332 research outputs found
Non-gapped Fermi surfaces, quasiparticles and the anomalous temperature dependence of the near- electronic states in the CMR oxide LaSrMnO with
After years of research into colossal magnetoresistant (CMR) manganites using
bulk techniques, there has been a recent upsurge in experiments directly
probing the electronic states at or near the surface of the bilayer CMR
materials LaSrMnO using angle-resolved photoemission
or scanning probe microscopy. Here we report new, temperature dependent, angle
resolved photoemission data from single crystals with a doping level of
. The first important result is that there is no sign of a pseudogap in
the charge channel of this material for temperatures below the Curie
temperature . The second important result concerns the temperature
dependence of the electronic states. The temperature dependent changes in the
Fermi surface spectra both at the zone face and zone diagonal regions in
-space indicate that the coherent quasiparticle weight disappears for
temperatures significantly above , and that the -dependence of the
T-induced changes in the spectra invalidate an interpretation of these data in
terms of the superposition of a `universal' metallic spectrum and an insulating
spectrum whose relative weight changes with temperature. In this sense, our
data are not compatible with a phase separation scenario.Comment: 6 pages, 4 figure
Heritable functional architecture in human visual cortex
How much of the functional organization of our visual system is inherited? Here we tested the heritability of retinotopic maps in human visual cortex using functional magnetic resonance imaging. We demonstrate that retinotopic organization shows a closer correspondence in monozygotic (MZ) compared to dizygotic (DZ) twin pairs, suggesting a partial genetic determination. Using population receptive field (pRF) analysis to examine the preferred spatial location and selectivity of these neuronal populations, we estimate a heritability around 10â20% for polar angle preferences and spatial selectivity, as quantified by pRF size, in extrastriate areas V2 and V3. Our findings are consistent with heritability in both the macroscopic arrangement of visual regions and stimulus tuning properties of visual cortex. This could constitute a neural substrate for variations in a range of perceptual effects, which themselves have been found to be at least partially genetically determined. These findings also add convergent evidence for the hypothesis that functional map topology is linked with cortical morphology
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Queues don't matter when you can JUMP them!
QJUMP is a simple and immediately deployable approach
to controlling network interference in datacenter
networks. Network interference occurs when congestion
from throughput-intensive applications causes queueing
that delays traffic from latency-sensitive applications.
To mitigate network interference, QJUMP applies Internet
QoS-inspired techniques to datacenter applications.
Each application is assigned to a latency sensitivity level
(or class). Packets from higher levels are rate-limited
in the end host, but once allowed into the network can
âjump-the-queueâ over packets from lower levels. In settings
with known node counts and link speeds, QJUMP
can support service levels ranging from strictly bounded
latency (but with low rate) through to line-rate throughput
(but with high latency variance).
We have implemented QJUMP as a Linux Traffic Control
module. We show that QJUMP achieves bounded
latency and reduces in-network interference by up to
300Ă, outperforming Ethernet Flow Control (802.3x),
ECN (WRED) and DCTCP. We also show that QJUMP
improves average flow completion times, performing
close to or better than DCTCP and pFabric.This work was supported
by a Google Fellowship, EPSRC INTERNET Project
EP/H040536/1, Defense Advanced Research Projects
Agency (DARPA) and Air Force Research Laboratory
(AFRL), under contract FA8750-11-C-0249.This is the final published version. It first appeared at https://www.usenix.org/conference/nsdi15/technical-sessions/presentation/grosvenor
Extrastriate projections in human visual system: Evidence from fMRI-informed tractography
The human optic radiation (OR) is the main pathway for conveying visual input to occipital cortex, but it is unclear whether it projects beyond primary visual cortex (V1). In this study, we used functional MRI mapping to delineate early visual areas in 30 healthy volunteers and determined the termination area of the OR as reconstructed with diffusion tractography. Direct thalamo-cortical projections to areas V2 and V3 were found in all hemispheres tested, with a distinct anatomical arrangement of superiorâinferior fiber placement for dorsal and ventral projections, respectively, and a medio-lateral nesting arrangement for projections to V1, V2 and V3. Finally, segment-specific microstructure was examined, revealing sub-fascicular information. This is to date the first in vivo demonstration of direct extrastriate projections of the OR in humans
Can environmental DNA be used to detect first arrivals of the cane toad, Rhinella marina, into novel locations?
