Impurities and electronic localization in graphene bilayers

We analyze the electronic properties of bilayer graphene with Bernal stacking and a low concentration of adatoms. Assuming that the host bilayer lies on top of a substrate, we consider the case where impurities are adsorbed only on the upper layer. We describe non-magnetic impurities as a single orbital hybridized with carbon's pz states. The effect of impurity doping on the local density of states with and without a gated electric field perpendicular to the layers is analyzed. We look for Anderson localization in the different regimes and estimate the localization length. In the biased system, the field induced gap is partially filled by strongly localized impurity states. Interestingly, the structure, distribution and localization length of these states depend on the field polarization.Comment: 7 pages, 6 figure

Bilayer graphene under pressure: Electron-hole Symmetry Breaking, Valley Hall Effect, and Landau Levels

The electronic structure of bilayer graphene under pressure develops very interesting features with an enhancement of the trigonal warping and a splitting of the parabolic touching bands at the K point of the reciprocal space into four Dirac cones, one at K and three along the T symmetry lines. As pressure is increased, these cones separate in reciprocal space and in energy, breaking the electron-hole symmetry. Due to their energy separation, their opposite Berry curvature can be observed in valley Hall effect experiments and in the structure of the Landau levels. Based on the electronic structure obtained by Density Functional Theory, we develop a low energy Hamiltonian that describes the effects of pressure on measurable quantities such as the Hall conductivity and the Landau levels of the system.Comment: 11 pages, 9 figure

Tuning the proximity effect in a superconductor-graphene-superconductor junction

We have tuned in situ the proximity effect in a single graphene layer coupled to two Pt/Ta superconducting electrodes. An annealing current through the device changed the transmission coefficient of the electrode/graphene interface, increasing the probability of multiple Andreev reflections. Repeated annealing steps improved the contact sufficiently for a Josephson current to be induced in graphene.Comment: Accepted for publication in Phys. Rev.

Supersymmetry of FRW barotropic cosmologies

Barotropic FRW cosmologies are presented from the standpoint of nonrelativistic supersymmetry. First, we reduce the barotropic FRW system of differential equations to simple harmonic oscillator differential equations. Employing the factorization procedure, the solutions of the latter equations are divided into the two classes of bosonic (nonsingular) and fermionic (singular) cosmological solutions. We next introduce a coupling parameter denoted by K between the two classes of solutions and obtain barotropic cosmologies with dissipative features acting on the scale factors and spatial curvature of the universe. The K-extended FRW equations in comoving time are presented in explicit form in the low coupling regime. The standard barotropic FRW cosmologies correspond to the dissipationless limit K =0Comment: 6 page

Measurements of Stellar Inclinations for Kepler Planet Candidates II: Candidate Spin-Orbit Misalignments in Single and Multiple-Transiting Systems

We present a test for spin-orbit alignment for the host stars of 25 candidate planetary systems detected by the {\it Kepler} spacecraft. The inclination angle of each star's rotation axis was estimated from its rotation period, rotational line broadening, and radius. The rotation periods were determined using the {\it Kepler} photometric time series. The rotational line broadening was determined from high-resolution optical spectra with Subaru/HDS. Those same spectra were used to determine the star's photospheric parameters (effective temperature, surface gravity, metallicity) which were then interpreted with stellar-evolutionary models to determine stellar radii. We combine the new sample with the 7 stars from our previous work on this subject, finding that the stars show a statistical tendency to have inclinations near 90$^\circ$, in alignment with the planetary orbits. Possible spin-orbit misalignments are seen in several systems, including three multiple-planet systems (KOI-304, 988, 2261). Ideally these systems should be scrutinized with complementary techniques---such as the Rossiter-McLaughlin effect, starspot-crossing anomalies or asteroseismology---but the measurements will be difficult owing to the relatively faint apparent magnitudes and small transit signals in these systems.Comment: 11 pages, 9 figures, accepted for publication in Ap

Inhalación de esporas de Aspergillus fumigatus induce en ratones una inflamación de las vías aéreas similar a la observada en equinos con Obstrucción Recurrente de las Vías Aéreas

