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Matches in Ghent University Academic Bibliography for { <https://biblio.ugent.be/publication/01JHFXEXH5ME7HVCMHYFHXSSBN> ?p ?o. }

• 01JHFXEXH5ME7HVCMHYFHXSSBN classification A1.
• 01JHFXEXH5ME7HVCMHYFHXSSBN date "2024".
• 01JHFXEXH5ME7HVCMHYFHXSSBN language "eng".
• 01JHFXEXH5ME7HVCMHYFHXSSBN type journalArticle.
• 01JHFXEXH5ME7HVCMHYFHXSSBN hasPart 01JHFXFJ3PKGBZ4R8Q6C6Q498H.pdf.
• 01JHFXEXH5ME7HVCMHYFHXSSBN subject "Physics and Astronomy".
• 01JHFXEXH5ME7HVCMHYFHXSSBN doi "10.1103/PhysRevD.109.072007".
• 01JHFXEXH5ME7HVCMHYFHXSSBN issn "2470-0010".
• 01JHFXEXH5ME7HVCMHYFHXSSBN issn "2470-0029".
• 01JHFXEXH5ME7HVCMHYFHXSSBN issue "7".
• 01JHFXEXH5ME7HVCMHYFHXSSBN volume "109".
• 01JHFXEXH5ME7HVCMHYFHXSSBN abstract "A search is presented for charged, long-lived supersymmetric particles in final states with one or more disappearing tracks. The search is based on data from proton-proton collisions at a center-of-mass energy of 13 TeV collected with the CMS detector at the CERN LHC between 2016 and 2018, corresponding to an integrated luminosity of 137 fb(-1). The search is performed over final states characterized by varying numbers of jets, b-tagged jets, electrons, and muons. The length of signal-candidate tracks in the plane perpendicular to the beam axis is used to characterize the lifetimes of wino- and Higgsino-like charginos produced in the context of the minimal supersymmetric standard model. The dE/dx energy loss of signal-candidate tracks is used to increase the sensitivity to charginos with a large mass and thus a small Lorentz boost. The observed results are found to be statistically consistent with the background-only hypothesis. Limits on the pair-production cross section of gluinos and squarks are presented in the framework of simplified models of supersymmetric particle production and decay, and for electroweakino production based on models of wino and Higgsino dark matter. The limits presented are the most stringent to date for scenarios with light third-generation squarks and a wino- or Higgsino-like dark matter candidate capable of explaining the observed dark matter relic density.".
• 01JHFXEXH5ME7HVCMHYFHXSSBN author 481d1d32-4c85-11eb-808e-8ab49d8c46c1.
• 01JHFXEXH5ME7HVCMHYFHXSSBN author 54FE3FAA-05F6-11E3-970D-B3B910BDE39D.
• 01JHFXEXH5ME7HVCMHYFHXSSBN author 7d67629a-9f9c-11ea-96ba-d014da0b18cb.
• 01JHFXEXH5ME7HVCMHYFHXSSBN author 946BA6A4-6FC6-11E6-B34B-B74CB5D1D7B1.
• 01JHFXEXH5ME7HVCMHYFHXSSBN author 9835284b-ea17-11e9-a0da-a582e24a4a34.
• 01JHFXEXH5ME7HVCMHYFHXSSBN author C0D62136-E687-11E2-AD28-C2B310BDE39D.
• 01JHFXEXH5ME7HVCMHYFHXSSBN author C69762EA-02FD-11E4-89C9-5E074B2F559A.
• 01JHFXEXH5ME7HVCMHYFHXSSBN author CCD81336-4F36-11E4-A93C-06A6B5D1D7B1.
• 01JHFXEXH5ME7HVCMHYFHXSSBN author E93CD864-C937-11E5-A139-C70DB5D1D7B1.
• 01JHFXEXH5ME7HVCMHYFHXSSBN author F4E76394-F0ED-11E1-A9DE-61C894A0A6B4.
• 01JHFXEXH5ME7HVCMHYFHXSSBN author F86D2B4A-9285-11E7-BDF5-1B0FAE28A064.
• 01JHFXEXH5ME7HVCMHYFHXSSBN author a1dea179-e5d3-11e9-b023-f6712251f5d0.
• 01JHFXEXH5ME7HVCMHYFHXSSBN author f74f4369-9ffc-11ec-a2d8-f591dcbf69ce.
• 01JHFXEXH5ME7HVCMHYFHXSSBN author urn:uuid:0002169d-7108-464c-b74b-9f380eb79b24.
• 01JHFXEXH5ME7HVCMHYFHXSSBN author urn:uuid:002e46e9-f048-4408-a7f1-175781e8f9c2.
• 01JHFXEXH5ME7HVCMHYFHXSSBN author urn:uuid:004b4c1f-80a0-4a44-a372-7392e016a7db.
• 01JHFXEXH5ME7HVCMHYFHXSSBN author urn:uuid:006e94a9-fef6-42d3-b851-abc2f6d5b926.
• 01JHFXEXH5ME7HVCMHYFHXSSBN author urn:uuid:00730916-92d1-4c45-80f0-0cde636e1699.
• 01JHFXEXH5ME7HVCMHYFHXSSBN author urn:uuid:00792f9d-8896-442a-b7f3-4a61bd785b3b.
• 01JHFXEXH5ME7HVCMHYFHXSSBN author urn:uuid:00d03c5e-9193-4864-aa73-95f32f30603c.
• 01JHFXEXH5ME7HVCMHYFHXSSBN author urn:uuid:01003449-5a53-4a50-b78a-c0487fa17725.
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• 01JHFXEXH5ME7HVCMHYFHXSSBN author urn:uuid:011524ec-be75-4f30-b208-22b766ca6f64.
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• 01JHFXEXH5ME7HVCMHYFHXSSBN author urn:uuid:01d51d9a-9fce-45f8-a12f-aa6e3fe2f026.
• 01JHFXEXH5ME7HVCMHYFHXSSBN author urn:uuid:01e2824c-76f3-4523-8bf7-261282b45c13.
• 01JHFXEXH5ME7HVCMHYFHXSSBN author urn:uuid:01f5477c-1db2-45ec-b26b-5e04c0662631.
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