002708678 001__ 2708678
002708678 005__ 20250606092033.0
002708678 0248_ $$aoai:cds.cern.ch:2708678$$pcerncds:FULLTEXT$$pcerncds:CERN:FULLTEXT$$pcerncds:CERN
002708678 0247_ $$2DOI$$9arXiv$$a10.1103/PhysRevLett.126.071801$$qpublication
002708678 0247_ $$2DOI$$9APS$$a10.1103/PhysRevLett.133.239902$$qerratum
002708678 037__ $$9arXiv$$aarXiv:2002.00861$$chep-ex
002708678 035__ $$9arXiv$$aoai:arXiv.org:2002.00861
002708678 035__ $$9Inspire$$aoai:inspirehep.net:1778419$$d2025-06-05T07:17:09Z$$h2025-06-06T02:09:54Z$$mmarcxml$$ttrue$$uhttps://inspirehep.net/api/oai2d
002708678 035__ $$9Inspire$$a1778419
002708678 041__ $$aeng
002708678 100__ $$aAcharya, B.$$uKing's Coll. London$$uICTP, Trieste$$vTheoretical Particle Physics & Cosmology Group, Physics Dept., King's College London, UK$$vInternational Centre for Theoretical Physics, Trieste, Italy
002708678 245__ $$9arXiv$$aFirst search for dyons with the full MoEDAL trapping detector in 13 TeV pp collisions
002708678 246__ $$9APS$$aErratum: First Search for Dyons with the Full MoEDAL Trapping Detector in 13 TeV <math display="inline"><mi>p</mi><mi>p</mi></math> Collisions [Phys. Rev. Lett. 126, 071801 (2021)]
002708678 269__ $$c2020-01-30
002708678 260__ $$c2021-02-20
002708678 260__ $$c2024-12-04
002708678 300__ $$a7 p
002708678 500__ $$9arXiv$$aarXiv admin note: text overlap with arXiv:1903.08491
002708678 520__ $$9APS$$aThe MoEDAL trapping detector consists of approximately 800 kg of aluminum volumes. It was exposed during run 2 of the LHC program to 6.46 fb-1 of 13 TeV proton-proton collisions at the LHCb interaction point. Evidence for dyons (particles with electric and magnetic charge) captured in the trapping detector was sought by passing the aluminum volumes comprising the detector through a superconducting quantum interference device (SQUID) magnetometer. The presence of a trapped dyon would be signaled by a persistent current induced in the SQUID magnetometer. On the basis of a Drell-Yan production model, we exclude dyons with a magnetic charge ranging up to five Dirac charges (5gD) and an electric charge up to 200 times the fundamental electric charge for mass limits in the range 870–3120 GeV and also monopoles with magnetic charge up to and including 5gD with mass limits in the range 870–2040 GeV.
002708678 520__ $$9arXiv$$aThe MoEDAL trapping detector, consists of approximately 800 kg of aluminium volumes. It was exposed during Run-2 of the LHC program to 6.46 fb^-1 of 13 TeV proton-proton collisions at the LHCb interaction point. Evidence for dyons (particles with electric and magnetic charge) captured in the trapping detector was sought by passing the aluminium volumes comprising the detector through a SQUID magnetometer. The presence of a trapped dyon would be signalled by a persistent current induced in the SQUID magnetometer. On the basis of a Drell-Yan production model, we exclude dyons with a magnetic charge ranging up to 5 Dirac charges, and an electric charge up to 200 times the fundamental electric charge for mass limits in the range 790 - 3130 GeV.
