3,179 research outputs found

    Energy-Scale Dependence of the Lepton-Flavor-Mixing Matrix

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    We study an energy-scale dependence of the lepton-flavor-mixing matrix in the minimal supersymmetric standard model with the effective dimension-five operators which give the masses of neutrinos. We analyze the renormalization group equations of kappa_{ij}s which are coefficients of these effective operators under the approximation to neglect the corrections of O(\kappa^2). As a consequence, we find that all phases in κ\kappa do not depend on the energy-scale, and that only n_g-1 (n_g: generation number) real independent parameters in the lepton-flavor-mixing matrix depend on the energy-scale.Comment: 6 pages, no figur

    The effect of Majorana phase in degenerate neutrinos

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    There are physical Majorana phases in the lepton flavor mixing matrix when neutrinos are Majorana fermions. In the case of two degenerate neutrinos, the physical Majorana phase plays the crucial role for the stability of the maximal flavor mixing between the second and the third generations against quantum corrections. The physical Majorana phase of π\pi guarantees the maximal mixing to be stable against quantum corrections, while the Majorana phase of zero lets the maximal mixing be spoiled by quantum corrections when neutrino masses are of O(eV). The continuous change of the Majorana phase from π\pi to 0 makes the maximal mixing be spoiled by quantum corrections with O(eV) degenerate neutrino masses. On the other hand, when there is the large mass hierarchy between neutrinos, the maximal flavor mixing is not spoiled by quantum corrections independently of the Majorana phase.Comment: 7 pages, 1 figures, LaTe

    Did Mesosiderites See the FU Orionis Outbursts of the Solar Nebula?

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    第3回極域科学シンポジウム/第35回南極隕石シンポジウム 11月29日(木) 国立国語研究所 2階講

    How Do Nonlinear Voids Affect Light Propagation ?

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    Propagation of light in a clumpy universe is examined. As an inhomogeneous matter distribution, we take a spherical void surrounded by a dust shell where the ``lost mass'' in the void is compensated by the shell. We study how the angular-diameter distance behaves when such a structure exists. The angular-diameter distance is calculated by integrating the Raychaudhuri equation including the shear. An explicit expression for the junction condition for the massive thin shell is calculated. We apply these results to a dust shell embedded in a Friedmann universe and determine how the distance-redshift relation is modified compared with that in the purely Friedmann universe. We also study the distribution of distances in a universe filled with voids. We show that the void-filled universe gives a larger distance than the FRW universe by 5\sim 5% at z1z \sim 1 if the size of the void is 5\sim 5% of the Horizon radius.Comment: To appear in Prog. Theor. Phys. 10

    Origin of metal in mesosiderites.

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    第2回極域科学シンポジウム/第34回南極隕石シンポジウム 11月18日(金) 国立国語研究所 2階講

    Validation of CFD Codes for the Helicopter Wake in Ground Effect

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    When a helicopter takes off, lands, or makes hovering or taxiing flights in ground effect, its downwash interferes with the ground. Encounters with such highly turbulent helicopter wakes have been blamed for two fixed-wing aircraft crashes in the United Kingdom. Additional incidents including tents blown away are reported in Japan. Due to these accidents, the Japan Aerospace Exploration Agency (JAXA) and the University of Glasgow (UoG) are investigating the helicopter wake structure in ground effect, especially during taxiing, by means of computational fluid dynamics (CFD). In this study, CFD codes of UoG and JAXA are validated through comparing numerical results of each party and flight experiment data. As a result, it is found that the CFD codes show qualitatively the same results each other and they are also close to the experiment

    The Effect of Operating Method and Configuration of Soil Trench System on NH3-N and NO3-N Nitrogen Removal: Computer Simulation Results

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    Rosana G. Moreira, Editor-in-Chief; Texas A&M UniversityThis is a paper from International Commission of Agricultural Engineering (CIGR, Commission Internationale du Genie Rural) E-Journal Volume 8 (2006): The Effect of Operating Method and Configuration of Soil Trench System on NH3-N and NO3-N Nitrogen Removal: Computer Simulation Results. Manuscript LW 05 009. Vol. VIII. April, 2006

    Metal-nonmetal transition in LixCoO2 thin film and thermopower enhancement at high Li concentration

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    We investigate the transport properties of LixCoO2 thin films whose resistivities are nearly an order of magnitude lower than those of the bulk polycrystals. A metal-nonmetal transition occurs at ~0.8 in a biphasic domain, and the Seebeck coefficient (S) is drastically increased at ~140 K (= T*) with increasing the Li concentration to show a peak of magnitude ~120 \muV/K in the S-T curve of x = 0.87. We show that T* corresponds to a crossover temperature in the conduction, most likely reflecting the correlation-induced temperature dependence in the low-energy excitations

    Induction of inflorescence by CCC application on primary shoots of grapevines

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    Repeated CCC application at 500 ppm under the conditions of extended lang days and lower temperature of about 20 °C specifically induced inflorescences in place of tendrils on extending primary shoots of young graftings or cuttings of Muscat of Alexandria grapes.Inflorescence formation in the winter buds was much greater at 30 °C than at 20 °C along the whole shoot. CCC application increased inflorescence formation remarkably at either temperature, the effect being more pronounced at 20 °C.Die Induktion von Infloreszenzen durch Behandlung der Haupttriebe von Reben mit CCCJunge Pfropfreben oder Stecklinge der Sorte Muskat von Alexandria, deren Haupttriebe sich im Streekungswachstum befanden, wurden wiederholt mit 500 ppm CCC behandelt. Hierdurch wurden im ausgedehnten Langtag und in einem niedrigeren Temperaturbereich (ca. 20 °C) anstelle von Ranken speziell Infloreszenzen induziert. Längs des ganzen Triebes wurden in den Winterknospen bei 30 °C (ohne CCC-Behandlung) viel mehr Infloreszenzen angelegt als bei 20 °C. Durch CCC wurde die Infloreszenzbildung in beiden Temperaturbereichen beträchtlich gefördert, wobei für 20 °C eine auffälligere Wirkung festzustellen war
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