Artículo

Search for long-lived stopped R-hadrons decaying out-of-time with pp collisions using the ATLAS detector

Aad, G. ; Abajyan, T. ; Abbott, B. ; Abdallah, J. ; Abdel Khalek, S. ; Alonso, Francisco Icon; Anduaga, Xabier Sebastian Icon; Dova, Maria Teresa Icon; González Silva, María Laura Icon; Monticelli, Fernando Gabriel Icon; Otero y Garzon, Gustavo Javier Icon; Piegaia, Ricardo Nestor Icon; Romeo, Gaston Leonardo Icon; Tripiana, Martin Fernando Icon; Zhuang, X. ; Zibell, A. ; Zieminska, D. ; Zimin, N. I. ; Zimmermann, C. ; Zimmermann, R. ; Zimmermann, S. ; Zimmermann, S. ; Ziolkowski, M. ; Zitoun, R. ; Živković, L. ; Zobernig, G. ; Zoccoli, A. ; zur Nedden, M. ; Zurzolo, G. ; Zutshi, V. ; Zwalinski, L.

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Fecha

10/2013

Editorial

American Physical Society

Revista

Physical Review D: Particles, Fields, Gravitation and Cosmology

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ISSN

1550-7998

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Inglés

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Clasificación temática

Resumen

An updated search is performed for gluino, top squark, or bottom squark R-hadrons that have come to rest within the ATLAS calorimeter, and decay at some later time to hadronic jets and a neutralino, using 5.0 and 22.9 fb-1 of pp collisions at 7 and 8 TeV, respectively. Candidate decay events are triggered in selected empty bunch crossings of the LHC in order to remove pp collision backgrounds. Selections based on jet shape and muon-system activity are applied to discriminate signal events from cosmic ray and beam-halo muon backgrounds. In the absence of an excess of events, improved limits are set on gluino, stop, and sbottom masses for different decays, lifetimes, and neutralino masses. With a neutralino of mass 100 GeV, the analysis excludes gluinos with mass below 832 GeV (with an expected lower limit of 731 GeV), for a gluino lifetime between 10 microseconds and 1000 s in the generic R-hadron model with equal branching ratios for decays to qqbar+neutralino and gluon+neutralino. Under the same assumptions for the neutralino mass and squark lifetime, top squarks and bottom squarks in the Regge R-hadron model are excluded with masses below 379 and 344 GeV, respectively.

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