272 research outputs found

    Higgs Boson Mass and Complex Snuetrino Dark Matter in the Supersymmetric Inverse Seesaw Models

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    The discovery of a relatively heavy Standard Model (SM) -like Higgs boson challenges naturalness of the minimal supersymmetric standard model (MSSM) from both Higgs and dark matter (DM) sectors. We study these two aspects in the MSSM extended by the low-scale inverse seesaw mechanism. Firstly, it admits a sizable radiative correction on the Higgs boson mass m_h, up to \sim 4 GeV in the case of an IR-fixed point of the coupling Y_\nu LH_u\nu^c and a large sneutrino mixing. Secondly, the lightest sneutrino, highly complex as expected, is a viable thermal DM candidate. Owing to the correct relic density and XENON100, two cases survive: a Higgs-portal complex DM with mass lying around the Higgs pole or above WW threshold, and a coannihilating DM with slim prospect of detection. Given an extra family of sneutrinos, both scenarios naturally work when we attempt to suppress the DM left-handed sneutrino component, confronting with enhancing m_h.Comment: 19 pages, 6 figures, JHEP versio

    Realistic Type IIB Supersymmetric Minkowski Flux Vacua

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    We show that there exist supersymmetric Minkowski vacua on Type IIB toroidal orientifold with general flux compactifications where the RR tadpole cancellation conditions can be relaxed elegantly. Then we present a realistic Pati-Salam like model. At the string scale, the gauge symmetry can be broken down to the Standard Model (SM) gauge symmetry, the gauge coupling unification can be achieved naturally, and all the extra chiral exotic particles can be decoupled so that we have the supersymmetric SMs with/without SM singlet(s) below the string scale. The observed SM fermion masses and mixings can also be obtained. In addition, the unified gauge coupling, the dilaton, the complex structure moduli, the real parts of the K\"ahler moduli and the sum of the imaginary parts of the K\"ahler moduli can be determined as functions of the four-dimensional dilaton and fluxes, and can be estimated as well.Comment: RevTex4, 4 pages, 3 table

    Simplified Supersymmetry with Sneutrino LSP at 8 TeV LHC

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    The current searches of supersymmetry (SUSY) are based on the neutralino lightest sparticle (LSP). In this article we instead focus on SUSY with sneutrino LSP. It is well motivated in many contexts, especially in which sneutrino services as a dark matter candidate. We first develop a simplified model, which contains the stop, chagino/neutralino and sneutrino, to describe the LHC phenomenologies of a large class of models with sneutrino LSP. Then we investigate bounds on the model using the SUSY searches at the 8 TeV LHC. Strong exclusion limits are derived, e.g., masses of stop and chargino can be excluded up to about 900 GeV and 550 GeV, respectively. We also propose optimizations for some searches without turning to higher energy and luminosity.Comment: 26 pages, 8 figures,Minor corrections,References adde

    Light Doubly Charged Higgs Boson via the WWWW^* Channel at LHC

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    The doubly charged Higgs bosons H±±H^{\pm\pm} searches at the Large Hadron Collider (LHC) have been studied extensively and strong bound is available for H±±H^{\pm\pm} dominantly decaying into a pair of same-sign di-leptons. In this paper we point out that there is a large cavity in the light H±±H^{\pm\pm} mass region left unexcluded. In particular, H±±H^{\pm\pm} can dominantly decay into WWWW or WWWW^* (For instance, in the type-II seesaw mechanism the triplet acquires a vacuum expectation value around 1 GeV.), and then it is found that H±±H^{\pm\pm} with mass even below 2mW2m_W remains untouched by the current collider searches. Searching for such a H±±H^{\pm\pm} at the LHC is the topic of this paper. We perform detailed signal and background simulation, especially including the non-prompt ttˉt\bar{t} background which is the dominant one nevertheless ignored before. We show that such H±±H^{\pm\pm} should be observable at the 14 TeV LHC with 10-30 fb1^{-1} integrated luminosity.Comment: 23 pages, 4 figures, typos fixed, references added, EPJC versio

