1,221 research outputs found

    Direct Detection of Electroweak-Interacting Dark Matter

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    Assuming that the lightest neutral component in an SU(2)L gauge multiplet is the main ingredient of dark matter in the universe, we calculate the elastic scattering cross section of the dark matter with nucleon, which is an important quantity for the direct detection experiments. When the dark matter is a real scalar or a Majorana fermion which has only electroweak gauge interactions, the scattering with quarks and gluon are induced through one- and two-loop quantum processes, respectively, and both of them give rise to comparable contributions to the elastic scattering cross section. We evaluate all of the contributions at the leading order and find that there is an accidental cancellation among them. As a result, the spin-independent cross section is found to be O(10^-(46-48)) cm^2, which is far below the current experimental bounds.Comment: 19 pages, 7 figures, published versio

    Neutrino Oscillation and Charged Lepton-Flavor Violation in the Supersymmetric Standard Models

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    The neutrino experiment results suggest that the neutrinos have finite masses and the lepton-flavor symmetries are violating in nature. In the supersymmetric models, the charged lepton-flavor violating processes, such as mu -> e gamma and tau -> mu gamma, may have the branching ratios accessible to the future experiments, depending on origins of the neutrino masses and the SUSY breaking. In this paper we discuss the branching ratios in the supergravity scenario using the current solar and atmospheric neutrino experimental data.Comment: 12 pages. Talk given at the Workshop on High Intensity Muon Sources (HIMUS99), Tsukuba, Japan, 1-4 Dec 199

    An N=2 SUSY Gauge Model for Dynamical Breaking of the Grand Unified SU(5) Symmetry

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    We construct an extension of the recently proposed dynamical model for the breaking of SU(5)GUT_{\rm GUT} gauge symmetry, in which a pair of massless chiral supermultiplets for Higgs doublets are naturally obtained. We point out that a model at a specific point in the parameter space of superpotential is regarded as a low-energy effective theory of an N=2 supersymmetric gauge model for the strongly interacting hypercolor sector.Comment: 7 page

    Flavor and CP Violation Induced by Atmospheric Neutrino Mixing

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    Neutrino oscillation experiments suggest existence of new flavor-violating interactions in high energy scale. It may be possible to probe them by the flavor- and CP-violating processes in leptons and hadrons in the supersymmetric (SUSY) models. In this article the third-generation flavor violation is reviewed in the SUSY seesaw model and SUSY SU(5) GUT with the right-handed neutrinos.Comment: 12 pages. Talk at Fujihara Seminar on Neutrino Mass and Seesaw Mechanism (SEESAW 1979-2004), Tsukuba, Ibaraki, Japan, 23-25 Feb 200

    Probing Left-handed Slepton Flavor Mixing at Future Lepton Colliders

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    It has been argued in the literature that the search for the slepton oscillation phenomenon can be a powerful probe of intergenerational mixing between sleptons, once sleptons are found at future colliders. In this article we estimate possible reach of future lepton colliders in probing left-handed slepton flavor mixing, especially mixing between the first and third generations, on which constraints imposed by other processes like τeγ\tau \to e \gamma are very weak. e+ee^+e^- collider is suitable for this purpose, since it can produce, if kinematically allowed, sleptons of the first generation via t-channel, in addition to s-channel. Utilizing e^+e^- \to \tau e + 4jets + \E signal at e+ee^+e^- linear collider with integrated luminosity L=50 fb^{-1}(500 fb^{-1}) it may be possible to reach mixing angle sin2θν~0.06(0.04)\sin 2\theta_{\tilde{\nu}} \gtrsim 0.06 (0.04) and mass difference Δmν~0.07(0.04)\Delta m_{\tilde{\nu}} \gtrsim 0.07 (0.04) GeV for sneutrinos in the first and third generations at the statistical significance of 5 \sigma.Comment: 27 pages, 6 figures. A new section added. Conclusion unchanged. To appear in Phys. Rev.
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