54 research outputs found

    Knowledge and Technology Transfer in Materials Science and Engineering in Europe

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    Advanced Materials is one of the Key Enabling 3 Technologies identified by the European Commission1. Together with Advanced Manufacturing it underpins almost all other Key Enabling and Industrial Technologies. The basic science and engineering research that results in the development of Advanced Materials lies within the field of Materials Science and Engineering (MSE). The transfer of knowledge from basic research into final products and applications in the field of MSE involves certain MSE-typical motifs and specific issues, as well as certain aspects that are special to Europe. In comparison with underlying traditional (or basic) disciplines such as physics, chemistry or biology, MSE involves a range of aspects that are more characteristic of applied science, where relevance has equal importance to curiosity in order to drive the research effort and justify expenditure – the defined goals often being a proven innovative technology or indeed a particular product. MSE and the related transfer of knowledge and technology includes consideration of factors such as materials and product life cycles, the abundance of materials, the technical, ecological and economic feasibility of materials engineering and processing, as well as the multidisciplinarity of the ‘background’ knowledge and the efficiency of the academic effort involved. This is even more the case for situations that involve successful validation of technologies and effective transfer of knowledge between academia and industry. The state of knowledge and technology transfer in Europe differs from that of other global players, such as the US, China or Japan. Europe’s cultural diversity gives rise to both positive and negative factors. Positive aspects include the high standard of general education and Europe’s highly skilled work force (for both technical and academic staff), and the flexibility and variety of research topics and directions. Major negative factors are the fragmentation of national research efforts, and the lack of a European mechanism to create critical mass in new technologies and to invest in pilot lines. These negative issues are manifested by the fragmentation of research programmes, the lack of venture capital and a general risk aversion on the part of investors in Europe, in particular in the light of the current economic crisis in Europe. The present situation has often been described as a malfunctioning interface between strong basic research and poor, inefficient technological development and commercial exploitation of knowledge. MSE spans this interface. ‘European’ knowledge is world-class, and even leads the world in certain fundamental areas of MSE, for example in the investigation and understanding of materials properties, the development and application of new concepts of materials design, computational materials sciences, and several other fields. However, Europe’s MSE knowledge and technological progress will not readily lead to the establishment of new technologies and products by European industries without dedicated intervention. This knowledge must be delicately directed in a highly impact-oriented way. To accelerate development and validation of technological applications and the introduction of technological innovation into the market, to intensify the collaboration between academic institutions and industry in Europe, and to facilitate the creation of spin-out companies and new industrial–academic career paths, MatSEEC recommends the creation of European Technology Research and Validation Platforms (ETVPs). Such platforms would provide powerful tools for innovation and allow better protection of intellectual property rights in Europe. We recommend the creation of an ‘Open-Access-Open-Innovation’ European Technology Research and Validation Infrastructure Initiative to streamline and improve technology and knowledge transfer in Europe. The initiative would be dedicated to technology research and validation. It could be based on a similar model to the current Integrated Infrastructure Initiatives (I3s) for research infrastructures of the European Commission (the I3 Programme in H2020 and the Seventh Framework Programme,FP7)

    Harnessing a Vibroacoustic Mode for Enabling Smart Functions on Surface Acoustic Wave Devices -- Application to Icing Monitoring and Deicing

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    Microacoustic wave devices are essential components in the RF electronics and MEMS industry with increasing impact in various sensing and actuation applications. Reliable and smart operation of acoustic wave devices at low costs would cause a crucial advancement. Herein, we present the enablement of temperature and mechanical sensing capabilities in a Rayleigh-mode standing surface acoustic wave (sSAW) chip device by harnessing an acoustic shear plate wave mode using the same set of electrodes. Most importantly, this mode is excited by switching the polarity of the sSAW transducer electrodes by simple electronics, allowing for direct and inexpensive compatibility with an existing setup. We validated the method in the emergent topic of surface de-icing by continuously monitoring temperature and water liquid-solid phase changes using the plate wave mode, and on-demand Rayleigh-wave deicing with a negligible energy cost. The flexibility for adapting the system to different scenarios, loads and scalability opens the path to impact in lab-on-a-chip, IoT technology, and sectors requiring autonomous acoustic wave actuators.Comment: 8 pages, 3 figure

