{"@context":"http://schema.org","@id":"https://doi.org/10.17182/hepdata.64435.v1","@reverse":{"isBasedOn":[{"@type":"ScholarlyArticle","identifier":{"@type":"PropertyValue","propertyID":"URL","value":"https://inspirehep.net/literature/1291940"}},{"@id":"https://doi.org/10.1103/PhysRevD.90.032006","@type":"JournalArticle"}]},"@type":"Dataset","additionalType":"Collection","author":{"@type":"Organization","name":"CMS Collaboration"},"creator":{"@type":"Organization","name":"CMS Collaboration"},"datePublished":"2014","description":"CERN-LHC.  A search for physics beyond the standard model in events with at least three leptons is presented.  The data sample, corresponding to an integrated luminosity of 19.5 inverse femtobarns of proton-proton collisions with center-of-mass energy sqrt(s) = 8 TeV, was collected by the CMS experiment at the LHC during 2012.  The data are divided into exclusive categories based on the number of leptons and their flavor, the presence or absence of an opposite-sign, same-flavor lepton pair (OSSF), the invariant mass of the OSSF pair, the presence or absence of a tagged bottom-quark jet, the number of identified hadronically decaying tau leptons, and the magnitude of the missing transverse energy and of the scalar sum of jet transverse momenta.  \n\nWe also place a 95% confidence level upper limit of 1.3% on the branching fraction for the decay of a top quark to a charm quark and a Higgs boson (TOP --> CHARM HIGGS), which translates to a bound on the left- and right-handed top-charm flavor-violating Higgs Yukawa couplings, LAMBDA(HIGGS TOP CHARM) and LAMBDA(HIGGS CHARM TOP) respectively, of SQRT(ABS(LAMBDA(HIGGS TOP CHARM))**2 + ABS(LAMBDA(HIGGS CHARM TOP))**2) < 0.21. \n\nWe also present the product of the acceptance and efficiency for the calculations of the 95% C.L. in several different SUSY scenarios.","hasPart":[{"@id":"https://doi.org/10.17182/hepdata.64435.v1/t1","@type":"Dataset","description":"Observed and expected numbers of events with four or more leptons with the scalar sum of jet transverse momentum values...","name":"Table 1"},{"@id":"https://doi.org/10.17182/hepdata.64435.v1/t2","@type":"Dataset","description":"Observed and expected numbers of events with four or more leptons with the scalar sum of jet transverse momentum values...","name":"Table 2"},{"@id":"https://doi.org/10.17182/hepdata.64435.v1/t3","@type":"Dataset","description":"Observed and expected numbers of events with exactly three leptons with the scalar sum of jet transverse momentum values HT...","name":"Table 3"},{"@id":"https://doi.org/10.17182/hepdata.64435.v1/t4","@type":"Dataset","description":"Observed and expected numbers of events with exactly three leptons with the scalar sum of jet transverse momentum values HT...","name":"Table 4"},{"@id":"https://doi.org/10.17182/hepdata.64435.v1/t5","@type":"Dataset","description":"The product of acceptance and efficiency for the calculation of the 95% C.L. limits for the natural Higgsino NLSP scenario...","name":"Table 5"},{"@id":"https://doi.org/10.17182/hepdata.64435.v1/t6","@type":"Dataset","description":"The product of acceptance and efficiency for the calculation of the 95% C.L. limits for the natural Higgsino NLSP scenario...","name":"Table 6"},{"@id":"https://doi.org/10.17182/hepdata.64435.v1/t7","@type":"Dataset","description":"The product of acceptance and efficiency for the calculation of the 95% C.L. limits for the natural Higgsino NLSP scenario...","name":"Table 7"},{"@id":"https://doi.org/10.17182/hepdata.64435.v1/t8","@type":"Dataset","description":"The product of acceptance and efficiency for the calculation of the 95% C.L. limit for the natural Higgsino NLSP scenario...","name":"Table 8"},{"@id":"https://doi.org/10.17182/hepdata.64435.v1/t9","@type":"Dataset","description":"The product of acceptance and efficiency for the