The aim of this study was to determine if mice exposed to Aspergillus (A.) fumigatus spores develop airway inflammation in a similar manner to Recurrent Airway Obstruction (RAO) in horses. Different groups of 2-, 5-, 6- and 8-month-old Rockefeller (RK) mice were used throughout the experiment. The mice were maintained in the animal house for 16 days and kept in cages containing hay contaminated with A. fumigatus. After 16 days of mold exposure, the mice were bled and sacrificed to obtain bronchoalveolar lavage fluid (BALF) or lung tissues for histological analysis. In addition, we measured the levels of A. fumigatus-specific antibodies by ELISA. The results demonstrated that inhalation of A. fumigatus spores in mice induced an inflammatory response in the lungs that was characterized by peribronchiolar and perivascular mononuclear infiltration and bronchiolar luminal exudates. Moreover, there was extensive folding of the airway epithelia, which is a sign of airway smooth muscle contraction and smooth muscle hypertrophy. In addition, we observed a high number of neutrophils and an increase in IgE, IgG1 and IgG2a antibodies in the BALF from mice that were older than 5 months and were exposed to A. fumigatus. These animals recovered from their respiratory distress when they were placed in a remission environment. We conclude that simple exposure of mice to moldy hay induces a condition that is similar to RAO in horses. Therefore, using this mouse model for the study of equine RAO offers the opportunity to approximate the immunologic response to airborne irritants and allergens as well as to evaluate pharmacological therapies.El objetivo de este estudio fue determinar si ratones expuestos a esporas de Aspergillus fumigatus desarrollan una inflamación alérgica de las vías respiratorias similar a la observada en equinos con Obstrucción Recurrente de las Vías Aéreas (ORVA). Para esto se utilizaron ratones Rockefeller (RK) de 2, 5, 6 y 8 meses respectivamente, los cuales se mantuvieron por 16 días en jaulas que contenían heno contaminado con A. fumigatus. Posterior a la exposición, los animales fueron sangrados y sacrificados para la obtención de suero sanguíneo, lavado broncoalveolar (LBA) y muestras de tejido pulmonar. Además, se midieron los niveles de anticuerpos específicos para A. fumigatus a través de un ELISA indirecto. Los resultados mostraron que la inhalación de esporas de A. fumigatus en ratones induce una respuesta alérgica inflamatoria en pulmones similar a lo observado en ORVA equino, con un aumento del porcentaje de neutrófilos en el LBA y cambios histológicos pulmonares característicos de una hipersensibilidad bronquial. Asimismo, se observó un aumento de los niveles de inmunoglubulinas IgE, IgG1 e IgG2a específicas para este hongo en fluidos bronquiales. Además, los animales remitieron el estrés respiratorio cuando fueron expuestos en un ambiente de remisión. Se puede concluir que la simple exposición de esporas de A. fumugatus produce una condición alérgica similar al ORVA en equinos. Por lo tanto, este modelo experimental puede ser de utilidad para el estudio de los mecanismos inmunológicos, y probar nuevas opciones terapéuticas para esta enfermedad respiratoria de los caballos

Extended States in a One-dimensional Generalized Dimer Model

The transmission coefficient for a one dimensional system is given in terms of Chebyshev polynomials using the tight-binding model. This result is applied to a system composed of two impurities located between $N$ sites of a host lattice. It is found that the system has extended states for several values of the energy. Analytical expressions are given for the impurity site energy in terms of the electron's energy. The number of resonant states grows like the number of host sites between the impurities. This property makes the system interesting since it is a simple task to design a configuration with resonant energy very close to the Fermi level $E_F$.Comment: 4 pages, 3 figure

Using Kepler transit observations to measure stellar spot belt migration rates

Planetary transits provide a unique opportunity to investigate the surface distributions of star spots. Our aim is to determine if, with continuous observation (such as the data that will be provided by the Kepler mission), we can in addition measure the rate of drift of the spot belts. We begin by simulating magnetic cycles suitable for the Sun and more active stars, incorporating both flux emergence and surface transport. This provides the radial magnetic field distribution on the stellar surface as a function of time. We then model the transit of a planet whose orbital axis is misaligned with the stellar rotation axis. Such a planet could occult spots at a range of latitudes. This allows us to complete the forward modelling of the shape of the transit lightcurve. We then attempt the inverse problem of recovering spot locations from the transit alone. From this we determine if transit lightcurves can be used to measure spot belt locations as a function of time. We find that for low-activity stars such as the Sun, the 3.5 year Kepler window is insufficient to determine this drift rate. For more active stars, it may be difficult to distinguish subtle differences in the nature of flux emergence, such as the degree of overlap of the "butterfly wings". The rate and direction of drift of the spot belts can however be determined for these stars. This would provide a critical test of dynamo theory.Comment: 5 pages. Accepted for publication in Monthly Notices of the Royal Astronomical Society Letter