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dc.contributor.authorCampanario, F.-
dc.contributor.authorCzyż, Henryk-
dc.contributor.authorGluza, Janusz-
dc.contributor.authorGunia, Michał-
dc.contributor.authorRiemann, T.-
dc.contributor.authorRodrigo, G.-
dc.contributor.authorYundin, V.-
dc.date.accessioned2019-05-29T07:34:13Z-
dc.date.available2019-05-29T07:34:13Z-
dc.date.issued2014-
dc.identifier.citationJournal of High Energy Physics, 2014, iss. 2, art. no. 114pl_PL
dc.identifier.issn1029-8479-
dc.identifier.urihttp://hdl.handle.net/20.500.12128/9227-
dc.description.abstractKLOE and Babar have an observed discrepancy of 2% to 5% in the invariant pion pair production cross section. These measurements are based on approximate NLO μ+μ− cross section predictions of the Monte Carlo event generator PHOKHARA7.0. In this article, the complete NLO radiative corrections to μ+μ− production are calculated and implemented in the Monte Carlo event generator PHOKHARA9.0. Numerical reliability is guaranteed by two independent approaches to the real and the virtual corrections. The novel features include the contribution of pentagon diagrams in the virtual corrections, which form a gauge-invariant set when combined with their box diagram partners. They may contribute to certain distributions at the percent level. Also the real emission was complemented with two-photon final state emission contributions not included in the generator PHOKHARA7.0. We demonstrate that the numerical influence reaches, for realistic charge-averaged experimental setups, not more than 0.1% at KLOE and 0.3% at BaBar energies. As a result, we exclude the approximations in earlier versions of PHOKHARA as origin of the observed experimental discrepancy.pl_PL
dc.language.isoenpl_PL
dc.rightsUznanie autorstwa 3.0 Polska*
dc.rights.urihttp://creativecommons.org/licenses/by/3.0/pl/*
dc.subjectB-Physicspl_PL
dc.subjectStandard Modelpl_PL
dc.titleComplete QED NLO contributions to the reaction e(+)e(-) -> mu(+)mu(-)gamma and their implementation in the event generator PHOKHARApl_PL
dc.typeinfo:eu-repo/semantics/articlepl_PL
dc.relation.journalJournal of High Energy Physicspl_PL
dc.identifier.doi10.1007/JHEP02(2014)114-
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Uznanie Autorstwa 3.0 Polska Creative Commons Creative Commons