52 research outputs found

    SU(3)FSU(3)_{F} Gauge Family Model and New Symmetry Breaking Scale From FCNC Processes

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    Based on the SU(3)FSU(3)_{F} gauge family symmetry model which was proposed to explain the observed mass and mixing pattern of neutrinos, we investigate the symmetry breaking, the mixing pattern in quark and lepton sectors, and the contribution of the new gauge bosons to some flavour changing neutral currents (FCNC) processes at low energy. With the current data of the mass differences in the neutral pseudo-scalar P0−Pˉ0P^{0}-\bar{P}^{0} systems, we find that the SU(3)FSU(3)_{F} symmetry breaking scale can be as low as 300TeV and the mass of the lightest gauge boson be about 100100TeV. Other FCNC processes, such as the lepton flavour number violation process μ−→e−e+e−\mu^{-}\rightarrow e^{-}e^{+}e^{-} and the semi-leptonic rare decay K→πνˉνK\rightarrow \pi \bar{\nu} \nu, contain contributions via the new gauge bosons exchanging. With the constrains got from P0−Pˉ0P^0-\bar{P}^0 system, we estimate that the contribution of the new physics is around 10−1610^{-16}, far below the current experimental bounds.Comment: 3figure

    Fourth generation Majorana neutrino, dark matter and Higgs physics

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    We consider extensions of the standard model with fourth generation fermions (SM4) in which extra symmetries are introduced such that the transitions between the fourth generation fermions and the ones in the first three generations are forbidden. In these models, the stringent lower bounds on the masses of fourth generation quarks from direct searches are relaxed, and the lightest fourth neutrino is allowed to be stable and light enough to trigger the Higgs boson invisible decay. In addition, the fourth Majorana neutrino can be a subdominant but highly detectable dark matter component. We perform a global analysis of the current LHC data on the Higgs production and decay in this type of SM4. The results show that the mass of the lightest fourth Majorana neutrino is confined in the range ∼41−59\sim 41-59 GeV. Within the allowed parameter space, the predicted effective cross-section for spin-independent DM-nucleus scattering is ∼3×10−48−6×10−46cm2\sim 3\times 10^{-48}-6\times 10^{-46} \text{cm}^{2}, which is close to the current Xenon100 upper limit and is within the reach of the Xenon1T experiment in the near future. The predicted spin-dependent cross sections can also reach ∼8×10−40cm2\sim 8\times 10^{-40}\text{cm}^{2}.Comment: arXiv admin note: substantial text overlap with arXiv:1110.293

    W±H∓W^{\pm}H^{\mp} associated production at LHC in the general 2HDM with Spontaneous CP Violation

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    Spontaneous CP violation motivates the introduction of two Higgs doublets in the electroweak theory. Such a simple extension of the standard model has three neutral Higgs bosons and a pair charged Higgs, especially it leads to rich CP-violating sources including the induced Kobayashi-Maskawa CP-violating phase, the mixing of the neutral Higgs bosons due to the CP-odd Higgs and the effective complex Yukawa couplings of the charged and neutral Higgs bosons. Within this model, we present the production of a charged Higgs boson in association with a W boson at the LHC, and calculate in detail the cross section and the transverse momentum distribution of the associated W boson.Comment: 16 pages, 6 figures, omitted 3 figures, motivations for Type III 2HDM with SCPV is emphasized, to be published in PR

    Probing WL′WHW^\prime_L WH and WR′WHW^\prime_R W H Interaction at LHC

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    Many new physics models predict the existence of TeV-scale charged gauge boson W′W^\prime together with Higgs boson(s). We study the W′WHW^\prime WH interaction and explore the angular distribution of charged lepton to distinguish WR′WHW_R^\prime WH from WL′WHW_L^\prime WH in pp→HW→bbˉlνpp\to HW\to b \bar b l \nu process at the LHC. It is found that a new type forward-backward asymmetry(AFBA_{FB}) relating to the angle between the direction of the charged lepton in WW rest frame and that of the reconstructed W′W^\prime in laboratory frame is useful to investigate the properties of W′WHW^\prime W H interaction. We analyze the Standard Model backgrounds and develop a set of cuts to highlight the signal and suppress the backgrounds at LHC. We find that AFBA_{FB} can reach 0.03(-0.07) for WR′W_R^\prime(WL′W_L^\prime) production at S=14\sqrt{S}=14 TeV