002708678 540__ $$3preprint$$aarXiv nonexclusive-distrib 1.0$$uhttp://arxiv.org/licenses/nonexclusive-distrib/1.0/
002708678 540__ $$3publication$$aCC-BY-4.0$$bAPS$$fSCOAP3$$uhttps://creativecommons.org/licenses/by/4.0/
002708678 542__ $$3publication$$dauthors$$g2021
002708678 65017 $$2arXiv$$ahep-ph
002708678 65017 $$2SzGeCERN$$aParticle Physics - Phenomenology
002708678 65017 $$2arXiv$$ahep-ex
002708678 65017 $$2SzGeCERN$$aParticle Physics - Experiment
002708678 690C_ $$aCERN
002708678 690C_ $$aARTICLE
002708678 693__ $$aCERN LHC$$eMOEDAL
002708678 700__ $$aAlexandre, J.$$uKing's Coll. London$$vTheoretical Particle Physics & Cosmology Group, Physics Dept., King's College London, UK
002708678 700__ $$aBenes, P.$$uIEAP CTU, Prague$$vIEAP, Czech Technical University in Prague, Czech~Republic
002708678 700__ $$aBergmann, B.$$uIEAP CTU, Prague$$vIEAP, Czech Technical University in Prague, Czech~Republic
002708678 700__ $$aBernabéu, J.$$uValencia U., IFIC$$vIFIC, Universitat de València - CSIC, Valencia, Spain
002708678 700__ $$aBevan, A.$$uQueen Mary, U. of London$$vSchool of Physics and Astronomy, Queen Mary University of London, UK
002708678 700__ $$aBranzas, H.$$uBucharest, Inst. Space Science$$vInstitute of Space Science, Bucharest - Măgurele, Romania
002708678 700__ $$aBurian, P.$$uIEAP CTU, Prague$$vIEAP, Czech Technical University in Prague, Czech~Republic
002708678 700__ $$aCampbell, M.$$uCERN$$vExperimental Physics Department, CERN, Geneva, Switzerland
002708678 700__ $$aCecchini, S.$$uINFN, Bologna$$vINFN, Section of Bologna, Bologna, Italy
002708678 700__ $$aCho, Y.M.$$uCQUeST, Seoul$$uKonkuk U.$$vCenter for Quantum Spacetime, Sogang University, Seoul, Korea$$vPhysics Department, Konkuk University, Seoul, Korea
002708678 700__ $$ade Montigny, M.$$uAlberta U.$$vPhysics Department, University of Alberta, Edmonton, Alberta, Canada
002708678 700__ $$aDe Roeck, A.$$uCERN$$vExperimental Physics Department, CERN, Geneva, Switzerland
002708678 700__ $$aEllis, J.R.$$uNICPB, Tallinn$$uKing's Coll. London$$uCERN$$vNational Institute of Chemical Physics & Biophysics, Tallinn, Estonia$$vTheoretical Particle Physics & Cosmology Group, Physics Dept., King's College London, UK$$vTheoretical Physics Department, CERN, Geneva, Switzerland
002708678 700__ $$aEl Sawy, M.$$uBeni-Suef U.$$uCERN$$vDepartment of Physics, Faculty of Science, Beni-Suef University, Beni-Suef, Egypt$$vExperimental Physics Department, CERN, Geneva, Switzerland
002708678 700__ $$aFairbairn, M.$$uKing's Coll. London$$vTheoretical Particle Physics & Cosmology Group, Physics Dept., King's College London, UK
002708678 700__ $$aFelea, D.$$uBucharest, Inst. Space Science$$vInstitute of Space Science, Bucharest - Măgurele, Romania
002708678 700__ $$aFrank, M.$$uConcordia U., Montreal$$vDepartment of Physics, Concordia University, Montréal, Québec, Canada
002708678 700__ $$aHays, J.$$uQueen Mary, U. of London$$vSchool of Physics and Astronomy, Queen Mary University of London, UK
002708678 700__ $$aHirt, A.M.$$uZurich, ETH$$vDepartment of Earth Sciences, Swiss Federal Institute of Technology, Zurich, Switzerland
002708678 700__ $$aJanecek, J.$$uIEAP CTU, Prague$$vIEAP, Czech Technical University in Prague, Czech~Republic
002708678 700__ $$aKalliokoski, M.$$uBoskovic Inst., Zagreb$$vThe Center for Detectors, Sensors and Electronics (CDSE) of the Ruder Boscovic Institute, Zagreb, Croatia.
