048 0247_ $$2ISSN$$a2470-0037 000594048 0247_ $$2ISSN$$a2470-0029 000594048 0247_ $$2arXiv$$aarXiv:2309.08604 000594048 0247_ $$2datacite_doi$$a10.3204/PUBDB-2023-05602 000594048 0247_ $$2WOS$$aWOS:001174137800010 000594048 0247_ $$2openalex$$aopenalex:W4390727150 000594048 037__ $$aPUBDB-2023-05602 000594048 041__ $$aEnglish 000594048 082__ $$a530 000594048 088__ $$2DESY$$aDESY-23-133 000594048 088__ $$2arXiv$$aarXiv:2309.08604 000594048 1001_ $$0P:(DE-HGF)0$$aFieg, Max$$b0$$eCorresponding author 000594048 245__ $$aTuning pythia for forward physics experiments 000594048 260__ $$aRidge, NY$$bAmerican Physical Society$$c2023 000594048 3367_ $$2DRIVER$$aarticle 000594048 3367_ $$2DataCite$$aOutput Types/Journal article 000594048 3367_ $$0PUB:(DE-HGF)16$$2PUB:(DE-HGF)$$aJournal Article$$bjournal$$mjournal$$s1720009063_1845733 000594048 3367_ $$2BibTeX$$aARTICLE 000594048 3367_ $$2ORCID$$aJOURNAL_ARTICLE 000594048 3367_ $$00$$2EndNote$$aJournal Article 000594048 500__ $$aWe will first submit to arXiv, and later also to a journal. 000594048 520__ $$aEvent generators like pythia play an important role in physics studies at the Large Hadron Collider (LHC). While they make accurate predictions in the central region, i.e., at pseudorapidities η<5, a disagreement between pythia and measurements in the forward region η>7 has been observed. We introduce a dedicated forward physics tune for the pythia event generator to be used for forward physics studies at the LHC, which uses a more flexible modeling of beam remnant hadronization and is tuned to available particle spectra measured by LHCf. Furthermore, we provide an uncertainty estimate on the new tune in a data-driven way which can be used as a means of flux uncertainty for future forward physics studies. We demonstrate an application of our tune by showing the updated neutrino and dark photon spectra at the FASER experiment. 000594048 536__ $$0G:(DE-HGF)POF4-611$$a611 - Fundamental Particles and Forces (POF4-611)$$cPOF4-611$$fPOF IV$$x0 000594048 536__ $$0G:(GEPRIS)390833306$$aDFG project 390833306 - EXC 2121: Quantum Universe (390833306)$$c390833306$$x1 000594048 588__ $$aDataset connected to CrossRef, INSPIRE, Journals: bib-pubdb1.desy.de 000594048 650_7 $$2INSPIRE$$aPYTHIA 000594048 650_7 $$2INSPIRE$$aparticle: spectrum 000594048 650_7 $$2INSPIRE$$aphoton: spectrum 000594048 650_7 $$2INSPIRE$$aneutrino: spectrum 000594048 650_7 $$2INSPIRE$$aCERN LHC Coll 000594048 650_7 $$2INSPIRE$$aMonte Carlo 000594048 650_7 $$2INSPIRE$$aLHC-F 000594048 650_7 $$2INSPIRE$$aflux 000594048 650_7 $$2INSPIRE$$ahadronization 000594048 650_7 $$2INSPIRE$$arapidity 000594048 650_7 $$2INSPIRE$$acentral region 000594048 650_7 $$2INSPIRE$$aforward production 000594048 693__ $$0EXP:(DE-MLZ)NOSPEC-20140101$$5EXP:(DE-MLZ)NOSPEC-20140101$$eNo specific instrument$$x0 000594048 7001_ $$0P:(DE-H253)PIP1097110$$aKling, Felix$$b1 000594048 7001_ $$aSchulz, Holger$$b2 000594048 7001_ $$00000-0002-7630-8605$$aSjöstrand, Torbjörn$$b3 000594048 773__ $$0PERI:(DE-600)2844732-3$$a10.1103/PhysRevD.109.016010$$gVol. 109, no. 1, p. 016010$$n1$$p016010$$tPhysical review / D$$v109$$x2470-0010$$y2023 000594048 7870_ $$0PUBDB-2023-05595$$aFieg, Max et.al.