161 research outputs found

    Fast Neutrino Decay in the Minimal Seesaw Model

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    Neutrino decay in the minimal seesaw model containing three right handed neutrinos and a complex SU(2)×U(1)SU(2)\times U(1) singlet Higgs in addition to the standard model fields is considered. A global horizontal symmetry U(1)HU(1)_H is imposed, which on spontaneous breaking gives rise to a Goldstone boson. This symmetry is chosen in a way that makes a) the contribution of heavy (\leq MeV) majorana neutrinos to the neutrinoless double beta decay amplitude vanish and b) allows the heavy neutrino to decay to a lighter neutrino and the Goldstone boson. It is shown that this decay can occur at a rate much faster than in the original Majoron model even if one does not introduce any additional Higgs fields as is done in the literature. Possibility of describing the 17 keV neutrino in this minimal seesaw model is investigated. While most of the cosmological and astrophysical constraints on the 17 keV neutrino can be satisfied in this model, the laboratory limits coming from the neutrino oscillations cannot be easily met. An extension which removes this inadequacy and offers a consistent description of the 17 keV neutrino is discussed.Comment: 16 pages, PRL-TH/92-1

    Radiatively Generated νe\nu_e Oscillations: General Analysis, Textures and Models

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    We study the consequences of assuming that the mass scale Δodot\Delta_{odot} corresponding to the solar neutrino oscillations and mixing angle Ue3U_{e3} corresponding to the electron neutrino oscillation at CHOOZ are radiatively generated through the standard electroweak gauge interactions. All the leptonic mass matrices having zero Δodot\Delta_{odot} and Ue3U_{e3} at a high scale lead to a unique low energy value for the Δodot\Delta_{odot} which is determined by the (known) size of the radiative corrections, solar and the atmospheric mixing angle and the Majorana mass of the neutrino observed in neutrinoless double beta decay. This prediction leads to the following consequences: (ii) The MSSM radiative corrections generate only the dark side of the solar neutrino solutions. (iiii) The inverted mass hierarchy (m,m,0m,-m,0) at the high scale fails in generating the LMA solution but it can lead to the LOW or vacuum solutions. (iiiiii) The Δodot\Delta_{odot} generated in models with maximal solar mixing at a high scale is zero to the lowest order in the radiative parameter. It tends to get suppressed as a result of this and lies in the vacuum region. We discuss specific textures which can lead to the LMA solution in the present framework and provide a gauge theoretical realization of this in the context of the seesaw model.Comment: 19 pages, LATE

    Fermion Dipole Moments in Supersymmetric Models with Explicitly Broken R-parity

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    We present a simple analysis that allows us to extract the leading mass dependence of the dipole moment of matter fermions that might be induced by new physics. We present explicit results for the supersymmetric model with broken R-parity as an illustration. We show that the extra contributions to the electric dipole moment (edm) of fermions from R-parity violating interactions can occur only at two loop level, contrary to claims in the literature. We further find that unlike the generic lepto-quark models, the extra contributions to the dipole moments of the leptons can only be enhanced by m_b/m_l and not by m_t/m_l relative to the expectations in the Standard Model. An interesting feature about this enhancement of these dipole moments is that it does not involve unknown mixing angles. We then use experimental constraints on the electric dipole moments of electron and neutron to obtain bounds on (the imaginary part of) products of R-parity violating couplings, and show that bounds claimed in the literature are too stringent by many orders of magnitude.Comment: 16 pages latex, 7 figure

    T-odd correlations from CP violating anomalous top-quark couplings revisited

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    We revisit the effect of CP violating anomalous top-quark couplings in ttˉt\bar{t} production and decay. We consider ttˉt\bar{t} production through gluon fusion (and light qqˉq{\bar q} annihilation) followed by top-quark decay into bWbW or bνb\ell\nu. We find explicit analytic expressions for all the triple products generated by the anomalous couplings that fully incorporate all spin correlations. Our results serve as a starting point for numerical simulations for the LHC.Comment: minor typos correcte

    Vacuum solutions of neutrino anomalies through a softly broken U (1) symmetry

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    We discuss an extended SU(2)×U(1) model which naturally leads to mass scales and mixing angles relevant for understanding both the solar and atmospheric neutrino anomalies in terms of the vacuum oscillations of the three known neutrinos. The model uses a softly broken Le-Lμ-Lτ symmetry and contains a heavy scale MH ~1015 GeV. The Le-Lμ-Lτ symmetric neutrino masses solve the atmospheric neutrino anomaly while breaking of Le-Lμ-Lτ generates highly suppressed radiative mass scale ΔS ~10−10 eV2 needed for the vacuum solution of the solar neutrino problem. All the neutrino masses in the model are inversely related to MH, thus providing seesaw-type of masses without invoking any heavy right-handed neutrinos. Possible embedding of the model into an SU(5) grand unified theory is discussed

    γγ\gamma \gamma Processes at High Energy pp Colliders

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    In this note we investigate the production of charged heavy particles via \gaga\ fusion at high energy pp colliders. We revise previous claims that the \gaga\ cross section is comparable to or larger than that for the corresponding Drell-Yan process at high energies. Indeed we find that the \gaga\ contribution to the total production cross section at pp is far below the Drell-Yan cross section. As far as the individual elastic, semi-elastic and inelastic contributions to the \gaga\ process are concerned we find that they are all of the same order of magnitude.Comment: REVTEX, 12 pages, two uuencoded figures appended at the end of the fil

    Lepton distribution as a probe of new physics in production and decay of the t quark and its polarization

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    We investigate the possibilities of studying new physics in various processes of t-quark production using kinematical distributions of the secondary lepton coming from decay of t quarks. We show that the angular distributions of the secondary lepton are insensitive to the anomalous tbW vertex and hence are pure probes of new physics in a generic process of t-quark production. The energy distribution of the lepton is distinctly affected by anomalous tbW couplings and can be used to analyze them independent of the production process of t quarks. The effects of t polarization on the distributions of the decay lepton are demonstrated for top-pair production process at a gamma-gamma collider mediated by a heavy Higgs boson.Comment: 15 pages, 7 figures, uses axodraw.sty (included), references added. v3 to appear in Journal of High Energy Physics. Incorporates minor changes in the discussion on radiative corrections which do not affect the results. Typo in reference correcte
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