2,002 research outputs found

    Las especies del gĂŠnero Myotis (Chiroptera: Vespertilionidae) en el bajo delta del ParanĂĄ y la pampa ondulada, Argentina

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    El gĂŠnero Myotis se distribuye en todo el mundo, excepto en los polos, e incluye mĂĄs de 100 especies, de las cuales 12 se presentan en Argentina. El conocimiento sobre los murciĂŠlagos de este gĂŠnero es escaso en amplias ĂĄreas de Argentina, como por ejemplo en la Pampa Ondulada y el Bajo Delta del ParanĂĄ. En este trabajo se estudian las especies de Myotis colectadas en tres localidades del ĂĄrea mencionada: dos en el departamento Islas del Ibicuy (provincia de Entre RĂ­os), y una en el Parque Costero Sur (provincia de Buenos Aires). Se presentan datos morfomĂŠtricos y caracterĂ­sticas de los ejemplares colectados, aportando informaciĂłn sobre la variabilidad intraespecĂ­fica de cada especie colectada en el ĂĄrea. En total se colectaron 51 ejemplares pertenecientes a 5 especies: M. albescens, M. dinellii, M. levis, M. ruber y M. riparius. Esta Ăşltima especie es registrada por primera vez para las provincias de Entre RĂ­os y Buenos Aires.The genus Myotis is distributed worldwide, except at the poles. It includes more than 100 species, 12 of which are present in Argentina. Knowledge about the bats of this genus is sparse in large areas of Argentina, including the Rolling Pampa and Lower Delta of the Parana River. Here, we present a study about the species of Myotis collected in three locations: two at Islas del Ibicuy department (Entre RĂ­os province), and one at Parque Costero del Sur (Buenos Aires province). Morphometric data and characteristics of the collected specimens are described, providing information on intraspecific variability of each species collected in the area. We collected 51 specimens belonging to 5 species of this genus: M. albescens, M. dinellii, M. levis, M. ruber and M. riparius. The latter is recorded for first time in the provinces of Entre RĂ­os and Buenos Aires.ISSN 1666-053

    Study of the one-dimensional off-lattice hot-monomer reaction model

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    Hot monomers are particles having a transient mobility (a ballistic flight) prior to being definitely absorbed on a surface. After arriving at a surface, the excess energy coming from the kinetic energy in the gas phase is dissipated through degrees of freedom parallel to the surface plane. In this paper we study the hot monomer-monomer adsorption-reaction process on a continuum (off-lattice) one-dimensional space by means of Monte Carlo simulations. The system exhibits second-order irreversible phase transition between a reactive and saturated (absorbing) phases which belong to the directed percolation (DP) universality class. This result is interpreted by means of a coarse-grained Langevin description which allows as to extend the DP conjecture to transitions occurring in continuous media.Comment: 13 pages, 5 figures, final version to appear in J. Phys.

    Population genetics in compressible flows

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    We study competition between two biological species advected by a compressible velocity field. Individuals are treated as discrete Lagrangian particles that reproduce or die in a density-dependent fashion. In the absence of a velocity field and fitness advantage, number fluctuations lead to a coarsening dynamics typical of the stochastic Fisher equation. We then study three examples of compressible advecting fields: a shell model of turbulence, a sinusoidal velocity field and a linear velocity sink. In all cases, advection leads to a striking drop in the fixation time, as well as a large reduction in the global carrying capacity. Despite localization on convergence zones, one species goes extinct much more rapidly than in well-mixed populations. For a weak harmonic potential, one finds a bimodal distribution of fixation times. The long-lived states in this case are demixed configurations with a single boundary, whose location depends on the fitness advantage.Comment: 10 pages, 5 figures, submitte

    Transition to Stochastic Synchronization in Spatially Extended Systems

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    Spatially extended dynamical systems, namely coupled map lattices, driven by additive spatio-temporal noise are shown to exhibit stochastic synchronization. In analogy with low-dymensional systems, synchronization can be achieved only if the maximum Lyapunov exponent becomes negative for sufficiently large noise amplitude. Moreover, noise can suppress also the non-linear mechanism of information propagation, that may be present in the spatially extended system. A first example of phase transition is observed when both the linear and the non-linear mechanisms of information production disappear at the same critical value of the noise amplitude. The corresponding critical properties can be hardly identified numerically, but some general argument suggests that they could be ascribed to the Kardar-Parisi-Zhang universality class. Conversely, when the non-linear mechanism prevails on the linear one, another type of phase transition to stochastic synchronization occurs. This one is shown to belong to the universality class of directed percolation.Comment: 21 pages, Latex - 14 EPS Figs - To appear on Physical Review

    Reduction of Dispersion in Ultrasonically-Enhanced Micropacked Beds

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    Channeling of gas can reduce mass transfer performance in multiphase micropacked-bed reactors. Viscous and capillary forces cause this undesired and often unpredictable phenomenon in systems with catalyst particle sizes of hundreds of micrometers. In this work, we acoustically modify flow in a micropacked-bed reactor to reduce gas channeling by applying high-power sonication at low ultrasonic frequencies (∟40 kHz). Experimental residence time distributions reveal two orders of magnitude reduction in dispersion with ultrasound, allowing for nearly plug-flow behavior at high flow rates in the bed. Sonication appears to partially fluidize the packed-bed under pressurized cocurrent two-phase flow, effectively improving dispersion characteristics.This research was partially funded by the EU project MAPSYN: Microwave, Acoustic and Plasma SYNtheses, under Grant CPIP 309376 of the European Union Seventh Framework Program

    KELT-8b: A highly inflated transiting hot Jupiter and a new technique for extracting high-precision radial velocities from noisy spectra

