1,582 research outputs found

    Programmable Integrated Photonics for Topological Hamiltonians

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    A variety of topological Hamiltonians have been demonstrated in photonic platforms, leading to fundamental discoveries and enhanced robustness in applications such as lasing, sensing, and quantum technologies. To date, each topological photonic platform implements a specific type of Hamiltonian with inexistent or limited reconfigurability. Here, we propose and demonstrate different topological models by using the same reprogrammable integrated photonics platform, consisting of a hexagonal mesh of silicon Mach-Zehnder interferometers with phase-shifters. We specifically demonstrate a one-dimensional Su-Schrieffer-Heeger Hamiltonian supporting a localized topological edge mode and a higher-order topological insulator based on a two-dimensional breathing Kagome Hamiltonian with three corner states. These results highlight a nearly universal platform for topological models that may fast-track research progress toward applications of topological photonics and other coupled systems

    RESULTADOS PRELIMINARES EN LOS ESTUDIOS DE EFICIENCIA ENERGÉTICA DENTRO DEL PROYECTO DE I+D+i OPTIREG: GESTIÓN EFICIENTE DE REGADÍOS

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    [ES] El grupo de trabajo WP3 “Eficiencia energética” en el marco del proyecto I+D+i OPTIREG “Gestión Eficiente de Regadíos” del grupo Tragsa, lleva a cabo diversas actuaciones encaminadas a conocer el estado energético y organizativo de la gestión de las CC.RR. modernizadas, buscando metodologías que mejoren las herramientas de diagnóstico de la situación hídrico-energética de una C.RR., como también estrategias operativas que mejoren la eficiencia energética adaptándose a la idiosincrasia y condición de cada caso particular. Para alcanzar estos objetivos, los trabajos se están centrando en varios aspectos: – Recopilación de medidas efectivas de eficiencia energética aplicadas a los diversos ámbitos de la infraestructura y organización en que se diversifica una C.RR. – Caracterización de CC.RR. de Castilla y León con indicadores conocidos y nuevas propuestas de los mismos (benchmarking). – Evaluación de los rendimientos de la EB mediante el estudio de las curvas globales H-Q, P-Q y Rto-Q. – Estudio de curvas de frecuencia de caudales. – Elaboración y calibración de modelos hidráulicos de EB y red de riego en dos zonas piloto para análisis de escenarios simulados con fines a valorar nuevas estrategias de gestión que mejoren la eficiencia energética sin que se vea mermada la calidad del servicio (presión y caudal en el hidrante), ni aumenten el coste energético anual. – Pasarela de comunicación entre el programa de gestión de riegos Progar y Telegestar.Naranjo Hernández, D.; Colom Delgado, S.; Blanco Redondo, J.; González Muñoz, L.; Iglesias Gómez, S. (2015). RESULTADOS PRELIMINARES EN LOS ESTUDIOS DE EFICIENCIA ENERGÉTICA DENTRO DEL PROYECTO DE I+D+i OPTIREG: GESTIÓN EFICIENTE DE REGADÍOS. En XXXIII CONGRESO NACIONAL DE RIEGOS. Valencia 16-18 junio de 2015. Editorial Universitat Politècnica de València. https://doi.org/10.4995/CNRiegos.2015.1463OC

    Pure-quartic solitons

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    Temporal optical solitons have been the subject of intense research due to their intriguing physics and applications in ultrafast optics and supercontinuum generation. Conventional bright optical solitons result from the interaction of anomalous group-velocity dispersion and self-phase modulation. Here we experimentally demonstrate a class of bright soliton arising purely from the interaction of negative fourth-order dispersion and self-phase modulation, which can occur even for normal group-velocity dispersion. We provide experimental and numerical evidence of shape-preserving propagation and flat temporal phase for the fundamental pure-quartic soliton and periodically modulated propagation for the higher-order pure-quartic solitons. We derive the approximate shape of the fundamental pure-quartic soliton and discover that is surprisingly Gaussian, exhibiting excellent agreement with our experimental observations. Our discovery, enabled by precise dispersion engineering, could find applications in communications, frequency combs and ultrafast lasers

    Topologically protected localised states in spin chains

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    We consider spin chain families inspired by the Su, Schrieffer and Hegger (SSH) model. We demonstrate explicitly the topologically induced spatial localisation of quantum states in our systems. We present detailed investigations of the effects of random noise, showing that these topologically protected states are very robust against this type of perturbation. Systems with such topological robustness are clearly good candidates for quantum information tasks and we discuss some potential applications. Thus, we present interesting spin chain models which show promising applications for quantum devices

    Measurement of the Depth of Maximum of Extensive Air Showers above 10^18 eV

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    We describe the measurement of the depth of maximum, Xmax, of the longitudinal development of air showers induced by cosmic rays. Almost four thousand events above 10^18 eV observed by the fluorescence detector of the Pierre Auger Observatory in coincidence with at least one surface detector station are selected for the analysis. The average shower maximum was found to evolve with energy at a rate of (106 +35/-21) g/cm^2/decade below 10^(18.24 +/- 0.05) eV and (24 +/- 3) g/cm^2/decade above this energy. The measured shower-to-shower fluctuations decrease from about 55 to 26 g/cm^2. The interpretation of these results in terms of the cosmic ray mass composition is briefly discussed.Comment: Accepted for publication by PR

    Operations of and Future Plans for the Pierre Auger Observatory

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    Technical reports on operations and features of the Pierre Auger Observatory, including ongoing and planned enhancements and the status of the future northern hemisphere portion of the Observatory. Contributions to the 31st International Cosmic Ray Conference, Lodz, Poland, July 2009.Comment: Contributions to the 31st ICRC, Lodz, Poland, July 200

    Anisotropy and chemical composition of ultra-high energy cosmic rays using arrival directions measured by the Pierre Auger Observatory

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    The Pierre Auger Collaboration has reported evidence for anisotropy in the distribution of arrival directions of the cosmic rays with energies E>Eth=5.5×1019E>E_{th}=5.5\times 10^{19} eV. These show a correlation with the distribution of nearby extragalactic objects, including an apparent excess around the direction of Centaurus A. If the particles responsible for these excesses at E>EthE>E_{th} are heavy nuclei with charge ZZ, the proton component of the sources should lead to excesses in the same regions at energies E/ZE/Z. We here report the lack of anisotropies in these directions at energies above Eth/ZE_{th}/Z (for illustrative values of Z=6, 13, 26Z=6,\ 13,\ 26). If the anisotropies above EthE_{th} are due to nuclei with charge ZZ, and under reasonable assumptions about the acceleration process, these observations imply stringent constraints on the allowed proton fraction at the lower energies

    Atmospheric effects on extensive air showers observed with the Surface Detector of the Pierre Auger Observatory

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    Atmospheric parameters, such as pressure (P), temperature (T) and density, affect the development of extensive air showers initiated by energetic cosmic rays. We have studied the impact of atmospheric variations on extensive air showers by means of the surface detector of the Pierre Auger Observatory. The rate of events shows a ~10% seasonal modulation and ~2% diurnal one. We find that the observed behaviour is explained by a model including the effects associated with the variations of pressure and density. The former affects the longitudinal development of air showers while the latter influences the Moliere radius and hence the lateral distribution of the shower particles. The model is validated with full simulations of extensive air showers using atmospheric profiles measured at the site of the Pierre Auger Observatory.Comment: 24 pages, 9 figures, accepted for publication in Astroparticle Physic
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