calculation of the 95% C.L. limit for the natural Higgsino NLSP scenario...","name":"Table 9"},{"@id":"https://doi.org/10.17182/hepdata.64435.v1/t10","@type":"Dataset","description":"The product of acceptance and efficiency for the calculation of the 95% C.L. limits for the natural Higgsino NLSP scenario...","name":"Table 10"},{"@id":"https://doi.org/10.17182/hepdata.64435.v1/t11","@type":"Dataset","description":"The product of acceptance and efficiency for the calculation of the 95% C.L. limits for the natural Higgsino NLSP scenario...","name":"Table 11"},{"@id":"https://doi.org/10.17182/hepdata.64435.v1/t12","@type":"Dataset","description":"The product of acceptance and efficiency for the calculation of the 95% C.L. limits for the natural Higgsino NLSP scenario...","name":"Table 12"},{"@id":"https://doi.org/10.17182/hepdata.64435.v1/t13","@type":"Dataset","description":"The product of acceptance and efficiency for the calculation of the 95% C.L. limits for the natural Higgsino NLSP scenario...","name":"Table 13"},{"@id":"https://doi.org/10.17182/hepdata.64435.v1/t14","@type":"Dataset","description":"The product of acceptance and efficiency for the calculation of the 95% C.L. limit on BR(NEUTRALINO1 --> HIGGS GRAVITINO) for...","name":"Table 14"},{"@id":"https://doi.org/10.17182/hepdata.64435.v1/t15","@type":"Dataset","description":"The product of acceptance and efficiency for the calculation of the 95% C.L. limit on BR(NEUTRALINO1 --> HIGGS GRAVITINO) for...","name":"Table 15"},{"@id":"https://doi.org/10.17182/hepdata.64435.v1/t16","@type":"Dataset","description":"The product of acceptance and efficiency for the calculation of the 95% C.L. limit on BR(NEUTRALINO1 --> HIGGS GRAVITINO) for...","name":"Table 16"},{"@id":"https://doi.org/10.17182/hepdata.64435.v1/t17","@type":"Dataset","description":"The product of acceptance and efficiency for the calculation of the 95% C.L. limits for the slepton co-NLSP model in...","name":"Table 17"},{"@id":"https://doi.org/10.17182/hepdata.64435.v1/t18","@type":"Dataset","description":"The product of acceptance and efficiency for the calculation of the 95% C.L. limits for the stau-NLSP and stau-NNLSP scenario...","name":"Table 18"},{"@id":"https://doi.org/10.17182/hepdata.64435.v1/t19","@type":"Dataset","description":"The product of acceptance and efficiency for the calculation of the 95% C.L. limits for the T1tttt model in the...","name":"Table 19"},{"@id":"https://doi.org/10.17182/hepdata.64435.v1/t20","@type":"Dataset","description":"The product of acceptance and efficiency for the calculation of the 95% C.L. limits for the T6ttWW model in the...","name":"Table 20"},{"@id":"https://doi.org/10.17182/hepdata.64435.v1/t21","@type":"Dataset","description":"Observed 95% C.L. exclusion contour for the T1tttt scenario.","name":"Table 21"},{"@id":"https://doi.org/10.17182/hepdata.64435.v1/t22","@type":"Dataset","description":"Observed - 1sig(theoretical) 95% C.L. exclusion contour for the T1tttt scenario.","name":"Table 22"},{"@id":"https://doi.org/10.17182/hepdata.64435.v1/t23","@type":"Dataset","description":"Observed + 1sig(theoretical) 95% C.L. exclusion contour for the T1tttt scenario.","name":"Table 23"},{"@id":"https://doi.org/10.17182/hepdata.64435.v1/t24","@type":"Dataset","description":"Expected 95% C.L. exclusion contour for the T1tttt scenario.","name":"Table 24"},{"@id":"https://doi.org/10.17182/hepdata.64435.v1/t25","@type":"Dataset","description":"Expected - 1sig 95% C.L. exclusion contour for the T1tttt scenario.","name":"Table 25"},{"@id":"https://doi.org/10.17182/hepdata.64435.v1/t26","@type":"Dataset","description":"Expected + 1sig 95% C.L. exclusion contour for the T1tttt scenario.","name":"Table 26"},{"@id":"https://doi.org/10.17182/hepdata.64435.v1/t27","@type":"Dataset","description":"Observed 95% C.L. exclusion contour for the T6ttWW