191 research outputs found
Giant thermoemf in multiterminal superconductor/normal metal mesoscopic structures
We considered a mesoscopic superconductor/normal metal (S/N) structure in
which the N reservoirs are maintained at different temperatures. It is shown
that in the absence of current between the N reservoirs a voltage difference
arises between the superconducting and normal conductors. The voltage
oscillates with increasing phase difference between the
superconductors, and its magnitude does not depend on the small parameter
Comment: Resubmited, some changes to Text and Figure
Weak Charge Quantization on Superconducting Islands
We consider the Coulomb blockade on a superconductive quantum dot strongly
coupled to a lead through a tunnelling barrier and/or normal diffusive metal.
Andreev transport of the correlated pairs leads to quantum fluctuations of the
charge on the dot. These fluctuations result in exponential renormalization of
the effective charging energy. We employ two complimentary ways to approach the
problem, leading to the coinciding results: the instanton and the functional RG
treatment of the non-linear sigma model. We also derive the charging energy
renormalization in terms of arbitrary transmission matrix of the multi-channel
interface.Comment: 21 pages, 4 eps figures, RevTe
Service innovations: A depersonalisation research unit progress report
Depersonalisation was described clinically over 100 years ago, yet there has been little research into this interesting but distressing psychiatric disorder. The symptom of depersonalisation can occur alone or in the context of other psychiatric and neurological illnesses and is characterised by the experience of detachment from one's senses and the outside environment, and may be present for several years without remission. Two years after the establishment of the depersonalisation research unit at the Maudsley Hospital, London, we report on current neurobiological and clinical research findings, including functional magnetic resonance imaging, psychophysiology and neuroendocrinology and progress regarding the development of effective treatments
A Diagrammatic Theory of Random Scattering Matrices for Normal-Superconducting Mesoscopic Junctions
The planar-diagrammatic technique of large- random matrices is extended to
evaluate averages over the circular ensemble of unitary matrices. It is then
applied to study transport through a disordered metallic ``grain'', attached
through ideal leads to a normal electrode and to a superconducting electrode.
The latter enforces boundary conditions which coherently couple electrons and
holes at the Fermi energy through Andreev scattering. Consequently, the {\it
leading order} of the conductance is altered, and thus changes much larger than
are observed when, e.g., a weak magnetic field is applied. This is in
agreement with existing theories. The approach developed here is intermediate
between the theory of dirty superconductors (the Usadel equations) and the
random-matrix approach involving transmission eigenvalues (e.g. the DMPK
equation) in the following sense: even though one starts from a scattering
formalism, a quantity analogous to the superconducting order-parameter within
the system naturally arises. The method can be applied to a variety of
mesoscopic normal-superconducting structures, but for brevity we consider here
only the case of a simple disordered N-S junction.Comment: 39 pages + 9 postscript figure
Mapping social work across 10 countries: Structure, intervention, identity and challenges
An emerging global consciousness and rising attention given to international social work
development has seen the recognition of comparative research within the profession.
Understanding the functioning and organisation of social work within various country contexts
is critical in order to formulate knowledge around its overall impact, successes and challenges,
allowing social workers to learn from one another and build professional consolidation. The
profession is mapped out in 10 countries, reflecting on its structure, identity and development.
Although the profession is developing globally, it is also experiencing significant challenges. Key
insights, conclusions and recommendations for future research are presented
Layer-by-layer technique to developing functional nanolaminate films with antifungal activity
The layer-by-layer (LbL) deposition method was used to build up alternating layers (five) of different polyelectrolyte solutions (alginate, zein-carvacrol nanocapsules, chitosan and chitosan-carvacrol emulsions) on an aminolysed/charged polyethylene terephthalate (A/C PET) film. These nanolaminated films were characterised by contact angle measurements and through the determination of water vapour (WVTR) and oxygen (O2TR) transmission rates. The effect of active nanolaminated films against the Alternaria sp. and Rhizopus stolonifer was also evaluated. This procedure allowed developing optically transparent nanolaminated films with tuneable water vapour and gas properties and antifungal activity. The water and oxygen transmission rate values for the multilayer films were lower than those previously reported for the neat alginate or chitosan films. The presence of carvacrol and zein nanocapsules significantly decreased the water transmission rate (up to 40 %) of the nanolaminated films. However, the O2TR behaved differently and was only improved (up to 45 %) when carvacrol was encapsulated, i.e. nanolaminated films prepared by alternating alginate with nanocapsules of zein-carvacrol layers showed better oxygen barrier properties than those prepared as an emulsion of chitosan and carvacrol. These films containing zein-carvacrol nanocapsules also showed the highest antifungal activity (30 %), which did not significantly differ from those obtained with the highest amount of carvacrol, probably due to the controlled release of the active agent (carvacrol) from the zein-carvacrol nanocapsules. Thus, this work shows that nanolaminated films prepared with alternating layers of alginate and zein-carvacrol nanocapsules can be considered to improve the shelf-life of foodstuffs.The authors acknowledge financial support from
FP7 IP project BECOBIOCAP^. M. J. Fabra is recipients of a Juan de la
Cierva contract from the Spanish Ministry of Economy and
Competitivity. Maria L. Flores-López thanks Mexican Science and Technology
Council (CONACyT, Mexico) for PhD fellowship support
(CONACyT Grant Number 215499/310847). The author Miguel A.