002708678 700__ $$aKorzenev, A.$$uGeneva U.$$vDépartement de Physique Nucléaire et Corpusculaire, Université de Genève, Geneva, Switzerland
002708678 700__ $$aLacarrère, D.H.$$uCERN$$vExperimental Physics Department, CERN, Geneva, Switzerland
002708678 700__ $$aLeroy, C.$$uMontreal U.$$vDépartement de Physique, Universitéde Montréal, Québec, Canada
002708678 700__ $$aLevi, G.$$uINFN, Bologna$$uU. Bologna, DIFA$$vINFN, Section of Bologna & Department of Physics & Astronomy, University of Bologna, Italy
002708678 700__ $$aLionti, A.$$uGeneva U.$$vDépartement de Physique Nucléaire et Corpusculaire, Université de Genève, Geneva, Switzerland
002708678 700__ $$aMamuzic, J.$$uValencia U., IFIC$$vIFIC, Universitat de València - CSIC, Valencia, Spain
002708678 700__ $$aMaulik, A.$$uINFN, Bologna$$uAlberta U.$$vINFN, Section of Bologna, Bologna, Italy$$vPhysics Department, University of Alberta, Edmonton, Alberta, Canada
002708678 700__ $$aMargiotta, A.$$uINFN, Bologna$$uU. Bologna, DIFA$$vINFN, Section of Bologna & Department of Physics & Astronomy, University of Bologna, Italy
002708678 700__ $$aMauri, N.$$uINFN, Bologna$$vINFN, Section of Bologna, Bologna, Italy
002708678 700__ $$aMavromatos, N.E.$$uKing's Coll. London$$vTheoretical Particle Physics & Cosmology Group, Physics Dept., King's College London, UK
002708678 700__ $$aMermod, P.$$uGeneva U.$$vDépartement de Physique Nucléaire et Corpusculaire, Université de Genève, Geneva, Switzerland
002708678 700__ $$aMieskolainen, M.$$uHelsinki U.$$vPhysics Department, University of Helsinki, Helsinki, Finland
002708678 700__ $$aMillward, L.$$uQueen Mary, U. of London$$vSchool of Physics and Astronomy, Queen Mary University of London, UK
002708678 700__ $$aMitsou, V.A.$$uValencia U., IFIC$$vIFIC, Universitat de València - CSIC, Valencia, Spain
002708678 700__ $$aOrava, R.$$uHelsinki U.$$vPhysics Department, University of Helsinki, Helsinki, Finland
002708678 700__ $$aOstrovskiy, I.$$uAlabama U.$$vDepartment of Physics and Astronomy, University of Alabama, Tuscaloosa, Alabama, USA
002708678 700__ $$aOuimet, P.-P.$$uRegina U.$$uAlberta U.$$vPhysics Department, University of Regina, Regina, Saskatchewan, Canada$$vPhysics Department, University of Alberta, Edmonton, Alberta, Canada
002708678 700__ $$aPapavassiliou, J.$$uValencia U., IFIC$$vIFIC, Universitat de València - CSIC, Valencia, Spain
002708678 700__ $$aParker, B.$$uInst. Res. in Schools, UK$$vInstitute for Research in Schools, Canterbury, UK
002708678 700__ $$aPatrizii, L.$$uINFN, Bologna$$vINFN, Section of Bologna, Bologna, Italy
002708678 700__ $$aPăvălaş, G.E.$$uBucharest, Inst. Space Science$$vInstitute of Space Science, Bucharest - Măgurele, Romania
002708678 700__ $$aPinfold, J.L.$$jORCID:[email protected]$$uAlberta U.$$vPhysics Department, University of Alberta, Edmonton, Alberta, Canada
002708678 700__ $$aPopa, L.A.$$uBucharest, Inst. Space Science$$vInstitute of Space Science, Bucharest - Măgurele, Romania
002708678 700__ $$aPopa, V.$$uBucharest, Inst. Space Science$$vInstitute of Space Science, Bucharest - Măgurele, Romania
002708678 700__ $$aPozzato, M.$$uINFN, Bologna$$vINFN, Section of Bologna, Bologna, Italy
002708678 700__ $$aPospisil, S.$$uIEAP CTU, Prague$$vIEAP, Czech Technical University in Prague, Czech~Republic
002708678 700__ $$aRajantie, A.$$uImperial Coll., London$$vDepartment of Physics, Imperial College London, UK
002708678 700__ $$aRuiz de Austri, R.$$uValencia U., IFIC$$vIFIC, Universitat de València - CSIC, Valencia, Spain
002708678 700__ $$aSahnoun, Z.$$uCNAAG, Algiers$$uINFN, Bologna$$vCentre for Astronomy, Astrophysics and Geophysics, Algiers, Algeria$$vINFN, Section of Bologna, Bologna, Italy
