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2013
DOI: 10.1007/jhep11(2013)209
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Non-universal gaugino masses and fine tuning implications for SUSY searches in the MSSM and the GNMSSM

Abstract: For the case of the MSSM and the most general form of the NMSSM (GN-MSSM) we determine the reduction in the fine tuning that follows from allowing gaugino masses to be non-degenerate at the unification scale, taking account of the LHC8 bounds on SUSY masses, the Higgs mass bound, gauge coupling unification and the requirement of an acceptable dark matter density. We show that low-fine tuned points fall in the region of gaugino mass ratios predicted by specific unified and string models. For the case of the MSS… Show more

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Cited by 55 publications
(39 citation statements)
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References 70 publications
(111 reference statements)
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“…However, this also makes it very difficult to test even in the long run. A similar conclusion is shared in the context of gravity mediation by grand unified theory (GUT) models with the non-universal gaugino masses induced by the breaking of the GUT group [12][13][14][15][16][17][18][19].…”
Section: Introductionmentioning
confidence: 65%
“…However, this also makes it very difficult to test even in the long run. A similar conclusion is shared in the context of gravity mediation by grand unified theory (GUT) models with the non-universal gaugino masses induced by the breaking of the GUT group [12][13][14][15][16][17][18][19].…”
Section: Introductionmentioning
confidence: 65%
“…[39][40][41][42][43][44][45][46][47][48][49]. In the present paper we remain agnostic about any such correlations and take purely phenomenological point of view and calculate the fine-tuning measure as a function of physical masses of sparticles.…”
Section: Jhep08(2018)080mentioning
confidence: 99%
“…The CP-violating version of the NMSSM also received some attention [65,66]. [67][68][69] analysed the fine-tuning in a Z 3 -violating version of the NMSSM and variants. Other groups confronted the presence of a Higgs state at this mass with direct searches for SUSY particles at the LHC or Dark-Matter constraints [70][71][72].…”
Section: Jhep04(2016)095mentioning
confidence: 99%