2,298 research outputs found

    Resonant X-Ray Scattering Measurements of a Spatial Modulation of the Cu 3d and O 2p Energies in Stripe-Ordered Cuprate Superconductors

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    A prevailing description of the stripe phase in underdoped cuprate superconductors is that the charge carriers (holes) phase segregate on a microscopic scale into hole rich and hole poor regions. We report resonant elastic x-ray scattering measurements of stripe-ordered La1.475_{1.475}Nd0.4_{0.4}Sr0.125_{0.125}CuO4_4 at the Cu LL and O KK absorption edges that identify an additional feature of stripe order. Analysis of the energy dependence of the scattering intensity reveals that the dominant signature of the stripe order is a spatial modulation in the energies of Cu 3d and O 2p states rather than the large modulation of the charge density (valence) envisioned in the common stripe paradigm. These energy shifts are interpreted as a spatial modulation of the electronic structure and may point to a valence-bond-solid interpretation of the stripe phase.Comment: 5 pages, 2 figure

    Orbital Symmetries of Charge Density Wave Order in YBa2Cu3O6+x

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    Charge density wave (CDW) order has been shown to compete and coexist with superconductivity in underdoped cuprates. Theoretical proposals for the CDW order include an unconventional dd-symmetry form factor CDW, evidence for which has emerged from measurements, including resonant soft x-ray scattering (RSXS) in YBa2_2Cu3_3O6+x_{6+x} (YBCO). Here, we revisit RSXS measurements of the CDW symmetry in YBCO, using a variation in the measurement geometry to provide enhanced sensitivity to orbital symmetry. We show that the $(0\ 0.31\ L)CDWpeakmeasuredattheCu CDW peak measured at the Cu Ledgeisdominatedbyan edge is dominated by an sformfactorratherthana form factor rather than a dformfactoraswasreportedpreviously.Inaddition,bymeasuringboth form factor as was reported previously. In addition, by measuring both (0.31\ 0\ L)and and (0\ 0.31\ L)peaks,weidentifyapronounceddifferenceintheorbitalsymmetryoftheCDWorderalongthe peaks, we identify a pronounced difference in the orbital symmetry of the CDW order along the aand and baxes,withtheCDWalongthe axes, with the CDW along the a$ axis exhibiting orbital order in addition to charge order.Comment: 17 pages, 4 figures + supplementary informatio

    The symmetry of charge order in cuprates

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    Charge-ordered ground states permeate the phenomenology of 3d-based transition metal oxides, and more generally represent a distinctive hallmark of strongly-correlated states of matter. The recent discovery of charge order in various cuprate families fueled new interest into the role played by this incipient broken symmetry within the complex phase diagram of high-Tc superconductors. Here we use resonant X-ray scattering to resolve the main characteristics of the charge-modulated state in two cuprate families: Bi2201 and YBCO. We detect no signatures of spatial modulations along the nodal direction in Bi2201, thus clarifying the inter-unit-cell momentum-structure of charge order. We also resolve the intra-unit-cell symmetry of the charge ordered state, which is revealed to be best represented by a bond-order with modulated charges on the O-2p orbitals and a prominent d-wave character. These results provide insights on the microscopic description of charge order in cuprates, and on its origin and interplay with superconductivity.Comment: A high-resolution version with supplementary material can be found at: http://www.phas.ubc.ca/~quantmat/ARPES/PUBLICATIONS/Articles/CDW_symmetry.pd

    Chaotic Amplification of Neutrino Chemical Potentials by Neutrino Oscillations in Big Bang Nucleosynthesis

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    We investigate in detail the parameter space of active-sterile neutrino oscillations that amplifies neutrino chemical potentials at the epoch of Big Bang Nucleosynthesis. We calculate the magnitude of the amplification and show evidences of chaos in the amplification process. We also discuss the implications of the neutrino chemical potential amplification in the Big Bang Nucleosynthesis. It is shown that with a 1\sim 1 eV \nue, the amplification of its chemical potential by active-sterile neutrino oscillations can lower the effective number of neutrino species at Big Bang Nucleosynthesis to significantly below 3.Comment: Revtex 20 pages, 7 postscript figures. Also by ftp://astro.queensu.ca/pub/shi/ . Submitted to PR

    Neutrino mass matrix with U(2) flavor symmetry and neutrino oscillations

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    The three neutrino mass matrices in the SU(5)×U(2)SU(5)\times U(2) model are studied focusing on the neutrino oscillation experiments. The atmospheric neutrino anomaly could be explained by the large νμντ\nu_{\mu} - \nu_{\tau} oscillation. The long baseline experiments are expected to detect signatures of the neutrino oscillation even if the atmospheric neutrino anomaly is not due to the neutrino oscillation. However, the model cannot solve the solar neutrino deficit while it could be reconciled with the LSND data.Comment: 12 pages, LaTex file, to be published in PR

    Is CP Violation Observable in Long Baseline Neutrino Oscillation Experiments ?

