107 research outputs found

    An Improved Supersymmetric SU(5)

    Get PDF
    By supplementing minimal supersymmetric SU(5) (MSSU(5)) with a flavor U(1){\cal U}(1) symmetry and two pairs of 15ˉ+15\bar{15}+15 `matter' supermultiplets, we present an improved model which explains the charged fermion mass hierarchies and the magnitudes of the CKM matrix elements, while avoiding the undesirable asymptotic mass relations ms=mμ,md/ms=me/mμm_s=m_{\mu}, m_d/m_s = m_e/m_{\mu}. The strong coupling αs(MZ)\alpha_s (M_Z) is predicted to be approximately 0.115, and the proton lifetime is estimated to be about five times larger than the MSSU(5) value. The atmospheric and solar neutrino puzzles are respectively resolved via maximal νμντ\nu_{\mu}-\nu_{\tau} and small mixing angle νeνs\nu_e-\nu_s MSW oscillations, where νs\nu_s denotes a sterile neutrino. The U(1){\cal U}(1) symmetry ensures not only a light νs\nu_s but also automatic `matter' parity.Comment: 11 pp. LATEX. Version with minor addition accepted for publication in Physics Letters

    Neutrino Mixing and the Pattern of Supersymmetry Breaking

    Get PDF
    We study the implications of a large νμντ\nu_\mu - \nu_\tau mixing angle on lepton flavour violating radiative transitions in supersymmetric extensions of the standard model. The transition rates are calculated to leading order in ϵ\epsilon, the parameter which characterizes the flavour mixing. The uncertainty of the predicted rates is discussed in detail. For models with modular invariance the branching ratio BR(μeγ)BR(\mu \to e \gamma) mostly exceeds the experimental upper limit. In models with radiatively induced flavour mixing the predicted range includes the upper limit, if the Yukawa couplings in the lepton sector are large, as favoured by Yukawa coupling unification.Comment: 12 pages, 2 figures, used axodraw.sty, to be published in Physics Letters

    Reentrant violation of special relativity in the low-energy corner

    Get PDF
    In the effective relativistic quantum field theories the energy region, where the special relativity holds, can be sandwiched from both the high and low energies sides by domains where the special relativity is violated. An example is provided by 3He-A where the relativistic quantum field theory emerges as the effective theory. The reentrant violation of the special relativity in the ultralow energy corner is accompanied by the redistribution of the momentum-space topological charges between the fermionic flavors. At this ultralow energy an exotic massless fermion with the topological charge N3=2N_3=2 arises, whose energy spectrum mixes the classical and relativistic behavior. This effect can lead to neutrino oscillations if neutrino flavors are still massless at this energy scale.Comment: RevTeX file, 5 pages, one figure, submitted to JETP Let

    Bethe-Salpeter Approach for Meson-Meson Scattering in Chiral Perturbation Theory

    Get PDF
    The Bethe-Salpeter equation restores exact elastic unitarity in the s- channel by summing up an infinite set of chiral loops. We use this equation to show how a chiral expansion can be undertaken by successive approximations to the potential which should be iterated. Renormalizability of the amplitudes in a broad sense can be achieved by allowing for an infinite set of counter-terms as it is the case in ordinary Chiral Perturbation Theory. Within this framework we calculate the ππ\pi \pi scattering amplitudes both for s- and p-waves at lowest order in the proposed expansion where a successful description of the low-lying resonances (σ\sigma and ρ\rho) and threshold parameters is obtained. We also extract the SU(2) low energy parameters lˉ1,2,3,4{\bar l}_{1,2,3,4} from our amplitudes.Comment: 11 pages, final version submitted to PL

    Infrared Fixed Points and Fixed Lines in the Top-Bottom-Tau Sector in Supersymmetric Grand Unification

    Get PDF
    The two-loop ``top-down'' renormalization group flow for the top, bottom and tau Yukawa couplings is explored in the framework of supersymmetric grand unification; reproduction of the physical bottom and tau masses is required. Instead of following the recent trend of implementing exact Yukawa coupling unification i) a search for infrared (IR) fixed lines and fixed points in the m(top)-tan(beta) plane is performed and ii) the extent to which these imply approximate Yukawa unification is determined. Two IR fixed lines, intersecting in an IR fixed point, are located. The more attractive fixed line has a branch of almost constant top mass, 168-180 GeV, close to the experimental value, for the large interval 2.5<tan(beta)<55; it realizes tau-bottom Yukawa unification at MGUT approximately. The fixed point at m(top)= 170 GeV, tan(beta)=55 implements approximate top-bottom Yukawa unification at all scales. The fixed point and lines are distinct from the much quoted effective IR fixed point m(top)=O(200)GeV sin(beta).Comment: 12 pages, latex, epsfig, 3 figure

    A Mechanism for Baryogenesis in Low Energy Supersymmetry Breaking Models

    Get PDF
    A generic prediction of models where supersymmetry is broken at scales within a few orders of magnitude of the weak scale and is fed down to the observable sector by gauge interactions is the existence of superconducting cosmic strings which carry baryon number. In this paper we propose a novel mechanism for the generation of the baryon asymmetry which takes place at temperatures much lower than the weak scale. Superconducting strings act like ``bags'' containing the baryon charge and protect it from sphaleron wash-out throughout the evolution of the Universe, until baryon number violating processes become harmless. This mechanism is efficient even if the electroweak phase transition in the MSSM is of the second order and therefore does not impose any upper bound on the mass of the Higgs boson. (13kb)Comment: LaTeX file, 17 pages. One ref. adde

    Quark and Lepton Mass Patterns and the Absolute Neutrino Mass Scale

    Get PDF
    We investigate what could be learned about the absolute scale of neutrino masses from comparisons among the patterns within quark and lepton mass hierarchies. First, we observe that the existing information on neutrino masses fits quite well to the unexplained, but apparently present regularities in the quark and charged lepton sectors. Second, we discuss several possible mass patterns, pointing out that this quite generally leads towards hierarchical neutrino mass patterns especially disfavoring the vacuum solution.Comment: final version to be published in PRD, 5 pages, 2 figures, RevTe

    Where to look for solving the gauge hierarchy problem?

    Get PDF
    A mass of the Higgs boson close to 126 GeV may give a hint that the standard model of particle physics is valid up to the Planck scale. We discuss perspectives for the solution of the gauge hierarchy problem at high scales. Scenarios with an ultraviolet fixed point have predicted a Higgs boson mass very close to 126 GeV if the fixed point value of the quartic scalar coupling is small. In this case the top quark pole mass should be close to 172 GeV.Comment: additional references, somewhat extended discussion, 5 page

    A Model for Neutrino Warm Dark Matter and Neutrino Oscillations

    Get PDF
    The muon- and tau-neutrinos with the mass in the keV range, which are allowed in a low reheating temperature cosmology, can compose the warm dark matter of the universe. A model of four light neutrinos including the keV scale νμ\nu_\mu and ντ\nu_\tau is studied, which combines the seesaw mechanism and the Abelian flavor symmetry. The atmospheric neutrino anomaly is due to the νμντ\nu_\mu-\nu_\tau oscillation. The solar neutrino problem is answered by the oscillation into the light sterile neutrino, where the SMA, LMA, and LOW-QVO solutions can be accommodated in our scenario.Comment: 11 pages, Final version to appear in PLB, References adde
    corecore