    In situ monitoring of the phenomenon of electrochemical promotion of catalysis

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    In this work we investigate by in-situ near-ambient pressure photoemission (NAPP) spectroscopy the phenomenon of Electrochemical Promotion of Catalysis (EPOC). We studied the reduction and diffusion kinetics of alkaline ions in a solid electrolyte cell formed by a nickel electrode supported on K+-ÎČ-alumina electrolyte. Experiments in ultra-high vacuum and in the presence of steam showed that the amount of potassium atoms supplied to the surface is probably affected by nickel electronic modifications induced by adsorbed OH− groups. It was also deduced that part of the segregated potassium would be adsorbed at inner interfaces where it would be inaccessible to the photoelectron analyzer. A migration mechanism of the promoter is proposed consisting in: (i) the electrochemical reduction of the alkali ions (potassium) at the Ni/solid electrolyte/gas interface; (ii) the spillover of potassium atoms onto the Ni gas-exposed surface; and (iii) the diffusion of potassium atoms to Ni inner grain boundary interfaces.En este trabajo investigamos mediante espectroscopĂ­a de fotoemisiĂłn a presiĂłn cercana al ambiente in situ (NAPP) el fenĂłmeno de la PromociĂłn ElectroquĂ­mica de la CatĂĄlisis (EPOC). Estudiamos la cinĂ©tica de reducciĂłn y difusiĂłn de iones alcalinos en una celda de electrolito sĂłlido formada por un electrodo de nĂ­quel soportado sobre electrolito K + -ÎČ-alĂșmina. Los experimentos en vacĂ­o ultraalto y en presencia de vapor mostraron que la cantidad de ĂĄtomos de potasio suministrados a la superficie probablemente se ve afectada por modificaciones electrĂłnicas de nĂ­quel inducidas por OH adsorbido .grupos TambiĂ©n se dedujo que parte del potasio segregado serĂ­a adsorbido en las interfaces internas donde serĂ­a inaccesible para el analizador de fotoelectrones. Se propone un mecanismo de migraciĂłn del promotor que consiste en: (i) la reducciĂłn electroquĂ­mica de los iones alcalinos (potasio) en la interfase Ni/electrolito sĂłlido/gas; (ii) el derrame de ĂĄtomos de potasio sobre la superficie expuesta al gas Ni; y (iii) la difusiĂłn de ĂĄtomos de potasio a las interfaces de lĂ­mite de grano interno de Ni

    Graphene Formation Mechanism by the Electrochemical Promotion of a Ni Catalyst

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    In this work, we show that multilayer graphene forms by methanol decomposition at 280 °C on an electrochemically promoted nickel catalyst film supported on a K-ÎČAl2O3 solid electrolyte. In operando near ambient pressure photoemission spectroscopy and electrochemical measurements have shown that polarizing negatively the Ni electrode induces the electrochemical reduction and migration of potassium to the nickel surface. This elemental potassium promotes the catalytic decomposition of methanol into graphene and also stabilizes the graphene formed via diffusion and direct K–C interaction. Experiments reveal that adsorbed methoxy radicals are intermediate species in this process and that, once formed, multilayer graphene remains stable after electrochemical oxidation and back migration of potassium to the solid electrolyte upon positive polarization. The reversible diffusion of ca. 100 equivalent monolayers of potassium through the carbon layers and the unprecedented low-temperature formation of graphene and other carbon forms are mechanistic pathways of high potential impact for applications where mild synthesis and operation conditions are required.En este trabajo mostramos que el grafeno multicapa se forma por descomposiciĂłn del metanol a 280 °C sobre una pelĂ­cula de catalizador de nĂ­quel promovida electroquĂ­micamente soportada sobre un K-ÎČAl 2 O 3electrolito sĂłlido. Operando cerca de la espectroscopia de fotoemisiĂłn a presiĂłn ambiental y las mediciones electroquĂ­micas han demostrado que la polarizaciĂłn negativa del electrodo de Ni induce la reducciĂłn electroquĂ­mica y la migraciĂłn del potasio a la superficie del nĂ­quel. Este potasio elemental promueve la descomposiciĂłn catalĂ­tica del metanol en grafeno y tambiĂ©n estabiliza el grafeno formado a travĂ©s de la difusiĂłn y la interacciĂłn directa K-C. Los experimentos revelan que los radicales metoxi adsorbidos son especies intermedias en este proceso y que, una vez formado, el grafeno multicapa permanece estable despuĂ©s de la oxidaciĂłn electroquĂ­mica y la migraciĂłn de regreso del potasio al electrolito sĂłlido tras la polarizaciĂłn positiva. La difusiĂłn reversible de ca

    Measurement of the cosmic ray spectrum above 4×10184{\times}10^{18} eV using inclined events detected with the Pierre Auger Observatory