002708678 700__ $$aSakellariadou, M.$$uKing's Coll. London$$vTheoretical Particle Physics & Cosmology Group, Physics Dept., King's College London, UK
002708678 700__ $$aSantra, A.$$uValencia U., IFIC$$vIFIC, Universitat de València - CSIC, Valencia, Spain
002708678 700__ $$aSarkar, S.$$uKing's Coll. London$$vTheoretical Particle Physics & Cosmology Group, Physics Dept., King's College London, UK
002708678 700__ $$aSemenoff, G.$$uBritish Columbia U.$$vDepartment of Physics, University of British Columbia, Vancouver, British Columbia, Canada
002708678 700__ $$aShaa, A.$$uAlberta U.$$vPhysics Department, University of Alberta, Edmonton, Alberta, Canada
002708678 700__ $$aSirri, G.$$uINFN, Bologna$$vINFN, Section of Bologna, Bologna, Italy
002708678 700__ $$aSliwa, K.$$uTufts U.$$vDepartment of Physics and Astronomy, Tufts University, Medford, Massachusetts, USA
002708678 700__ $$aSoluk, R.$$uAlberta U.$$vPhysics Department, University of Alberta, Edmonton, Alberta, Canada
002708678 700__ $$aSpurio, M.$$uINFN, Bologna$$uU. Bologna, DIFA$$vINFN, Section of Bologna & Department of Physics & Astronomy, University of Bologna, Italy
002708678 700__ $$aStaelens, M.$$uAlberta U.$$vPhysics Department, University of Alberta, Edmonton, Alberta, Canada
002708678 700__ $$aSuk, M.$$uIEAP CTU, Prague$$vIEAP, Czech Technical University in Prague, Czech~Republic
002708678 700__ $$aTenti, M.$$uINFN, CNAF$$vINFN, CNAF, Bologna, Italy
002708678 700__ $$aTogo, V.$$uINFN, Bologna$$vINFN, Section of Bologna, Bologna, Italy
002708678 700__ $$aTuszyński, J.A.$$uAlberta U.$$vPhysics Department, University of Alberta, Edmonton, Alberta, Canada
002708678 700__ $$aUpreti, A.$$uAlabama U.$$vDepartment of Physics and Astronomy, University of Alabama, Tuscaloosa, Alabama, USA
002708678 700__ $$aVento, V.$$uValencia U., IFIC$$vIFIC, Universitat de València - CSIC, Valencia, Spain
002708678 700__ $$aVives, O.$$uValencia U., IFIC$$vIFIC, Universitat de València - CSIC, Valencia, Spain
002708678 700__ $$aWall, A.$$uAlabama U.$$vDepartment of Physics and Astronomy, University of Alabama, Tuscaloosa, Alabama, USA
002708678 710__ $$gMoEDAL Collaboration
002708678 773__ $$c071801$$mpublication$$n7$$pPhys. Rev. Lett.$$v126$$xPhys. Rev. Lett. 126, 071801 (2021)$$y2021
002708678 8564_ $$82201013$$s6056523$$uhttp://cds.cern.ch/record/2708678/files/Spin1-3gd-lowe-x.png$$y00017 Cross-section upper limits at 95\% CL for DY dyon pair-production, with magnetic charge 3$\gd$ and multiple electric charges, in 13~\tev $pp$ collisions as a function of spin. The solid lines are leading order cross-section calculations.
002708678 8564_ $$82201014$$s7036923$$uhttp://cds.cern.ch/record/2708678/files/Spinhalf-2gd-highe-x.png$$y00010 Cross-section upper limits at 95\% CL for DY dyon pair-production, with magnetic charge 2$\gd$ and multiple electric charges, in 13~\tev $pp$ collisions as a function of spin. The solid lines are leading order cross-section calculations.
002708678 8564_ $$82201015$$s5053113$$uhttp://cds.cern.ch/record/2708678/files/Spin0-5gd-highe-x.png$$y00026 Cross-section upper limits at 95\% CL for DY dyon pair-production, with magnetic charge 5$g_{D}$ and 6$g_{D}$ and multiple electric charges in 13~\tev $pp$ collisions as a function of spin. The solid lines are leading order cross-section calculations.
002708678 8564_ $$82201016$$s7411988$$uhttp://cds.cern.ch/record/2708678/files/Spin1-1gd-highe-x.png$$y00006 Cross-section upper limits at 95\% CL for DY dyon pair-production, with magnetic charge 1$g_{D}$ and multiple electric charges, in 13~\tev $pp$ collisions as a function of spin. The solid lines are leading-order cross-section calculations.