$$d2023$$iIsParent$$rDESY-23-133$$tTuning Pythia for Forward Physics Experiments 000594048 8564_ $$uhttps://bib-pubdb1.desy.de/record/594048/files/HTML-Approval_of_scientific_publication.html 000594048 8564_ $$uhttps://bib-pubdb1.desy.de/record/594048/files/PDF-Approval_of_scientific_publication.pdf 000594048 8564_ $$uhttps://bib-pubdb1.desy.de/record/594048/files/PhysRevD.109.016010.pdf$$yRestricted$$zStatID:(DE-HGF)0599 000594048 8564_ $$uhttps://bib-pubdb1.desy.de/record/594048/files/TuningPythiaForFPF-2.pdf$$yOpenAccess$$zStatID:(DE-HGF)0510 000594048 8564_ $$uhttps://bib-pubdb1.desy.de/record/594048/files/PhysRevD.109.016010.pdf?subformat=pdfa$$xpdfa$$yRestricted$$zStatID:(DE-HGF)0599 000594048 8564_ $$uhttps://bib-pubdb1.desy.de/record/594048/files/TuningPythiaForFPF-2.pdf?subformat=pdfa$$xpdfa$$yOpenAccess$$zStatID:(DE-HGF)0510 000594048 909CO $$ooai:bib-pubdb1.desy.de:594048$$pdnbdelivery$$pdriver$$pVDB$$popen_access$$popenaire 000594048 9101_ $$0I:(DE-588b)2008985-5$$6P:(DE-H253)PIP1097110$$aDeutsches Elektronen-Synchrotron$$b1$$kDESY 000594048 9131_ $$0G:(DE-HGF)POF4-611$$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$$vFundamental Particles and Forces$$x0 000594048 9141_ $$y2023 000594048 915__ $$0StatID:(DE-HGF)0150$$2StatID$$aDBCoverage$$bWeb of Science Core Collection$$d2024-02-05 000594048 915__ $$0StatID:(DE-HGF)0160$$2StatID$$aDBCoverage$$bEssential Science Indicators$$d2024-02-05 000594048 915__ $$0StatID:(DE-HGF)1230$$2StatID$$aDBCoverage$$bCurrent Contents - Electronics and Telecommunications Collection$$d2024-02-05 000594048 915__ $$0LIC:(DE-HGF)CCBY4$$2HGFVOC$$aCreative Commons Attribution CC BY 4.0 000594048 915__ $$0StatID:(DE-HGF)0600$$2StatID$$aDBCoverage$$bEbsco Academic Search$$d2024-02-05 000594048 915__ $$0StatID:(DE-HGF)1150$$2StatID$$aDBCoverage$$bCurrent Contents - Physical, Chemical and Earth Sciences$$d2024-02-05 000594048 915__ $$0StatID:(DE-HGF)9905$$2StatID$$aIF >= 5$$bPHYS REV D : 2022$$d2024-02-05 000594048 915__ $$0StatID:(DE-HGF)0200$$2StatID$$aDBCoverage$$bSCOPUS$$d2024-02-05 000594048 915__ $$0StatID:(DE-HGF)0113$$2StatID$$aWoS$$bScience Citation Index Expanded$$d2024-02-05 000594048 915__ $$0StatID:(DE-HGF)0510$$2StatID$$aOpenAccess 000594048 915__ $$0StatID:(DE-HGF)0571$$2StatID$$aDBCoverage$$bSCOAP3 sponsored Journal$$d2024-02-05 000594048 915__ $$0StatID:(DE-HGF)0100$$2StatID$$aJCR$$bPHYS REV D : 2022$$d2024-02-05 000594048 915__ $$0StatID:(DE-HGF)0020$$2StatID$$aNo Peer Review$$bASC$$d2024-02-05 000594048 915__ $$0StatID:(DE-HGF)0300$$2StatID$$aDBCoverage$$bMedline$$d2024-02-05 000594048 915__ $$0StatID:(DE-HGF)0199$$2StatID$$aDBCoverage$$bClarivate Analytics Master Journal List$$d2024-02-05 000594048 915__ $$0StatID:(DE-HGF)0570$$2StatID$$aSCOAP3 000594048 9201_ $$0I:(DE-H253)T-20120731$$kT$$lTheorie-Gruppe$$x0 000594048 980__ $$ajournal 000594048 980__ $$aVDB 000594048 980__ $$aI:(DE-H253)T-20120731 000594048 980__ $$aUNRESTRICTED 000594048 9801_ $$aFullTexts