    Probing the CP-even Higgs Sector via H3H2H1H_3\to H_2H_1 in the Natural NMSSM

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    After the discovery of a Standard Model (SM) like Higgs boson, naturalness strongly favors the next to the Minimal Supersymmetric SM (NMSSM). In this letter, we point out that the most natural NMSSM predicts the following CP-even Higgs HiH_i sector: (A) H2H_2 is the SM-like Higgs boson with mass pushed-upward by a lighter H1H_1 with mass overwhelmingly within [mH2/2,mH2][m_{H_2}/2,m_{H_2}]; (B) mH32μ/sin2β300m_{H_3}\simeq 2\mu/\sin2\beta\gtrsim300 GeV; (C) H3H_3 has a significant coupling to top quarks and can decay to H1H2H_1H_2 with a large branching ratio. Using jet substructure we show that all the three Higgs bosons can be discovered via ggH3H1H2bbˉνjjgg\to H_3 \to H_1H_2\to b\bar b \ell\nu jj at the 14 TeV LHC. Especially, the LEP-LHC scenario with H198H_1\simeq98 GeV has a very good discovery potential.Comment: 5 pages, 2 figures. Some typos corrected and reference adde

    Standard-like Models as Type IIB Flux Vacua

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    We construct new semi-realistic Type IIB flux vacua on Z2×Z2Z_2\times Z_2 orientifolds with three- and four- Standard Model (SM) families and up to three units of quantized flux. The open-string sector is comprised of magnetized D-branes and is T-dual to supersymmetric intersecting D6-brane constructions. The SM sector contains magnetized D9-branes with negative D3-brane charge contribution. There are large classes of such models and we present explicit constructions for representative ones. In addition to models with one and two units of quantized flux, we also construct the first three- and four-family Standard-like models with supersymmetric fluxes, i.e. comprising three units of quantized flux. Supergravity fluxes are due to the self-dual NS-NS and R-R three-form field strength and they fix the toroidal complex structure moduli and the dilaton. The supersymmetry conditions for the D-brane sector fix in some models all three toroidal K\"ahler moduli. We also provide examples where toroidal K\" ahler moduli are fixed by strong gauge dynamics on the ``hidden sector'' D7-brane. Most of the models possess Higgs doublet pairs with Yukawa couplings that can generate masses for quarks and leptons. The models have (mainly right-) chiral exotics.Comment: 31 page

    Electroweak Baryogenesis, CDM and Anomaly-free Supersymmetric U(1)-prime Models

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    We construct two anomaly-free supersymmetric U(1)U(1)' models with a secluded U(1)U(1)'-breaking sector. For the one with E6E_6 embedding we show that there exists a strong enough first order electroweak phase transition for electroweak baryogenesis (EWBG) because of the large soft trilinear terms in the Higgs potential. Unlike the Minimal Supersymmetric Standard Model (MSSM), the stop masses can be very heavy. We then discuss possible CP violation in the Higgs sector, which can be both spontaneous and explicit, even at tree level. The spontaneous violation provides a direct source for baryogenesis, while its magnitude is mediated by an explicit phase from the secluded sector. These new CP sources do not introduce significant new contributions to electric dipole moments. EWBG in the thin wall (τ\tau leptons) and thick wall regimes (top squarks, charginos and top quarks) are systematically discussed. We find that the CP-violating stop and chargino currents are very different from those obtained in the MSSM. Due to the space-dependence of the relevant CP phases, they do not require a variation of tanβ\tan \beta in the bubble wall to have a non-trivial structure at the lowest order of Higgs insertion. In addition to τ\tau leptons, top squarks and charginos, we find that top quarks can also play a significant role. Numerical results show that the baryon asymmetry is large enough to explain the cosmological observation today. We illustrate that EWBG and neutralino cold dark matter can be accommodated in the same framework, i.e., there exists parameter space where a strong enough first order EWPT, large CP phase variations across the bubble wall, a reasonable baryon asymmetry as well as an acceptable neutralino dark matter relic density can be achieved simultaneously.Comment: 71 pages, 20 figure
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