4,422 research outputs found

    Chaotic synchronization of coupled electron-wave systems with backward waves

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    The chaotic synchronization of two electron-wave media with interacting backward waves and cubic phase nonlinearity is investigated in the paper. To detect the chaotic synchronization regime we use a new approach, the so-called time scale synchronization [Chaos, 14 (3) 603-610 (2004)]. This approach is based on the consideration of the infinite set of chaotic signals' phases introduced by means of continuous wavelet transform. The complex space-time dynamics of the active media and mechanisms of the time scale synchronization appearance are considered.Comment: 11 pages, 7 figures, published in CHAOS, 15 (2005) 01370

    Plantas medicinais das comunidades do Nordeste Paraense: Marapanim, Augusto Corrêa e Bragança.

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    The M4 Core Project with HST --- I. Overview and First-Epoch

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    We present an overview of the ongoing Hubble Space Telescope large program GO-12911. The program is focused on the core of M4, the nearest Galactic globular cluster, and the observations are designed to constrain the number of binaries with massive companions (black holes, neutron stars, or white dwarfs) by measuring the ``wobble'' of the luminous (main-sequence) companion around the center of mass of the pair, with an astrometric precision of ~50 micro-arcseconds. The high spatial resolution and stable medium-band PSFs of WFC3/UVIS will make these measurements possible. In this work we describe: (i) the motivation behind this study, (ii) our observing strategy, (iii) the many other investigations enabled by this unique data set, and which of those our team is conducting, and (iv) a preliminary reduction of the first-epoch data-set collected on October 10, 2012.Comment: 25 pages, 14 figures (9 at low resolution), 3 tables. Published in: Astronomische Nachrichten, Volume 334, Issue 10, pages 1062-1085, December 2013. http://onlinelibrary.wiley.com/doi/10.1002/asna.201311911/abstrac

    Long Cycles in a Perturbed Mean Field Model of a Boson Gas

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    In this paper we give a precise mathematical formulation of the relation between Bose condensation and long cycles and prove its validity for the perturbed mean field model of a Bose gas. We decompose the total density ρ=ρshort+ρlong\rho=\rho_{{\rm short}}+\rho_{{\rm long}} into the number density of particles belonging to cycles of finite length (ρshort\rho_{{\rm short}}) and to infinitely long cycles (ρlong\rho_{{\rm long}}) in the thermodynamic limit. For this model we prove that when there is Bose condensation, ρlong\rho_{{\rm long}} is different from zero and identical to the condensate density. This is achieved through an application of the theory of large deviations. We discuss the possible equivalence of ρlong0\rho_{{\rm long}}\neq 0 with off-diagonal long range order and winding paths that occur in the path integral representation of the Bose gas.Comment: 10 page

    M4 Core Project with HST - III. Search for variable stars in the primary field

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    We present the results of a photometric search for variable stars in the core of the Galactic globular cluster M4. The input data are a large and unprecedented set of deep Hubble Space Telescope WFC3 images (large program GO-12911; 120 orbits allocated), primarily aimed at probing binaries with massive companions by detecting their astrometric wobbles. Though these data were not optimised to carry out a time-resolved photometric survey, their exquisite precision, spatial resolution and dynamic range enabled us to firmly detect 38 variable stars, of which 20 were previously unpublished. They include 19 cluster-member eclipsing binaries (confirming the large binary fraction of M4), RR Lyrae, and objects with known X-ray counterparts. We improved and revised the parameters of some among published variables.Comment: 11 pages, 5 figures, 2 tables. Accepted for publication in MNRA

    Physics of IED Blast Shock Tube Simulations for mTBI Research

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    Shock tube experiments and simulations are conducted with a spherical gelatin filled skull–brain surrogate, in order to study the mechanisms leading to blast induced mild traumatic brain injury. A shock tube including sensor system is optimized to simulate realistic improvised explosive device blast profiles obtained from full scale field tests. The response of the skull–brain surrogate is monitored using pressure and strain measurements. Fluid–structure interaction is modeled using a combination of computational fluid dynamics (CFD) simulations for the air blast, and a finite element model for the structural response. The results help to understand the physics of wave propagation, from air blast into the skull–brain. The presence of openings on the skull and its orientation does have a strong effect on the internal pressure. A parameter study reveals that when there is an opening in the skull, the skull gives little protection and the internal pressure is fairly independent on the skull stiffness; the gelatin shear stiffness has little effect on the internal pressure. Simulations show that the presence of pressure sensors in the gelatin hardly disturbs the pressure field

    Emergence of a non trivial fluctuating phase in the XY model on regular networks

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    We study an XY-rotor model on regular one dimensional lattices by varying the number of neighbours. The parameter 2γ12\ge\gamma\ge1 is defined. γ=2\gamma=2 corresponds to mean field and γ=1\gamma=1 to nearest neighbours coupling. We find that for γ<1.5\gamma<1.5 the system does not exhibit a phase transition, while for γ>1.5\gamma > 1.5 the mean field second order transition is recovered. For the critical value γ=γc=1.5\gamma=\gamma_c=1.5, the systems can be in a non trivial fluctuating phase for whichthe magnetisation shows important fluctuations in a given temperature range, implying an infinite susceptibility. For all values of γ\gamma the magnetisation is computed analytically in the low temperatures range and the magnetised versus non-magnetised state which depends on the value of γ\gamma is recovered, confirming the critical value γc=1.5\gamma_{c}=1.5
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