2015
DOI: 10.1140/epjc/s10052-015-3599-y
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The pMSSM10 after LHC run 1

Abstract: We present a frequentist analysis of the parameter space of the pMSSM10, in which the following ten soft SUSY-breaking parameters are specified independently at the mean scalar top mass scale M SUSY ≡ √ mt 1 mt 2 :the gaugino masses M 1,2,3 , the first-and second-generation squark masses mq 1 = mq 2 , the third-generation squark mass mq 3 , a common slepton mass m˜ and a common trilinear mixing parameter A, as well as the Higgs mixing parameter μ, the pseudoscalar Higgs mass M A and tan β, the ratio of the two… Show more

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Cited by 70 publications
(101 citation statements)
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References 161 publications
(236 reference statements)
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“…Several groups have advocated the use of the pMSSM for interpretation of LHC results [33][34][35][36][37][38][39][40][41][42][43][44][45][46][47][48][49][50][51][52]. Most of these studies use estimated experimental efficiencies and acceptances for pMSSM points, and compare them to the model-independent limits from a selection of LHC searches to constrain the pMSSM parameter space.…”
Section: Jhep10(2015)134mentioning
confidence: 99%
“…Several groups have advocated the use of the pMSSM for interpretation of LHC results [33][34][35][36][37][38][39][40][41][42][43][44][45][46][47][48][49][50][51][52]. Most of these studies use estimated experimental efficiencies and acceptances for pMSSM points, and compare them to the model-independent limits from a selection of LHC searches to constrain the pMSSM parameter space.…”
Section: Jhep10(2015)134mentioning
confidence: 99%
“…Studies in the context of ultraviolet (UV) complete models like the Minimal Supersymmetric Standard Model (MSSM) allow for the most comprehensive combination of experimental data sets [7][8][9][10][11], but it is usually difficult to generalize their results to other models. Effective field theories (EFTs), on the other hand, offer highly modelindependent results, but their applicability is more restricted, especially in high energy…”
Section: Introductionmentioning
confidence: 99%
“…The no-observation of DM is starting to put some pressure on the so-called WIMP Miracle paradigm, which posits that the observed relic abundance can be explained by DM candidates which are weakly interacting massive particles (WIMPs) with masses in the 10s of GeV to a few TeV range (assuming simple 2 → 2 DM annihilation to SM particles and the standard thermal freeze-out mechanism). A growing number of such WIMP models of DM are being strongly constrained by, or at least show tension with the experimental limits, including supersymmetric DM realisations discussed in [3][4][5][6][7][8][9][10][11][12][13][14] as well as other models considered in e.g. [15,16].…”
Section: Jhep06(2017)041mentioning
confidence: 99%