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Gluino Meets Flavored Naturalness

Authors :
Gilad Perez
Iftah Galon
Monika Blanke
Benjamin Fuks
Institut für Theoretische Teilchenphysik
Universität Karlsruhe (TH)
Institut fur Kernphysik (Institut fur Kernphysik)
Forschung Centrum Karlsruhe
Laboratoire de Physique Théorique et Hautes Energies (LPTHE)
Université Pierre et Marie Curie - Paris 6 (UPMC)-Centre National de la Recherche Scientifique (CNRS)
Department of Physics and Astronomy [Irvine]
University of California [Irvine] (UC Irvine)
University of California (UC)-University of California (UC)
Department of Particle Physics and Astrophysics
Weizmann Institute of Science [Rehovot, Israël]
University of California [Irvine] (UCI)
University of California-University of California
Source :
Journal of High Energy Physics, Journal of High Energy Physics, 2016, 2016 (4), pp.44. ⟨10.1007/JHEP04(2016)044⟩, Journal of high energy physics, 2016 (4), 44, Journal of High Energy Physics, Springer Verlag (Germany), 2016, 2016 (4), pp.44. ⟨10.1007/JHEP04(2016)044⟩
Publication Year :
2015

Abstract

We study constraints from LHC run I on squark and gluino masses in the presence of squark flavor violation. Inspired by the concept of `flavored naturalness', we focus on the impact of a non-zero stop-scharm mixing and mass splitting in the right-handed sector. To this end, we recast four searches of the ATLAS and CMS collaborations, dedicated either to third generation squarks, to gluino and squarks of the first two generations, or to charm-squarks. In the absence of extra structure, the mass of the gluino provides an additional source of fine tuning and is therefore important to consider within models of flavored naturalness that allow for relatively light squark states. When combining the searches, the resulting constraints in the plane of the lightest squark and gluino masses are rather stable with respect to the presence of flavor-violation, and do not allow for gluino masses of less than 1.2 TeV and squarks lighter than about 550 GeV. While these constraints are stringent, interesting models with sizable stop-scharm mixing and a relatively light squark state are still viable and could be observed in the near future.<br />34 pages. v2: clarifying comments and few references added, typos fixed, matches published version

Details

Language :
English
ISSN :
10298479 and 11266708
Database :
OpenAIRE
Journal :
Journal of High Energy Physics, Journal of High Energy Physics, 2016, 2016 (4), pp.44. ⟨10.1007/JHEP04(2016)044⟩, Journal of high energy physics, 2016 (4), 44, Journal of High Energy Physics, Springer Verlag (Germany), 2016, 2016 (4), pp.44. ⟨10.1007/JHEP04(2016)044⟩
Accession number :
edsair.doi.dedup.....7f869d602f50b851dbad3632a3f04e40
Full Text :
https://doi.org/10.1007/JHEP04(2016)044⟩