Cerqueira is a recipient of a fellowship (SFRH/BPD/72753/2010) supported
by Fundação para a Ciência e Tecnologia, POPH-QREN and FSE
(FCT, Portugal). The authors also thank the FCT Strategic Project of UID/
BIO/04469/2013 unit, the project RECI/BBB-EBI/0179/2012 (FCOMP-
01-0124-FEDER-027462) and the project BBioInd - Biotechnology and
Bioengineering for improved Industrial and Agro-Food processes,^ REF.
NORTE-07-0124-FEDER-000028 Co-funded by the Programa
Operacional Regional do Norte (ON.2–O Novo Norte), QREN, FEDER.
The support of EU Cost Action FA0904 is gratefully acknowledged
Home-range and space use by Didelphis albiventris (Lund 1840) (Marsupialia, Didelphidae) in Mutum Island, Paraná river, Brazil
On the origin and evolution of the material in 67P/Churyumov-Gerasimenko
International audiencePrimitive objects like comets hold important information on the material that formed our solar system. Several comets have been visited by spacecraft and many more have been observed through Earth- and space-based telescopes. Still our understanding remains limited. Molecular abundances in comets have been shown to be similar to interstellar ices and thus indicate that common processes and conditions were involved in their formation. The samples returned by the Stardust mission to comet Wild 2 showed that the bulk refractory material was processed by high temperatures in the vicinity of the early sun. The recent Rosetta mission acquired a wealth of new data on the composition of comet 67P/Churyumov-Gerasimenko (hereafter 67P/C-G) and complemented earlier observations of other comets. The isotopic, elemental, and molecular abundances of the volatile, semi-volatile, and refractory phases brought many new insights into the origin and processing of the incorporated material. The emerging picture after Rosetta is that at least part of the volatile material was formed before the solar system and that cometary nuclei agglomerated over a wide range of heliocentric distances, different from where they are found today. Deviations from bulk solar system abundances indicate that the material was not fully homogenized at the location of comet formation, despite the radial mixing implied by the Stardust results. Post-formation evolution of the material might play an important role, which further complicates the picture. This paper discusses these major findings of the Rosetta mission with respect to the origin of the material and puts them in the context of what we know from other comets and solar system objects
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Gaia Early Data Release 3: The celestial reference frame (Gaia-CRF3)
Context. Gaia-CRF3 is the celestial reference frame for positions and proper motions in the third release of data from the Gaia mission, Gaia DR3 (and for the early third release, Gaia EDR3, which contains identical astrometric results). The reference frame is defined by the positions and proper motions at epoch 2016.0 for a specific set of extragalactic sources in the (E)DR3 catalogue. Aims. We describe the construction of Gaia-CRF3 and its properties in terms of the distributions in magnitude, colour, and astrometric quality. Methods. Compact extragalactic sources in Gaia DR3 were identified by positional cross-matching with 17 external catalogues of quasi-stellar objects (QSO) and active galactic nuclei (AGN), followed by astrometric filtering designed to remove stellar contaminants. Selecting a clean sample was favoured over including a higher number of extragalactic sources. For the final sample, the random and systematic errors in the proper motions are analysed, as well as the radio-optical offsets in position for sources in the third realisation of the International Celestial Reference Frame (ICRF3). Results. Gaia-CRF3 comprises about 1.6 million QSO-like sources, of which 1.2 million have five-parameter astrometric solutions in Gaia DR3 and 0.4 million have six-parameter solutions. The sources span the magnitude range G = 13-21 with a peak density at 20.6 mag, at which the typical positional uncertainty is about 1 mas. The proper motions show systematic errors on the level of 12 μas yr-1 on angular scales greater than 15 deg. For the 3142 optical counterparts of ICRF3 sources in the S/X frequency bands, the median offset from the radio positions is about 0.5 mas, but it exceeds 4 mas in either coordinate for 127 sources. We outline the future of Gaia-CRF in the next Gaia data releases. Appendices give further details on the external catalogues used, how to extract information about the Gaia-CRF3 sources, potential (Galactic) confusion sources, and the estimation of the spin and orientation of an astrometric solution
Model-independent measurement of mixing parameters in D → K ππ decays
The first model-independent measurement of the charm mixing parameters in the
decay is reported, using a sample of collision
data recorded by the LHCb experiment, corresponding to an integrated luminosity
of 1.0 fb at a centre-of-mass energy of 7 TeV. The measured values are
\begin{eqnarray*} x &=& (-0.86 \pm 0.53 \pm 0.17) \times 10^{-2}, \\ y &=&
(+0.03 \pm 0.46 \pm 0.13) \times 10^{-2}, \end{eqnarray*} where the first
uncertainties are statistical and include small contributions due to the
external input for the strong phase measured by the CLEO collaboration, and the
second uncertainties are systematic.Comment: 25 pages, 3 figures. Sign error in x fixed as of v2. All figures and
tables, along with any supplementary material and additional information, are
available at
https://lhcbproject.web.cern.ch/lhcbproject/Publications/LHCbProjectPublic/LHCb-PAPER-2015-042.htm
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