002708678 8564_ $$82201017$$s6736053$$uhttp://cds.cern.ch/record/2708678/files/Spinhalf-1gd-highe-x.png$$y00004 Cross-section upper limits at 95\% CL for DY dyon pair-production, with magnetic charge 1$g_{D}$ and multiple electric charges, in 13~\tev $pp$ collisions as a function of spin. The solid lines are leading-order cross-section calculations.
002708678 8564_ $$82201018$$s6010248$$uhttp://cds.cern.ch/record/2708678/files/Spinhalf-5gd-lowe-x.png$$y00027 Cross-section upper limits at 95\% CL for DY dyon pair-production, with magnetic charge 5$g_{D}$ and 6$g_{D}$ and multiple electric charges in 13~\tev $pp$ collisions as a function of spin. The solid lines are leading order cross-section calculations.
002708678 8564_ $$82201019$$s6161594$$uhttp://cds.cern.ch/record/2708678/files/Spin0-1gd-lowe-x.png$$y00001 Cross-section upper limits at 95\% CL for DY dyon pair-production, with magnetic charge 1$g_{D}$ and multiple electric charges, in 13~\tev $pp$ collisions as a function of spin. The solid lines are leading-order cross-section calculations.
002708678 8564_ $$82201020$$s6682568$$uhttp://cds.cern.ch/record/2708678/files/Spin0-4gd-highe-x.png$$y00020 Cross-section upper limits at 95\% CL for DY dyon pair-production, with magnetic charge 4$\gd$ and multiple electric charges, in 13~\tev $pp$ collisions as a function of spin. The solid lines are leading order cross-section calculations.
002708678 8564_ $$82201021$$s1054105$$uhttp://cds.cern.ch/record/2708678/files/2002.00861.pdf$$yFulltext
002708678 8564_ $$82201022$$s5990878$$uhttp://cds.cern.ch/record/2708678/files/Spinhalf-4gd-highe-x.png$$y00022 Cross-section upper limits at 95\% CL for DY dyon pair-production, with magnetic charge 4$\gd$ and multiple electric charges, in 13~\tev $pp$ collisions as a function of spin. The solid lines are leading order cross-section calculations.
002708678 8564_ $$82201023$$s4937490$$uhttp://cds.cern.ch/record/2708678/files/Spin1-6gd-highe-x.png$$y00032 Cross-section upper limits at 95\% CL for DY dyon pair-production, with magnetic charge 5$g_{D}$ and 6$g_{D}$ and multiple electric charges in 13~\tev $pp$ collisions as a function of spin. The solid lines are leading order cross-section calculations.
002708678 8564_ $$82201024$$s5784716$$uhttp://cds.cern.ch/record/2708678/files/Spin1-2gd-lowe-x.png$$y00011 Cross-section upper limits at 95\% CL for DY dyon pair-production, with magnetic charge 2$\gd$ and multiple electric charges, in 13~\tev $pp$ collisions as a function of spin. The solid lines are leading order cross-section calculations.
002708678 8564_ $$82201025$$s5740503$$uhttp://cds.cern.ch/record/2708678/files/Spin1-5gd-highe-x.png$$y00030 Cross-section upper limits at 95\% CL for DY dyon pair-production, with magnetic charge 5$g_{D}$ and 6$g_{D}$ and multiple electric charges in 13~\tev $pp$ collisions as a function of spin. The solid lines are leading order cross-section calculations.
002708678 8564_ $$82201026$$s6539270$$uhttp://cds.cern.ch/record/2708678/files/Spinhalf-4gd-lowe-x.png$$y00021 Cross-section upper limits at 95\% CL for DY dyon pair-production, with magnetic charge 4$\gd$ and multiple electric charges, in 13~\tev $pp$ collisions as a function of spin. The solid lines are leading order cross-section calculations.
002708678 8564_ $$82201027$$s6919450$$uhttp://cds.cern.ch/record/2708678/files/Spin0-2gd-highe-x.png$$y00008 Cross-section upper limits at 95\% CL for DY dyon pair-production, with magnetic charge 2$\gd$ and multiple electric charges, in 13~\tev $pp$ collisions as a function of spin. The solid lines are leading order cross-section calculations.
