2017
DOI: 10.1103/physrevd.96.015017
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DifferentiatingU(1)supersymmetric models with right sneutrino and neutralino dark matter

Abstract: We perform a detailed analysis of dark matter signals of supersymmetric models containing an extra U (1) gauge group. We investigate scenarios in which either the right sneutrino or the lightest neutralino are phenomenologically acceptable dark matter candidates and we explore the parameter spaces of different supersymmetric realisations featuring an extra U (1) . We impose consistency with low energy observables, with known mass limits for the superpartners and Z bosons, as well as with Higgs boson signal str… Show more

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Cited by 16 publications
(18 citation statements)
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References 78 publications
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“…We observe, similarly to the findings of Ref. [27], that only |θ E 6 | values in the intervals [0, π/4] and [3/4π, π] can accommodate all the imposed experimental constraints. Outside of these regions, the U (1) charge of the extra singlet supermultiplet S is in fact close to zero so that either the SM-like Higgs boson or the Z boson, or even both, are predicted to be too light with respect to current data.…”
Section: Scenarios With High-scale Boundary Conditionssupporting
confidence: 89%
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“…We observe, similarly to the findings of Ref. [27], that only |θ E 6 | values in the intervals [0, π/4] and [3/4π, π] can accommodate all the imposed experimental constraints. Outside of these regions, the U (1) charge of the extra singlet supermultiplet S is in fact close to zero so that either the SM-like Higgs boson or the Z boson, or even both, are predicted to be too light with respect to current data.…”
Section: Scenarios With High-scale Boundary Conditionssupporting
confidence: 89%
“…As discussed, e.g., in Refs. [25,27], U (1) χ models are ill-defined in supersymmetry as it they typically lead to unphysical sfermion masses after adding to the soft masses the D-term contributions. As to U (1) S , it may be theoretically acceptable, but we were not able to find scenarios capable of satisfying the constraints of Table 4.…”
Section: Scenarios With High-scale Boundary Conditionsmentioning
confidence: 99%
“…These inequations show that the ratio 33 is least constrained when λ, µ and v u (or alternatively tan β) are fixed. Besides the inputs λ, κ, µ and tan β in Higgs sector, the sneutrino sector in the ISS-NMSSM involves the parameters Y ν , λ ν , A ν , A λν , µ X , B µ X and the soft breaking masses ml, mν and mx.…”
Section: Sneutrino Sector Of the Iss-nmssmmentioning
confidence: 97%
“…The SU (2) R triplet scalar masses are allowed to be even smaller than the heaviest right-handed neutrino mass. Right-handed neutrinos could nevertheless be indirectly constrained by neutrinoless double-beta decays and cosmology [114][115][116].…”
Section: Numerical Analysis and Resultsmentioning
confidence: 99%