Eradicating invasive species is difficult, but success is more likely when populations are small after arrival. The cane toad, Rhinella marina, is an invasive pest species that threatens native fauna worldwide. Increasingly, environmental DNA (eDNA) is used as a technique to monitor the presence of invasive species given its power to detect low numbers of individuals. We aimed to investigate eDNA persistence in freshwater at three different temperatures (25, 30 and 35°C) and eDNA detection thresholds for R. marina using controlled experiments in aquaria. For the latter, two water volumes and two cane toad exposure times were used (800 or 200 L volume with 5 or 30 min exposure). A 15âml water sample was collected from each replicated aquaria and preserved with 5 ml Longmire's buffer. Environmental DNA was extracted and four technical quantitative PCR replicates were analyzed targeting the cane toad 16S rDNA mitochondrial gene. Environmental DNA decayed rapidly in water and was reliably detected for up to 3 days after cane toad removal, regardless of the temperature treatment. Also, cane toad eDNA was detected in the water after a 5âmin initial exposure of a single individual in 800 L of water. Under the physical parameters tested here, a positive detection means that a cane toad has been in contact with the water body between 1 and 3 days prior to the sampling event. The results of the present study show the importance of eDNA for determining the presence of a species that occurs at low abundance in a small water body, such as at the onset of a cane toad invasion
Condensation in randomly perturbed zero-range processes
The zero-range process is a stochastic interacting particle system that
exhibits a condensation transition under certain conditions on the dynamics. It
has recently been found that a small perturbation of a generic class of jump
rates leads to a drastic change of the phase diagram and prevents condensation
in an extended parameter range. We complement this study with rigorous results
on a finite critical density and quenched free energy in the thermodynamic
limit, as well as quantitative heuristic results for small and large noise
which are supported by detailed simulation data. While our new results support
the initial findings, they also shed new light on the actual (limited)
relevance in large finite systems, which we discuss via fundamental diagrams
obtained from exact numerics for finite systems.Comment: 18 pages, 6 figure
Corrosion studies on selected packaging materials for disposal of heat-generating radioactive wastes in rock-salt formations
Neutral Hydrogen and Optical Observations of Edge-on Galaxies: Hunting for Warps
We present 21-cm HI line and optical R-band observations for a sample of 26
edge-on galaxies. The HI observations were obtained with the Westerbork
Synthesis Radio Telescope, and are part of the WHISP database (Westerbork HI
Survey of Spiral and Irregular Galaxies). We present HI maps, optical images,
and radial HI density profiles. We have also derived the rotation curves and
studied the warping and lopsidedness of the HI disks.
20 out of the 26 galaxies of our sample are warped, confirming that warping
of the HI disks is a very common phenomenon in disk galaxies. Indeed, we find
that all galaxies that have an extended HI disk with respect to the optical are
warped.
The warping usually starts around the edge of the optical disk. The degree of
warping varies considerably from galaxy to galaxy. Furthermore, many warps are
asymmetric, as they show up in only one side of the disk or exhibit large
differences in amplitude in the approaching and receding sides of the galaxy.
These asymmetries are more pronounced in rich environments, which may indicate
that tidal interactions are a source of warp asymmetry. A rich environment
tends to produce larger warps as well. The presence of lopsidedness seems to be
related to the presence of nearby companions.Comment: To appear in Astronomy & Astrophysic
Work restructuring and changing craft identity: the Tale of the Disaffected Weavers (or what happens when the rug is pulled from under your feet)
This article explores the changes in worker identity that can occur during manufacturing restructuring â specifically those linked to the declining status of craft work â through an in-depth case study of Weaveco, a UK carpet manufacturer. An analysis of changes in the labour process is followed by employee reactions centred on the demise of the traditional craft identity of male carpet weavers. The voices of the weavers dramatize the tensions involved in reconstructing their masculine identity, and we consider the implications this has for understanding gendered work relations
Signatures of SN Ia in the galactic thick disk
We present the first results of a larger study into the stellar abundances
and chemical trends in long-lived dwarf stars in the solar neighbourhood that
belong to (based on their kinematics) the thin and thick galactic disk,
respectively. We confirm that the trends of alpha-elements in the thin and
thick disk are distinct (this has previously been shown for Mg by Fuhrmann
1998, but e.g. Chen et al. 2000 claimed the trends to follow smoothly upon each
other). We find that the thick disk show the typical signature of contribution
from SN Ia (i.e. the ``knee'') to the enrichment of the interstellar gas out of
which the later generations of thick disk stars formed. The trend starts out as
[Mg/Fe] ~0.35 at [Fe/H] ~ -0.7 and continue on this level with increasing
[Fe/H] until -0.4 dex where a decline in [Mg/Fe] starts and steadily continues
down to 0 dex at solar metallicity. The same is true for the other
alpha-elements (e.g. Si). Using ages from the literature we find that the thick
disk in the mean is older than the thin disk. Combining our results with other
observational facts we suggest that the most likely formation scenario for the
thick disk is, still, a violent merger event. We also suggest that there might
be tentativeevidence for diffusion of orbits in todays thin disk (based on
kinematics in combination with elemental abundances).Comment: 4 pages, 3 figures, A&A Letter in pres
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