002708678 8564_ $$82201028$$s6239035$$uhttp://cds.cern.ch/record/2708678/files/Spin0-4gd-lowe-x.png$$y00019 Cross-section upper limits at 95\% CL for DY dyon pair-production, with magnetic charge 4$\gd$ and multiple electric charges, in 13~\tev $pp$ collisions as a function of spin. The solid lines are leading order cross-section calculations.
002708678 8564_ $$82201029$$s6120370$$uhttp://cds.cern.ch/record/2708678/files/Spin0-2gd-lowe-x.png$$y00007 Cross-section upper limits at 95\% CL for DY dyon pair-production, with magnetic charge 2$\gd$ and multiple electric charges, in 13~\tev $pp$ collisions as a function of spin. The solid lines are leading order cross-section calculations.
002708678 8564_ $$82201030$$s7465220$$uhttp://cds.cern.ch/record/2708678/files/Spin0-3gd-highe-x.png$$y00014 Cross-section upper limits at 95\% CL for DY dyon pair-production, with magnetic charge 3$\gd$ and multiple electric charges, in 13~\tev $pp$ collisions as a function of spin. The solid lines are leading order cross-section calculations.
002708678 8564_ $$82201031$$s6779892$$uhttp://cds.cern.ch/record/2708678/files/Spinhalf-3gd-highe-x.png$$y00016 Cross-section upper limits at 95\% CL for DY dyon pair-production, with magnetic charge 3$\gd$ and multiple electric charges, in 13~\tev $pp$ collisions as a function of spin. The solid lines are leading order cross-section calculations.
002708678 8564_ $$82201032$$s6176218$$uhttp://cds.cern.ch/record/2708678/files/Spin1-4gd-lowe-x.png$$y00023 Cross-section upper limits at 95\% CL for DY dyon pair-production, with magnetic charge 4$\gd$ and multiple electric charges, in 13~\tev $pp$ collisions as a function of spin. The solid lines are leading order cross-section calculations.
002708678 8564_ $$82201033$$s6687966$$uhttp://cds.cern.ch/record/2708678/files/Spin0-1gd-highe-x.png$$y00002 Cross-section upper limits at 95\% CL for DY dyon pair-production, with magnetic charge 1$g_{D}$ and multiple electric charges, in 13~\tev $pp$ collisions as a function of spin. The solid lines are leading-order cross-section calculations.
002708678 8564_ $$82201034$$s5853877$$uhttp://cds.cern.ch/record/2708678/files/Spin0-5gd-lowe-x.png$$y00025 Cross-section upper limits at 95\% CL for DY dyon pair-production, with magnetic charge 5$g_{D}$ and 6$g_{D}$ and multiple electric charges in 13~\tev $pp$ collisions as a function of spin. The solid lines are leading order cross-section calculations.
002708678 8564_ $$82201035$$s7410165$$uhttp://cds.cern.ch/record/2708678/files/Spin1-2gd-highe-x.png$$y00012 Cross-section upper limits at 95\% CL for DY dyon pair-production, with magnetic charge 2$\gd$ and multiple electric charges, in 13~\tev $pp$ collisions as a function of spin. The solid lines are leading order cross-section calculations.
002708678 8564_ $$82201036$$s6775998$$uhttp://cds.cern.ch/record/2708678/files/Spin1-3gd-highe-x.png$$y00018 Cross-section upper limits at 95\% CL for DY dyon pair-production, with magnetic charge 3$\gd$ and multiple electric charges, in 13~\tev $pp$ collisions as a function of spin. The solid lines are leading order cross-section calculations.
002708678 8564_ $$82201037$$s6326128$$uhttp://cds.cern.ch/record/2708678/files/Spinhalf-2gd-lowe-x.png$$y00009 Cross-section upper limits at 95\% CL for DY dyon pair-production, with magnetic charge 2$\gd$ and multiple electric charges, in 13~\tev $pp$ collisions as a function of spin. The solid lines are leading order cross-section calculations.
002708678 8564_ $$82201038$$s4667012$$uhttp://cds.cern.ch/record/2708678/files/Spinhalf-5gd-highe-x.png$$y00028 Cross-section upper limits at 95\% CL for DY dyon pair-production, with magnetic charge 5$g_{D}$ and 6$g_{D}$ and multiple electric charges in 13~\tev $pp$ collisions as a function of spin. The solid lines are leading order cross-section calculations.
