14,185 research outputs found

    Differential Input from the Amygdaloid Body to the Ventromedial Hypothalamic Nucleus in the Rat

    Get PDF
    Differential amygdaloid afferents to anterior dorsal, anterior ventral, posterior dorsal and posterior ventral subdivisions of the ventromedial hypothalamic nucleus (VMH) were studied by means of retrograde transport of horseradish peroxidase (HRP). Injections of tracer confined to the VMH subdivisions mentioned, and enhancement of tracer uptake and transport were achieved by iontophoretic delivery of an HRP solution containing poly-L-α-ornithine. It was shown that the medial, central, basolateral, basomedial, lateroposterior and intercalated nuclei of the amygdala constitute afferent input sources to the ventromedial nucleus in a topographic pattern related to the various subdivisions of the VMH. This topographically organized amygdala-VMH projection is discussed against the background of the functional role that both amygdala and VMH play in the control of feeding, apart from various other autonomous functions that both brain centers are known to be concerned with.

    Biquadratic antisymmetric exchange and the magnetic phase diagram of magnetoelectric CuFeO2_2

    Full text link
    Biquadratic {\it antisymmetric} exchange terms of the form −[Cijeijα(si×sj)z]2 - [C_{ij} e^{\alpha}_{ij}({\bf s}_i\times{\bf s}_j)_z]^2, where eij{\bf e}_{ij} is the unit vector connecting sites ii and jj and α=x,y\alpha = x,y, due partially to magnetoelectric coupling effects, are shown to be responsible for the spin-flop helical phase in CuFeO2_2 at low magnetic field and temperature. Usual biquadratic {\it symmetric} exchange, likely due to magnetoelastic coupling, is found to support the stability of axial magnetic states at higher fields in this nearly-Heisenberg like stacked triangular antiferromagnet. A model Hamiltonian which also includes substantial interplane and higher-neighbor intraplane exchange interactions, reproduces the unique series of observed commensurate and incommensurate periodicity phases with increasing applied magnetic field in this highly frustrated system. The magnetic field-temperature phase diagram is discussed in terms of a Landau-type free energy.Comment: 7 pages, 9 figure

    Leptogenesis with Almost Degenerate Majorana Neutrinos

    Full text link
    We investigate the leptogenesis with almost degenerate neutrinos, in the framework of democratic mass matrix, which naturally explains the large mixing angles for neutrino oscillations as well as quark masses and mixing matrix. We find that the baryon asymmetry in the present universe is explained via the decays of right-handed neutrinos produced nonthermally by the inflaton decay. The model predicts neutrinoless double beta decays accessible in near future experiments.Comment: 17 pages, LaTeX, 2 figure

    Lepton Flavor Violation in Supersymmetric SO(10) Grand Unified Models

    Get PDF
    The study for lepton flavor violation combined with the neutrino oscillation may provide more information about the lepton flavor structure of the grand unified theory. In this paper, we study two lepton flavor violation processes, τ→μγ\tau\to \mu\gamma and Z→τμZ\to \tau\mu, in the context of supersymmetric SO(10) grand unified models. We find the two processes are both of phenomenological interest. In particular the latter may be important in some supersymmetric parameter space where the former is suppressed. Thus, Z-dacay may offer another chance for looking for lepton flavor violation.Comment: 26 pages, 10 figure

    Lepton-nucleus scattering in the impulse approximation regime

    Full text link
    We discuss theoretical calculations of electron- and neutrino-nucleus scattering, carried out using realistic nuclear spectral functions and including the effect of final state interactions. Comparison between electron scattering data and the calculated inclusive cross sections off oxygen shows that the Fermi gas model fails to provide a satisfactory description of the measured cross sections, and inclusion of nuclear dynamics is needed. The role of Pauli blocking in charged-current neutrino induced reactions at low Q2Q^2 is also analyzed.Comment: To be published in the Proceedings of NUFACT05 (Nucl. Phys. B, Proceedings Supplements

    Dynamical mass generation by source inversion: Calculating the mass gap of the Gross-Neveu model

    Get PDF
    We probe the U(N) Gross-Neveu model with a source-term JΨˉΨJ\bar{\Psi}\Psi. We find an expression for the renormalization scheme and scale invariant source J^\hat{J}, as a function of the generated mass gap. The expansion of this function is organized in such a way that all scheme and scale dependence is reduced to one single parameter d. We get a non-perturbative mass gap as the solution of J^=0\hat{J}=0. In one loop we find that any physical choice for d gives good results for high values of N. In two loops we can determine d self-consistently by the principle of minimal sensitivity and find remarkably accurate results for N>2.Comment: 13 pages, 3 figures, added referenc

    Nearly Bi-Maximal Neutrino Mixing, Muon g-2 Anomaly and Lepton-Flavor-Violating Processes

    Get PDF
    We interpret the newly observed muon g-2 anomaly in the framework of a leptonic Higgs doublet model with nearly degenerate neutrino masses and nearly bi-maximal neutrino mixing. Useful constraints are obtained on the rates of lepton-flavor-violating rare decays τ→μγ\tau \to \mu \gamma, μ→eγ\mu \to e \gamma and τ→eγ\tau \to e \gamma as well as the μ\mu-ee conversion ratio RμeR_{\mu e}. We find that Γ(μ→eγ)\Gamma (\mu \to e \gamma), Γ(τ→eγ)\Gamma (\tau \to e \gamma) and RμeR_{\mu e} depend crucially on possible non-zero but samll values of the neutrino mixing matrix element Ve3V_{e3}, and they are also sensitive to the Dirac-type CP-violating phase. In particular, we show that Γ(τ→μγ)/mτ5\Gamma (\tau \to \mu \gamma)/m^5_\tau, Γ(μ→eγ)/mμ5\Gamma (\mu \to e \gamma)/m^5_\mu and Γ(τ→eγ)/mτ5\Gamma (\tau \to e \gamma)/m^5_\tau are approximately in the ratio 1:2∣Ve3∣2:2∣Ve3∣21: 2|V_{e3}|^2: 2|V_{e3}|^2 if ∣Ve3∣|V_{e3}| is much larger than O(10−2){\cal O}(10^{-2}), and in the ratio 2(Δmatm2)2:(Δmsun2)2:(Δmsun2)22 (\Delta m^2_{\rm atm})^2: (\Delta m^2_{\rm sun})^2:(\Delta m^2_{\rm sun})^2 if ∣Ve3∣|V_{e3}| is much lower than O(10−3){\cal O}(10^{-3}), where Δmatm2\Delta m^2_{\rm atm} and Δmsun2\Delta m^2_{\rm sun} are the corresponding mass-squared differences of atmospheric and solar neutrino oscillations.Comment: LaTex 6 pages (2 PS figures). Phys. Rev. D (in printing
    • …
    corecore