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dc.contributor.authorBaringer, Philip S.
dc.contributor.authorBean, Alice
dc.contributor.authorChen, G.
dc.contributor.authorClutter, Justace Randall
dc.contributor.authorMcGivern, Carrie Lynne
dc.contributor.authorSekaric, Jadranka
dc.contributor.authorWilson, Graham Wallace
dc.contributor.authorAbazov, V. M.
dc.contributor.authorAbbott, B.
dc.contributor.authorAcharya, B. S.
dc.contributor.authorAdams, M.
dc.contributor.authorAdams, T.
dc.contributor.authorAlexeev, G. D.
dc.contributor.authorAlimena, J.
dc.contributor.authorAlkhazov, G.
dc.date.accessioned2015-05-28T13:52:46Z
dc.date.available2015-05-28T13:52:46Z
dc.date.issued2012-03-21
dc.identifier.citationAbazov, V. M. et al. (2012). "Search for Charged Massive Long-Lived Particles." Physical Review Letters, 108(12):121802. http://www.dx.doi.org/10.1103/PhysRevLett.108.121802.en_US
dc.identifier.urihttp://hdl.handle.net/1808/17856
dc.descriptionThis is the publisher's version, also available electronically from http://journals.aps.org/prl/abstract/10.1103/PhysRevLett.108.121802.en_US
dc.description.abstractWe report on a search for charged massive long-lived particles (CMLLPs), based on 5.2  fb^(−1) of integrated luminosity collected with the D0 detector at the Fermilab Tevatron ppbar collider. We search for events in which one or more particles are reconstructed as muons but have speed and ionization energy loss (dE/dx) inconsistent with muons produced in beam collisions. CMLLPs are predicted in several theories of physics beyond the standard model. We exclude pair-produced long-lived gauginolike charginos below 267 GeV and Higgsino-like charginos below 217 GeV at 95% C.L., as well as long-lived scalar top quarks with mass below 285 GeV.en_US
dc.publisherAmerican Physical Societyen_US
dc.titleSearch for Charged Massive Long-Lived Particlesen_US
dc.typeArticle
kusw.kuauthorBaringer, Philip S.
kusw.kuauthorBean, Alice
kusw.kuauthorChen, G.
kusw.kuauthorClutter, Justace Randall
kusw.kuauthorSekaric, Jadranka
kusw.kuauthorWilson, Graham Wallace
kusw.kudepartmentPhysics and Astronomyen_US
dc.identifier.doi10.1103/PhysRevLett.108.121802
kusw.oaversionScholarly/refereed, publisher version
kusw.oapolicyThis item meets KU Open Access policy criteria.
dc.rights.accessrightsopenAccess


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