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    We announce the discovery of a highly inflated transiting hot Jupiter discovered by the KELT-North survey. A global analysis including constraints from isochrones indicates that the V = 10.8 host star (HD 343246) is a mildly evolved, G dwarf with Teff=5754−55+54T_{\rm eff} = 5754_{-55}^{+54} K, log⁡g=4.078−0.054+0.049\log{g} = 4.078_{-0.054}^{+0.049}, [Fe/H]=0.272±0.038[Fe/H] = 0.272\pm0.038, an inferred mass M∗=1.211−0.066+0.078M_{*}=1.211_{-0.066}^{+0.078} M⊙_{\odot}, and radius R∗=1.67−0.12+0.14R_{*}=1.67_{-0.12}^{+0.14} R⊙_{\odot}. The planetary companion has mass MP=0.867−0.061+0.065M_P = 0.867_{-0.061}^{+0.065} MJM_{J}, radius RP=1.86−0.16+0.18R_P = 1.86_{-0.16}^{+0.18} RJR_{J}, surface gravity log⁡gP=2.793−0.075+0.072\log{g_{P}} = 2.793_{-0.075}^{+0.072}, and density ρP=0.167−0.038+0.047\rho_P = 0.167_{-0.038}^{+0.047} g cm−3^{-3}. The planet is on a roughly circular orbit with semimajor axis a=0.04571−0.00084+0.00096a = 0.04571_{-0.00084}^{+0.00096} AU and eccentricity e=0.035−0.025+0.050e = 0.035_{-0.025}^{+0.050}. The best-fit linear ephemeris is T0=2456883.4803±0.0007T_0 = 2456883.4803 \pm 0.0007 BJDTDB_{\rm TDB} and P=3.24406±0.00016P = 3.24406 \pm 0.00016 days. This planet is one of the most inflated of all known transiting exoplanets, making it one of the few members of a class of extremely low density, highly-irradiated gas giants. The low stellar log⁡g\log{g} and large implied radius are supported by stellar density constraints from follow-up light curves, plus an evolutionary and space motion analysis. We also develop a new technique to extract high precision radial velocities from noisy spectra that reduces the observing time needed to confirm transiting planet candidates. This planet boasts deep transits of a bright star, a large inferred atmospheric scale height, and a high equilibrium temperature of Teq=1675−55+61T_{eq}=1675^{+61}_{-55} K, assuming zero albedo and perfect heat redistribution, making it one of the best targets for future atmospheric characterization studies.Comment: Submitted to ApJ, feedback is welcom

    KELT-7b: A hot Jupiter transiting a bright V=8.54 rapidly rotating F-star

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    We report the discovery of KELT-7b, a transiting hot Jupiter with a mass of 1.28±0.181.28 \pm 0.18 MJ, radius of 1.53−0.047+0.0461.53_{-0.047}^{+0.046} RJ, and an orbital period of 2.7347749±0.00000392.7347749 \pm 0.0000039 days. The bright host star (HD33643; KELT-7) is an F-star with V=8.54V=8.54, Teff =6789−49+50=6789_{-49}^{+50} K, [Fe/H] =0.139−0.081+0.075=0.139_{-0.081}^{+0.075}, and log⁡g=4.149±0.019\log{g}=4.149 \pm 0.019. It has a mass of 1.535−0.054+0.0661.535_{-0.054}^{+0.066} Msun, a radius of 1.732−0.045+0.0431.732_{-0.045}^{+0.043} Rsun, and is the fifth most massive, fifth hottest, and the ninth brightest star known to host a transiting planet. It is also the brightest star around which KELT has discovered a transiting planet. Thus, KELT-7b is an ideal target for detailed characterization given its relatively low surface gravity, high equilibrium temperature, and bright host star. The rapid rotation of the star (73±0.573 \pm 0.5 km/s) results in a Rossiter-McLaughlin effect with an unusually large amplitude of several hundred m/s. We find that the orbit normal of the planet is likely to be well-aligned with the stellar spin axis, with a projected spin-orbit alignment of λ=9.7±5.2\lambda=9.7 \pm 5.2 degrees. This is currently the second most rapidly rotating star to have a reflex signal (and thus mass determination) due to a planetary companion measured.Comment: Accepted to The Astronomical Journa

    Measurements of Higgs boson production and couplings in diboson final states with the ATLAS detector at the LHC

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    Measurements are presented of production properties and couplings of the recently discovered Higgs boson using the decays into boson pairs, H →γ γ, H → Z Z∗ →4l and H →W W∗ →lνlν. The results are based on the complete pp collision data sample recorded by the ATLAS experiment at the CERN Large Hadron Collider at centre-of-mass energies of √s = 7 TeV and √s = 8 TeV, corresponding to an integrated luminosity of about 25 fb−1. Evidence for Higgs boson production through vector-boson fusion is reported. Results of combined fits probing Higgs boson couplings to fermions and bosons, as well as anomalous contributions to loop-induced production and decay modes, are presented. All measurements are consistent with expectations for the Standard Model Higgs boson

    Standalone vertex nding in the ATLAS muon spectrometer

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    A dedicated reconstruction algorithm to find decay vertices in the ATLAS muon spectrometer is presented. The algorithm searches the region just upstream of or inside the muon spectrometer volume for multi-particle vertices that originate from the decay of particles with long decay paths. The performance of the algorithm is evaluated using both a sample of simulated Higgs boson events, in which the Higgs boson decays to long-lived neutral particles that in turn decay to bbar b final states, and pp collision data at √s = 7 TeV collected with the ATLAS detector at the LHC during 2011
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