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    A measurement of the cosmic-ray spectrum for energies exceeding 4×10184{\times}10^{18} eV is presented, which is based on the analysis of showers with zenith angles greater than 60∘60^{\circ} detected with the Pierre Auger Observatory between 1 January 2004 and 31 December 2013. The measured spectrum confirms a flux suppression at the highest energies. Above 5.3×10185.3{\times}10^{18} eV, the "ankle", the flux can be described by a power law E−γE^{-\gamma} with index Îł=2.70±0.02 (stat)±0.1 (sys)\gamma=2.70 \pm 0.02 \,\text{(stat)} \pm 0.1\,\text{(sys)} followed by a smooth suppression region. For the energy (EsE_\text{s}) at which the spectral flux has fallen to one-half of its extrapolated value in the absence of suppression, we find Es=(5.12±0.25 (stat)−1.2+1.0 (sys))×1019E_\text{s}=(5.12\pm0.25\,\text{(stat)}^{+1.0}_{-1.2}\,\text{(sys)}){\times}10^{19} eV.Comment: Replaced with published version. Added journal reference and DO

    Energy Estimation of Cosmic Rays with the Engineering Radio Array of the Pierre Auger Observatory

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    The Auger Engineering Radio Array (AERA) is part of the Pierre Auger Observatory and is used to detect the radio emission of cosmic-ray air showers. These observations are compared to the data of the surface detector stations of the Observatory, which provide well-calibrated information on the cosmic-ray energies and arrival directions. The response of the radio stations in the 30 to 80 MHz regime has been thoroughly calibrated to enable the reconstruction of the incoming electric field. For the latter, the energy deposit per area is determined from the radio pulses at each observer position and is interpolated using a two-dimensional function that takes into account signal asymmetries due to interference between the geomagnetic and charge-excess emission components. The spatial integral over the signal distribution gives a direct measurement of the energy transferred from the primary cosmic ray into radio emission in the AERA frequency range. We measure 15.8 MeV of radiation energy for a 1 EeV air shower arriving perpendicularly to the geomagnetic field. This radiation energy -- corrected for geometrical effects -- is used as a cosmic-ray energy estimator. Performing an absolute energy calibration against the surface-detector information, we observe that this radio-energy estimator scales quadratically with the cosmic-ray energy as expected for coherent emission. We find an energy resolution of the radio reconstruction of 22% for the data set and 17% for a high-quality subset containing only events with at least five radio stations with signal.Comment: Replaced with published version. Added journal reference and DO

    Measurement of the Radiation Energy in the Radio Signal of Extensive Air Showers as a Universal Estimator of Cosmic-Ray Energy

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    We measure the energy emitted by extensive air showers in the form of radio emission in the frequency range from 30 to 80 MHz. Exploiting the accurate energy scale of the Pierre Auger Observatory, we obtain a radiation energy of 15.8 \pm 0.7 (stat) \pm 6.7 (sys) MeV for cosmic rays with an energy of 1 EeV arriving perpendicularly to a geomagnetic field of 0.24 G, scaling quadratically with the cosmic-ray energy. A comparison with predictions from state-of-the-art first-principle calculations shows agreement with our measurement. The radiation energy provides direct access to the calorimetric energy in the electromagnetic cascade of extensive air showers. Comparison with our result thus allows the direct calibration of any cosmic-ray radio detector against the well-established energy scale of the Pierre Auger Observatory.Comment: Replaced with published version. Added journal reference and DOI. Supplemental material in the ancillary file

    Multiple Scenario Generation of Subsurface Models:Consistent Integration of Information from Geophysical and Geological Data throuh Combination of Probabilistic Inverse Problem Theory and Geostatistics

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    Neutrinos with energies above 1017 eV are detectable with the Surface Detector Array of the Pierre Auger Observatory. The identification is efficiently performed for neutrinos of all flavors interacting in the atmosphere at large zenith angles, as well as for Earth-skimming \u3c4 neutrinos with nearly tangential trajectories relative to the Earth. No neutrino candidates were found in 3c 14.7 years of data taken up to 31 August 2018. This leads to restrictive upper bounds on their flux. The 90% C.L. single-flavor limit to the diffuse flux of ultra-high-energy neutrinos with an E\u3bd-2 spectrum in the energy range 1.0 7 1017 eV -2.5 7 1019 eV is E2 dN\u3bd/dE\u3bd < 4.4 7 10-9 GeV cm-2 s-1 sr-1, placing strong constraints on several models of neutrino production at EeV energies and on the properties of the sources of ultra-high-energy cosmic rays
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