RFID-triggered power activation for smart dynamic inductive wireless power transfer

A RFID-triggered power activation system is devised, implemented and tested as the key sensing mechanism for controlling wireless power transfer from an inductive lane to a moving lightweight electric vehicle. The RFID reader and tag used are based on ISO/IEC-14443A compatible types, working at 13.56 MHz, one of the least expensive currently available passive near-field technologies. In order to fit lightweight electric mobility application requirements, the RFID magnetic antennas are redesigned to larger than standard sizes, both at reader and tag sides, increasing the detection volume without increasing the required reading power, thus permitting the reuse of commercial RFID circuits and embedded protocol software. To trigger the wireless power transfer, a RFID reader coil is placed magnetically orthogonal to each primary power coil to be controlled, at the extremity where electric vehicles are expected to come from, in a one-way traffic. The power is turned off automatically when the vehicle leaves the primary coil field and the power demand is extinguished, or when time-out is reached. An inductive lane constituted of a sequence of such RFID-controlled primary coils can detect the presence of authorized electric vehicles and smartly energize the lane, manipulating the unique identifier codes and other information stored in the on-board tag to more efficiently handle dissimilar power level demands, and to implement tolling. The performance of the system is predicted based on the reconstructed 3D digital model of the RFID main detection lobe.Universidade de Vigo - Department of Electronics Technolog

The evolution of the UV luminosity and stellar mass functions of Lyman-α emitters from z ~2 to z ~6

We measure the evolution of the rest-frame UV luminosity function (LF) and the stellar mass function (SMF) of Lyman-α (Ly α) emitters (LAEs) from z ~ 2 to z ~ 6 by exploring ~4000 LAEs from the SC4K sample. We find a correlation between Ly α luminosity (LLy α) and rest-frame UV (MUV), with best fit MUV = -1.6+0.2-0.3 log10(LLy α/erg s-1) + 47+12-11 and a shallower relation between LLy α and stellar mass (M∗), with best fit log10(M∗/M·) = 0.9+0.1-0.1 log10(LLy α/erg s-1) - 28+4.0-3.8. An increasing LLy α cut predominantly lowers the number density of faint MUV and low M∗ LAEs. We estimate a proxy for the full UV LFs and SMFs of LAEs with simple assumptions of the faint end slope. For the UV LF, we find a brightening of the characteristic UV luminosity (M∗UV) with increasing redshift and a decrease of the characteristic number density (Φ∗). For the SMF, we measure a characteristic stellar mass (M∗∗/M·) increase with increasing redshift, and a Φ∗ decline. However, if we apply a uniform luminosity cut of log10(LLy α/erg s-1) ≥ 43.0, we find much milder to no evolution in the UV and SMF of LAEs. The UV luminosity density (ρUV) of the full sample of LAEs shows moderate evolution and the stellar mass density (ρM) decreases, with both being always lower than the total ρUV and ρM of more typical galaxies but slowly approaching them with increasing redshift. Overall, our results indicate that both ρUV and ρM of LAEs slowly approach the measurements of continuum-selected galaxies at z > 6, which suggests a key role of LAEs in the epoch of reionization

Electro-osmotic flow of couple stress fluids in a microchannel propagated by peristalsis

A mathematical model is developed for electro-osmotic peristaltic pumping of a non-Newtonian liquid in a deformable micro-channel. Stokes’ couple stress fluid model is deployed to represent realistic working liquids. The Poisson-Boltzmann equation for electric potential distribution is implemented owing to the presence of an electrical double layer (EDL) in the micro-channel. Using long wavelength, lubrication theory and Debye-Huckel approximations, the linearized transformed dimensionless boundary value problem is solved analytically. The influence of electro-osmotic parameter (inversely proportional to Debye length), maximum electro-osmotic velocity (a function of external applied electrical field) and couple stress parameter on axial velocity, volumetric flow rate, pressure gradient, local wall shear stress and stream function distributions is evaluated in detail with the aid of graphs. The Newtonian fluid case is retrieved as a special case with vanishing couple stress effects. With increasing couple stress parameter there is a significant elevation in axial pressure gradient whereas the core axial velocity is reduced. An increase in electro-osmotic parameter induces both flow acceleration in the core region (around the channel centreline) and also enhances axial pressure gradient substantially. The study is relevant to simulation of novel smart bio-inspired space pumps, chromatography and medical microscale devices

First-order formalism for dark energy and dust

This work deals with first-order formalism for dark energy and dust in standard cosmology, for models described by real scalar field in the presence of dust in spatially flat space. The field dynamics may be standard or tachyonic, and we show how the equations of motion can be solved by first-order differential equations. We investigate a model to illustrate how the dustlike matter may affect the cosmic evolution using this framework.Comment: 5 pages, 1 figure; title changed, new author included, discussions extended, references added, version to appear in EPJ

Recommendations for reporting ion mobility Mass Spectrometry measurements

Here we present a guide to ion mobility mass spectrometry experiments, which covers both linear and nonlinear methods: what is measured, how the measurements are done, and how to report the results, including the uncertainties of mobility and collision cross section values. The guide aims to clarify some possibly confusing concepts, and the reporting recommendations should help researchers, authors and reviewers to contribute comprehensive reports, so that the ion mobility data can be reused more confidently. Starting from the concept of the definition of the measurand, we emphasize that (i) mobility values (K0) depend intrinsically on ion structure, the nature of the bath gas, temperature, and E/N; (ii) ion mobility does not measure molecular surfaces directly, but collision cross section (CCS) values are derived from mobility values using a physical model; (iii) methods relying on calibration are empirical (and thus may provide method‐dependent results) only if the gas nature, temperature or E/N cannot match those of the primary method. Our analysis highlights the urgency of a community effort toward establishing primary standards and reference materials for ion mobility, and provides recommendations to do so. © 2019 The Authors. Mass Spectrometry Reviews Published by Wiley Periodicals, Inc