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    We have studied CP violation originated by the phase of the neutrino mixing matrix in the long baseline neutrino oscillation experiments. The direct measurements of CP violation is the difference of the transition probabilities between CP-conjugate channels. In those experiments, the CP violating effect is not suppressed if the highest neutrino mass scale is taken to be 1\sim 5 \eV, which is appropriate for the cosmological hot dark matter. Assuming the hierarchy for the neutrino masses, the upper bounds of CP violation have been caluculated for three cases, in which mixings are constrained by the recent short baseline ones. The calculated upper bounds are larger than 10210^{-2}, which will be observable in the long baseline accelerator experiments. The matter effect, which is not CP invariant, has been also estimated in those experiments.Comment: 28 pages, LaTex file, 6 figures included using epsfig Matter effect is estimated(Figs.3(a) (b)). Physical parameters are change

    Sensitivity of the Immunohistochemistry technique in central nervous system fragments of cattle and horses naturally infected by rabies virus

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    A raiva é uma zoonose viral que acomete o sistema nervoso central (SNC) de mamíferos, considerada um grave problema de saúde pública. Herbívoros (bovinos e equinos) são frequentemente acometidos pela in-fecção após serem atacados por morcegos hematófagos (Desmodus rotundus). A técnica de imunofluorescência direta (IFD) realizada em tecidos frescos, recomendada pela Organização Mundial de Saúde (OMS), é utilizada para o diagnóstico da raiva. A técnica de imuno-histoquímica (IHQ) é utilizada para detectar antígenos em tecidos fixados, pelo uso de anticorpos monoclonais/policlonais. O objetivo deste trabalho foi avaliar a sensibilidade da IHQ na detecção de antígenos do vírus da raiva em amostras de SNC de herbívoros fixadas em formol, analisando a distribuição antigênica em diferentes fragmentos do SNC. Os resultados demonstraram concordância das técnicas de IFD e IHQ. A IHQ mostrou maior sensibilidade em amostras de bovinos em relação às de equinos, especialmente quando realizada em fragmentos de cerebelo e tronco encefálico. A detecção de antígeno nestes fragmentos foi mais consistente para ambas as técnicas, nas duas espécies. Estes resultados demonstram que a IHQ pode ser empregada para a vigilância epidemiológica da raiva, entretanto, recomenda-se cautela ao se empregar a IHQ para diagnóstico de doença em herbívoros, especialmente quando o fragmento encaminhado ao laboratório for apenas o hipocampo.Rabies is a viral zoonosis that causes disease in the central nervous system (CNS) of mammals and it is considered a serious problem of public health. Herbivorous (bovines and equines) are often infected after being attacked by vampire bats (Desmodus rotundus). The direct fluorescent antibody technique is used as a diagnostic test to detect viral antigens in fresh tissues and is recommended by the World Health Organization. The immunohistochemistry technique (IHC) is used to detect the viral antigen through the use of monoclonal/policlonal antibodies in formalin-fixed tissues. The aim of this work was to evaluate the sensitivity of the IHC in samples of CNS of herbivorous fixed in formol, analyzing the antigenic distribution in different fragments of the CNS. The results demonstrated good agreement between the two techniques for the rabies diagnosis. The IHC presented higher sensitivity in samples of cattle comparing to horse samples, especially in fragments of cerebellum and brain stem. These fragments demonstrated to be more suitable for antigen detection by both techniques in the two species. These data demonstrate that the IHC is suitable for rabies vigilance yet cautions should be taken in examining cattle and horses samples, when the submitted specimen is only the hippocampus

    Effects of neutrino oscillations and neutrino magnetic moments on elastic neutrino-electron scattering

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    We consider elastic antineutrino-electron scattering taking into account possible effects of neutrino masses and mixing and of neutrino magnetic moments and electric dipole moments. Having in mind antineutrinos produced in a nuclear reactor we compute, in particular, the weak-electromagnetic interference terms which are linear in the magnetic (electric dipole) moments and also in the neutrino masses. We show that these terms are, however, suppressed compared to the pure weak and electromagnetic cross section. We also comment upon the possibility of using the electromagnetic cross section to investigate neutrino oscillations.Comment: 12 pages, REVTEX file, no figures, submitted to Phys.Rev.

    Final results from the Palo Verde Neutrino Oscillation Experiment

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    The analysis and results are presented from the complete data set recorded at Palo Verde between September 1998 and July 2000. In the experiment, the \nuebar interaction rate has been measured at a distance of 750 and 890 m from the reactors of the Palo Verde Nuclear Generating Station for a total of 350 days, including 108 days with one of the three reactors off for refueling. Backgrounds were determined by (a) the swapswap technique based on the difference between signal and background under reversal of the positron and neutron parts of the correlated event and (b) making use of the conventional reactor-on and reactor-off cycles. There is no evidence for neutrino oscillation and the mode \nuebar\to\bar\nu_x was excluded at 90% CL for \dm>1.1\times10^{-3} eV2^2 at full mixing, and \sinq>0.17 at large \dm.Comment: 11 pages, 8 figure
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