scenario.","name":"Table 27"},{"@id":"https://doi.org/10.17182/hepdata.64435.v1/t28","@type":"Dataset","description":"Observed - 1sig(theoretical) 95% C.L. exclusion contour for the T6ttWW scenario.","name":"Table 28"},{"@id":"https://doi.org/10.17182/hepdata.64435.v1/t29","@type":"Dataset","description":"Observed + 1sig(theoretical) 95% C.L. exclusion contour for the T6ttWW scenario.","name":"Table 29"},{"@id":"https://doi.org/10.17182/hepdata.64435.v1/t30","@type":"Dataset","description":"Expected 95% C.L. exclusion contour for the T6ttWW scenario.","name":"Table 30"},{"@id":"https://doi.org/10.17182/hepdata.64435.v1/t31","@type":"Dataset","description":"Expected - 1sig 95% C.L. exclusion contour for the T6ttWW scenario.","name":"Table 31"},{"@id":"https://doi.org/10.17182/hepdata.64435.v1/t32","@type":"Dataset","description":"Expected + 1sig 95% C.L. exclusion contour for the T6ttWW scenario.","name":"Table 32"},{"@id":"https://doi.org/10.17182/hepdata.64435.v1/t33","@type":"Dataset","description":"Observed and expected 95% C.L. limits for the natural Higgsino NLSP scenario with BR(NEUTRALINO1 --> HIGGS GRAVITINO) = BR(NEUTRALINO1 -->...","name":"Table 33"},{"@id":"https://doi.org/10.17182/hepdata.64435.v1/t34","@type":"Dataset","description":"Observed and expected 95% C.L. limits for the natural Higgsino NLSP scenario with BR(NEUTRALINO1 --> HIGGS GRAVITINO) = 1.0 for...","name":"Table 34"},{"@id":"https://doi.org/10.17182/hepdata.64435.v1/t35","@type":"Dataset","description":"Observed and expected 95% C.L. limits for the natural Higgsino NLSP scenario with BR(NEUTRALINO1 --> Z0 GLUINO) = 1.0 for...","name":"Table 35"},{"@id":"https://doi.org/10.17182/hepdata.64435.v1/t36","@type":"Dataset","description":"Observed 95% C.L. limits on BR(NEUTRALINO1 --> HIGGS GRAVITINO) for the natural Higgsino NLSP scenario with fixed chargino-Higgsino mass of...","name":"Table 36"},{"@id":"https://doi.org/10.17182/hepdata.64435.v1/t37","@type":"Dataset","description":"Observed 95% C.L. limits on BR(NEUTRALINO1 --> HIGGS GRAVITINO) for the natural Higgsino NLSP scenario with fixed chargino-Higgsino mass of...","name":"Table 37"},{"@id":"https://doi.org/10.17182/hepdata.64435.v1/t38","@type":"Dataset","description":"Observed 95% C.L. limits on BR(NEUTRALINO1 --> HIGGS GRAVITINO) for the natural Higgsino NLSP scenario with fixed chargino-Higgsino mass of...","name":"Table 38"},{"@id":"https://doi.org/10.17182/hepdata.64435.v1/t39","@type":"Dataset","description":"Observed and expected 95% C.L. limits for the slepton co-NLSP model in the gluino-chargino (wino-like chargino) mass plane are shown.","name":"Table 39"},{"@id":"https://doi.org/10.17182/hepdata.64435.v1/t40","@type":"Dataset","description":"Observed and expected 95% C.L. limits for the stau-NLSP and stau-NNLSP scenario in the degenerate smuon- and selectron- stau mass...","name":"Table 40"},{"@id":"https://doi.org/10.17182/hepdata.64435.v1/t41","@type":"Dataset","description":"Observed and expected 95% C.L. limits for the T1tttt model in the gluino-neutralino mass plane are shown.","name":"Table 41"},{"@id":"https://doi.org/10.17182/hepdata.64435.v1/t42","@type":"Dataset","description":"Observed and expected 95% C.L. limits for the T6ttWW model in the sbottom-chargino mass plane are given.","name":"Table 42"}],"identifier":[{"@type":"PropertyValue","propertyID":"HEPDataRecord","value":"https://www.hepdata.net/record/ins1291940?version=1"},{"@type":"PropertyValue","propertyID":"HEPDataRecordAlt","value":"https://www.hepdata.net/record/64435"}],"inLanguage":"en","name":"Search for Anomalous Production of Events with Three or More Leptons in $pp$ Collisions at $\\sqrt{s} =$ 8 TeV","provider":{"@type":"Organization","name":"HEPData"},"publisher":{"@type":"Organization","name":"HEPData"},"url":"https://www.hepdata.net/record/ins1291940?version=1","version":1}