2012
DOI: 10.1007/jhep01(2012)074
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Heavy flavor simplified models at the LHC

Abstract: We consider a comprehensive set of simplified models that contribute to final states with top and bottom quarks at the LHC. These simplified models are used to create minimal search strategies that ensure optimal coverage of new heavy flavor physics involving the pair production of color octets and triplets. We provide a set of benchmarks that are representative of model space, which can be used by experimentalists to perform their own optimization of search strategies. For data sets larger than 1 fb −1 , same… Show more

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Cited by 84 publications
(79 citation statements)
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“…The spectrum then contains two light neutralinos χ 0 1,2 and one chargino χ ± 1 which are gaugino-like and whose mass splitting is controlled by M 2 − M 1 , and heavier states at the scale µ which are higgsino-like. In the context of Natural SUSY [21][22][23][24][25] the opposite limit is achieved, namely µ ∼ O(100) GeV and M 1 , M 2 1 TeV. Qualitatively the same spectrum is obtained, but with the light (heavy) states being Higgsino (gaugino)-like.…”
Section: Jhep03(2014)060mentioning
confidence: 73%
“…The spectrum then contains two light neutralinos χ 0 1,2 and one chargino χ ± 1 which are gaugino-like and whose mass splitting is controlled by M 2 − M 1 , and heavier states at the scale µ which are higgsino-like. In the context of Natural SUSY [21][22][23][24][25] the opposite limit is achieved, namely µ ∼ O(100) GeV and M 1 , M 2 1 TeV. Qualitatively the same spectrum is obtained, but with the light (heavy) states being Higgsino (gaugino)-like.…”
Section: Jhep03(2014)060mentioning
confidence: 73%
“…Many third generation squark searches at the LHC rely on gluino production, with subsequent decay to stops or sbottoms [13][14][15][16][17][18][19]. This is because the production cross section for gluino is much larger than for direct stop or sbottom production, as long as the gluino mass is not much heavier.…”
Section: Introductionmentioning
confidence: 99%
“…In a recent paper, hereafter called [3], we explored the implications of the recent ATLAS and CMS searches for the NLSP stop scenario. The neutralino-stop coannihilation scenario can arise in realistic supersymmetric SU (5) and SO(10) models with b−τ Yukawa unification at M GU T [4]. In Ref.…”
Section: Introductionmentioning
confidence: 99%
“…Other recent papers related to the NLSP stop scenario are in Refs. [5][6][7][8][9][10] (other related scenarios include bino-sbottom coannihilation [11]). Motivated by these considerations in this paper we pursue a model-independent analysis of the NLSP stop scenario.…”
Section: Introductionmentioning
confidence: 99%