002708678 8564_ $$82201039$$s53120$$uhttp://cds.cern.ch/record/2708678/files/dy-diagram.png$$y00000 Feynman-like diagram for dyon-pair direct production at leading order via the benchmark Drell-Yan mechanism. The coupling $g'$ is given by $\sqrt{(g^{2} + q^{2})}$, in the eikonal approximation that is valid for LHC energies.
002708678 8564_ $$82201040$$s5687517$$uhttp://cds.cern.ch/record/2708678/files/Spin1-5gd-lowe-x.png$$y00029 Cross-section upper limits at 95\% CL for DY dyon pair-production, with magnetic charge 5$g_{D}$ and 6$g_{D}$ and multiple electric charges in 13~\tev $pp$ collisions as a function of spin. The solid lines are leading order cross-section calculations.
002708678 8564_ $$82201041$$s5891091$$uhttp://cds.cern.ch/record/2708678/files/Spinhalf-1gd-lowe-x.png$$y00003 Cross-section upper limits at 95\% CL for DY dyon pair-production, with magnetic charge 1$g_{D}$ and multiple electric charges, in 13~\tev $pp$ collisions as a function of spin. The solid lines are leading-order cross-section calculations.
002708678 8564_ $$82201042$$s6357880$$uhttp://cds.cern.ch/record/2708678/files/Spin0-3gd-lowe-x.png$$y00013 Cross-section upper limits at 95\% CL for DY dyon pair-production, with magnetic charge 3$\gd$ and multiple electric charges, in 13~\tev $pp$ collisions as a function of spin. The solid lines are leading order cross-section calculations.
002708678 8564_ $$82201043$$s6337805$$uhttp://cds.cern.ch/record/2708678/files/Spinhalf-3gd-lowe-x.png$$y00015 Cross-section upper limits at 95\% CL for DY dyon pair-production, with magnetic charge 3$\gd$ and multiple electric charges, in 13~\tev $pp$ collisions as a function of spin. The solid lines are leading order cross-section calculations.
002708678 8564_ $$82201044$$s6520580$$uhttp://cds.cern.ch/record/2708678/files/Spin1-4gd-highe-x.png$$y00024 Cross-section upper limits at 95\% CL for DY dyon pair-production, with magnetic charge 4$\gd$ and multiple electric charges, in 13~\tev $pp$ collisions as a function of spin. The solid lines are leading order cross-section calculations.
002708678 8564_ $$82201045$$s6223220$$uhttp://cds.cern.ch/record/2708678/files/Spin1-1gd-lowe-x.png$$y00005 Cross-section upper limits at 95\% CL for DY dyon pair-production, with magnetic charge 1$g_{D}$ and multiple electric charges, in 13~\tev $pp$ collisions as a function of spin. The solid lines are leading-order cross-section calculations.
002708678 8564_ $$82201046$$s5241881$$uhttp://cds.cern.ch/record/2708678/files/Spin1-6gd-lowe-x.png$$y00031 Cross-section upper limits at 95\% CL for DY dyon pair-production, with magnetic charge 5$g_{D}$ and 6$g_{D}$ and multiple electric charges in 13~\tev $pp$ collisions as a function of spin. The solid lines are leading order cross-section calculations.
002708678 8564_ $$82250126$$s167269$$uhttp://cds.cern.ch/record/2708678/files/high-e.png$$y00002 Cross-section upper limits at 95\% CL for DY spin-0, 1/2 and 1 dyon-pair production, with magnetic charge 1$g_{D}$ and multiple electric charges, in 13~\tev $pp$ collisions. The solid lines are leading-order cross-section calculations.
002708678 8564_ $$82250127$$s142256$$uhttp://cds.cern.ch/record/2708678/files/low-e.png$$y00001 Cross-section upper limits at 95\% CL for DY spin-0, 1/2 and 1 dyon-pair production, with magnetic charge 1$g_{D}$ and multiple electric charges, in 13~\tev $pp$ collisions. The solid lines are leading-order cross-section calculations.
002708678 8564_ $$82278478$$s529893$$uhttp://cds.cern.ch/record/2708678/files/scoap3-fulltext.pdf$$yArticle from SCOAP3
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