The NUHM2 after LHC Run 1

Buchmueller, O.; Cavanaugh, R.; Citron, M.; Roeck, A. De; Dolan, M. J.; Ellis, J. R.; Flaecher, H.; Heinemeyer, S.; Malik, S.; J., Marrouche,; Santos, D. Martinez; Olive, K. A.; Vries, K.J. de; Weiglein, G.

doi:10.48550/arxiv.1408.4060

Cited by 27 publications

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“…For many of these constraints, we follow very closely our previous implementations, which were summarized recently in Table 1 in [17]. Updates concerning BR(b → sγ), BR(B u → τ ν τ ), Higgs boson masses and rates etc.…”

Section: Our Methodsmentioning

confidence: 99%

“…In each panel the solid black line is for the pMSSM10, the solid blue line for the NUHM2, the dashed blue line for the NUHM1 and the dotted blue line for the CMSSM (the latter three lines are updated from Ref. [17] to include new constraints such as the LHC combined value of M h [33]). In the case of m g, we see that significantly lower masses are allowed in the pMSSM10 than in the other models: > 1250 GeV at the 68% CL and ∼ 1000 GeV at the 95% CL.…”

Section: Sparticle Massesmentioning

confidence: 99%

“…We calculate the observables that go into our likelihood evaluation using the MasterCode framework [5,6,[13][14][15][16][17][18], which interfaces various public and private codes: SoftSusy 3.3.9 [19] for the spectrum, FeynWZ [20] for the electroweak precision observables, FeynHiggs 2.10.0 [21,22] for the Higgs sector and (g −2) µ , SuFla [23], SuperIso [24] for the B-physics observables, Micromegas 3.2 [25] for the dark matter relic density, SSARD [26] for…”

Section: Acknowledgementsmentioning

confidence: 99%

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SUSY Fits and their Implications for ILC and CLIC

Heinemeyer

2016

Preprint

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Section: Our Methodsmentioning

confidence: 99%

Section: Sparticle Massesmentioning

confidence: 99%

Section: Acknowledgementsmentioning

confidence: 99%

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SUSY Fits and their Implications for ILC and CLIC

Heinemeyer

2016

Preprint

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“…In order to find values for the slepton generation mixing parameters we need a specific form of the product Y † ν Y ν as shown in Eq. (10). The simple consideration of direct hierarchical neutrinos with a common scale for right handed neutrinos provides a representative reference value.…”

Section: Mssm and Its Seesaw Extensionmentioning

confidence: 99%

“…[5] and references therein), the hypothesis of MFV has been used, and it has been assumed that the contributions coming from MFV are negligible for other observables as well, see, e.g., Ref. [10]. In this paper we will analyze whether this assumption is justified, and whether including these MFV effects could lead to additional constraints on the CMSSM parameter space.…”

Section: Introductionmentioning

confidence: 99%

Effects of sfermion mixing induced by RGE running in the minimal flavor violating CMSSM

2015

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Within the Constrained Minimal Supersymmetric Standard Model (CMSSM) with Minimal Flavor Violation (MFV) for scalar quarks, we study numerically the effects of intergenerational squark mixing on B-physics observables, electroweak precision observables (EWPO), and the Higgs-boson mass predictions. In models with universal soft terms at the GUT scale, squark mixing is generated through the Renormalization Group Equations (RGEs) running from the GUT scale to the electroweak scale due to presence of non-diagonal Yukawa matrices in the RGEs, e.g. due to the CKM matrix. Our numerical analysis is based on the code Spheno for the RGE running and full one-loop calculations, supplemented by further higher-order corrections, at the electroweak scale of the precision observables as included in the code FeynHiggs. Taking the CMSSM as a concrete "realistic" example, we find that the B-physics observables as well as the Higgs mass predictions do not receive sizable corrections. On the other hand, in our numerical analysis we observe that the EWPO such as the W boson mass can receive relevant corrections. Such contributions could in principle be used to place new bounds on the CMSSM parameter space. We extend our numerical analysis to the CMSSM extended with a mechanism to explain neutrino masses (CMSSMseesaw I), which induces flavor violation in the scalar lepton sector. The effects of slepton mixing on the analyzed observables are found to be, in general, smaller than those of squark mixing, but in our numerical analysis reach the level of the current experimental uncertainty for the EWPO.M. Rehman is a MulitDark Scholar. a

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Prospects for dark matter searches in the pMSSM

Roszkowski

Sessolo

Williams

2015

J. High Energ. Phys.

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We investigate the prospects for detection of neutralino dark matter in the 19-parameter phenomenological MSSM (pMSSM). We explore very wide ranges of the pMSSM parameters but pay particular attention to the higgsino-like neutralino at the ∼ 1 TeV scale, which has been shown to be a well motivated solution in many constrained supersymmetric models, as well as to a wino-dominated solution with the mass in the range of 2-3 TeV. After summarising the present bounds on the parameter space from direct and indirect detection experiments, we focus on prospects for detection of the Cherenkov Telescope Array (CTA). To this end, we derive a realistic assessment of the sensitivity of CTA to photon fluxes from dark matter annihilation by means of a binned likelihood analysis for the Einasto and Navarro-Frenk-White halo profiles. We use the most up to date instrument response functions and background simulation model provided by the CTA Collaboration. We find that, with 500 hours of observation, under the Einasto profile CTA is bound to exclude at the 95% C.L. almost all of the ∼ 1 TeV higgsino region of the pMSSM, effectively closing the window for heavy supersymmetric dark matter in many realistic models. CTA will be able to probe the vast majority of cases corresponding to a spin-independent scattering cross section below the reach of 1-tonne underground detector searches for dark matter, in fact even well below the irreducible neutrino background for direct detection. On the other hand, many points lying beyond the sensitivity of CTA will be within the reach of 1-tonne detectors, and some within collider reach. Altogether, CTA will provide a highly sensitive way of searching for dark matter that will be partially overlapping and partially complementary with 1-tonne detector and collider searches, thus being instrumental to effectively explore the nearly full parameter space of the pMSSM.

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The NUHM2 after LHC Run 1

Cited by 27 publications

References 0 publications

SUSY Fits and their Implications for ILC and CLIC

SUSY Fits and their Implications for ILC and CLIC

Effects of sfermion mixing induced by RGE running in the minimal flavor violating CMSSM

Prospects for dark matter searches in the pMSSM

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