Proceedings of 11th International Workshop Dark Side of the Universe 2015 — PoS(DSU2015) 2016
DOI: 10.22323/1.268.0034
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Searching for SUSY and decaying gravitino dark matter at the LHC and Fermi-LAT with the $\mu\nu$SSM

Abstract: The 'µ from ν' supersymmetric standard model (µνSSM) solves the µ problem of supersymmetric models and reproduces neutrino data, simply using couplings with the three families of right-handed neutrinos ν's. Novel signatures of supersymmetry at the LHC are expected through these new states, and couplings breaking R parity. All supersymmetric particles are potential candidates for the lightest one, which is not stable leading to prompt of displaced vertices and producing final states with multi-leptons/taus/jets… Show more

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Cited by 8 publications
(13 citation statements)
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“…(12)- (15) and the CP-even and CP-odd mass matrix elements in Eqs. (16) and (17). The following parameters appear in the Higgs potential: …”
Section: Renormalization Of the Higgs Potential At One-loopmentioning
confidence: 99%
See 2 more Smart Citations
“…(12)- (15) and the CP-even and CP-odd mass matrix elements in Eqs. (16) and (17). The following parameters appear in the Higgs potential: …”
Section: Renormalization Of the Higgs Potential At One-loopmentioning
confidence: 99%
“…Since the singlet of the NMSSM and the right-handed sneutrino of the μνSSM are both gauge-singlets, they share very similar properties. However, the explanation of the excesses in the μνSSM avoids bounds from direct detection experiments, because R-parity is broken in the μνSSM and the dark matter candidate is not a neutralino as in the NMSSM but a gravitino with a lifetime longer than the age of the universe [16]. This is important because the direct detection measurements were shown to be very constraining in the NMSSM while trying to explain the dark matter abundance on top of the excesses from LEP and CMS [114].…”
Section: The μνSsm and The Cms γ γ Excess At 96 Gevmentioning
confidence: 99%
See 1 more Smart Citation
“…For example, in the next-to-minimal supersymmetric standard model (NMSSM) [26] one extra singlet superfieldN is included in order to solve the µ problem [27]. In the µνSSM [23,28], the µ problem is solved using three families of right-handed neutrino superfieldsν c L , simultaneously reproducing at the tree level the correct neutrino physics [23,[29][30][31][32][33][34]. In this model, since R-parity is explicitly violated, all fields with the same quantum numbers mix together, and in particular the Higgses H u and H d turn out to be mixed with the right and left sneutrinos, ν R and ν L , although the mixing with the left ones is very small and they are basically decoupled.…”
Section: Jhep06(2017)095mentioning
confidence: 99%
“…As a result of the heavy mixing occurring within the neutral and charged sectors, the µνSSM presents a very rich phenomenology, markedly different from the usual collider scenarios [20][21][22][23][24][25][26]. This means not only that new parameter regions open up for SUSY searches but also that the µνSSM model predictions could have escaped unnoticed so far.…”
Section: Introductionmentioning
confidence: 99%