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dc.contributor.author
Aad, G.
dc.contributor.author
Abbott, B.
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Abdallah, J.
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Abdel Khalek, S.
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Abdinov, O.
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Otero y Garzon, Gustavo Javier
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Piegaia, Ricardo Nestor
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Sacerdoti, Sabrina
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Reisin, Hernan Diego
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Alconada Verzini, María Josefina
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Alonso, Francisco
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Anduaga, Xabier Sebastian
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Dova, Maria Teresa
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Monticelli, Fernando Gabriel
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Wahlberg, Hernan Pablo
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Zhuang, X.
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Zhukov, K.
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Zibell, A.
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Zieminska, D.
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Zimine, N. I.
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Zimmermann, C.
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Zimmermann, R.
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Zimmermann, S.
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Zimmermann, S.
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Ziolkowski, M.
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Zobernig, G.
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Zoccoli, A.
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Nedden, M. zur
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Zurzolo, G.
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Zutshi, V.
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Zwalinski, L.
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The ATLAS Collaboration
dc.date.available
2020-06-24T17:38:41Z
dc.date.issued
2014-09
dc.identifier.citation
Aad, G.; Abbott, B.; Abdallah, J.; Abdel Khalek, S.; Abdinov, O.; et al.; Search for pair-produced third-generation squarks decaying via charm quarks or in compressed supersymmetric scenarios in pp collisions at s√=8 TeV with the ATLAS detector; American Physical Society; Physical Review D: Particles, Fields, Gravitation and Cosmology; D90; 9-2014; 052008-43
dc.identifier.issn
1550-7998
dc.identifier.uri
http://hdl.handle.net/11336/108111
dc.description.abstract
Results of a search for supersymmetry via direct production of third-generation squarks are reported, using 20.3 fb−1 of proton-proton collision data at s√=8 TeV recorded by the ATLAS experiment at the LHC in 2012. Two different analysis strategies based on monojet-like and c-tagged event selections are carried out to optimize the sensitivity for direct top squark pair production in the decay channel to a charm quark and the lightest neutralino (t̃ 1→c+χ̃ 01) across the top squark--neutralino mass parameter space. No excess above the Standard Model background expectation is observed. The results are interpreted in the context of direct pair production of top squarks and presented in terms of exclusion limits in the (mt̃ 1, mχ̃ 01) parameter space. A top squark of mass up to about 240 GeV is excluded at 95% confidence level for arbitrary neutralino masses, within the kinematic boundaries. Top squark masses up to 270 GeV are excluded for a neutralino mass of 200 GeV. In a scenario where the top squark and the lightest neutralino are nearly degenerate in mass, top squark masses up to 260 GeV are excluded. The results from the monojet-like analysis are also interpreted in terms of compressed scenarios for top squark pair production in the decay channel t̃ 1→b+ff′+χ̃ 01 and sbottom pair production with b̃ 1→b+χ̃ 01, leading to a similar exclusion for nearly mass-degenerate third-generation squarks and the lightest neutralino. The results in this paper significantly extend previous results at colliders.
dc.format
application/pdf
dc.language.iso
eng
dc.publisher
American Physical Society
dc.rights
info:eu-repo/semantics/openAccess
dc.rights.uri
https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
dc.subject
High Energy
dc.subject
Experiment
dc.subject.classification
Astronomía
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Ciencias Físicas
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CIENCIAS NATURALES Y EXACTAS
dc.title
Search for pair-produced third-generation squarks decaying via charm quarks or in compressed supersymmetric scenarios in pp collisions at s√=8 TeV with the ATLAS detector
dc.type
info:eu-repo/semantics/article
dc.type
info:ar-repo/semantics/artículo
dc.type
info:eu-repo/semantics/publishedVersion
dc.date.updated
2018-01-12T16:31:26Z
dc.journal.volume
D90
dc.journal.pagination
052008-43
dc.journal.pais
Estados Unidos
dc.journal.ciudad
New York
dc.description.fil
Fil: Dova, Maria Teresa. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto de Física La Plata. Universidad Nacional de La Plata. Facultad de Ciencias Exactas. Instituto de Física La Plata; Argentina. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto de Física La Plata. Universidad Nacional de La Plata. Facultad de Ciencias Exactas. Instituto de Física La Plata; Argentina
dc.description.fil
Fil: Dova, Maria Teresa.
dc.journal.title
Physical Review D: Particles, Fields, Gravitation and Cosmology
dc.relation.alternativeid
info:eu-repo/semantics/altIdentifier/doi/http://dx.doi.org/10.1103/PhysRevD.90.052008
dc.relation.alternativeid
info:eu-repo/semantics/altIdentifier/url/https://journals.aps.org/prd/abstract/10.1103/PhysRevD.90.052008
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