    Improved Analytic Solution of Black Hole Superradiance

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    The approximate solution of the Klein-Gordon equation for a real scalar field of mass μ\mu in the geometry of a Kerr black hole obtained by Detweiler \cite{Detweiler:1980uk} is widely used in the analysis of the stability of black holes as well as the search of axion-like particles. In this work, we confirm a missing factor 1/21/2 in this solution, which was first identified in Ref.~\cite{Pani:2012bp}. The corrected result has strange features that put questions on the power-counting strategy. We solve this problem by adding the next-to-leading order (NLO) contribution. Compared to the numerical results, the NLO solution reduces the percentage error of the LO solution by a factor of 2 for all important values of rgμr_g \mu. Especially the percentage error is ≲10%\lesssim 10\% in the region of rgμ≲0.35r_g\mu \lesssim 0.35. The NLO solution also has a compact form and could be used straightforwardly.Comment: 5 pages, 3 figures, Accepted by PR

    Next-to-leading-order solution to Kerr-Newman black hole superradiance

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    The superradiant instabilities of Kerr-Newman black holes with charged or uncharged massive spin-0 fields are calculated analytically to the next-to-leading order in the limit of α∼rgμ≪1\alpha\sim r_g \mu \ll 1. A missing factor of 1/21/2 in the previous leading-order result is identified. The next-to-leading order result has a compact form and is in good agreement with existing numerical calculations. The percentage error increases with α\alpha, from a few percent for α∼0.1\alpha\sim 0.1 to about 50%50\% for α∼0.4\alpha\sim 0.4. Massive neutral scalars too heavy to be produced with Kerr black hole superradiance may exist in the superradiant region of Kerr-Newman black holes.Comment: 11 pages, 5 figures, 2 tables. Matches Physical Review D versio

    Study Majorana Neutrino Contribution to B-meson Semi-leptonic Rare Decays

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    B meson semi-leptonic rare decays are sensitive to new physics beyond standard model. We study the B−→π−μ+μ−B^{-}\to \pi^{-}\mu^{+}\mu^{-} process and investigate the Majorana neutrino contribution to its decay width. The constraints on the Majorana neutrino mass and mixing parameter are obtained from this decay channel with the latest LHCb data. Utilizing the best fit for the parameters, we study the lepton number violating decay B−→π+μ−μ−B^{-}\to \pi^{+}\mu^{-}\mu^{-}, and find its branching ratio is about 6.4×10−106.4\times10^{-10}, which is consistent with the LHCb data reported recently.Comment: 10 pages, 3 figure

    2,4-Dihydr­oxy-N′-(3,4,5-trimethoxy­benzyl­idene)benzohydrazide

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    In the title compound, C17H18N2O6, the mol­ecule is slightly twisted, with a dihedral angle of 18.1 (2)° between the two benzene rings. In the crystal structure, mol­ecules are linked into a network by inter­molecular N—H⋯O, O—H⋯N and O—H⋯O hydrogen bonds. An intra­molecular O—H⋯O hydrogen bond is also present

    Identify Charged Higgs Boson in W±H∓W^\pm H^\mp Associated Production at LHC

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    We investigate the possibility to discover the charged Higgs via pp\to W^{\pm}H^{\mp}\to l+\met+b\bar{b}jj process at LHC, which suffers from large QCD backgrounds. We optimize the kinematic cuts to suppress the backgrounds, so that the reconstruction of the charged Higgs through hadronic decay is possible. The angular distribution of the b-jet from H±H^{\pm} decay is investigated as a way to identify the charged scalar from vector bosons
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