5,155 research outputs found
Progress with the European Society for Paediatric Nephrology (ESPN)/ERA-EDTA Registry for children with established renal failure (ERF)
Weak Quasi-elastic Production of Hyperons
The quasielastic weak production of and hyperons from
nucleons and nuclei induced by antineutrinos is studied in the energy region of
some ongoing neutrino oscillation experiments in the intermediate energy
region. The hyperon nucleon transition form factors determined from neutrino
nucleon scattering and an analysis of high precision data on semileptonic
decays of neutron and hyperons using SU(3) symmetry have been used. The nuclear
effects due to Fermi motion and final state interaction effects due to hyperon
nucleon scattering have also been studied. The numerical results for
differential and total cross sections have been presented.Comment: 26 pages, 10 figure
On the universal X-ray luminosity function of binary X-ray sources in galaxies
The empirically determined universal power-law shape of X-ray luminosity
function of high mass X-ray binaries in galaxies is explained by fundamental
mass-luminosity and mass-radius relations for massive stars.Comment: 4 pages, plain LaTeX, no figures. Submitted to Astronomy Letter
Variance in Patient Access to Support Persons by Race/Ethnicity and Language Preference: An Analysis of Patient Survey Data
Regulatory and accreditation organizations have advocated open visitation policies and allowance of support persons of patientsâ choosing, but it is unknown if support is allowed equitably. Data from hospitalized patients were analyzed to determine access to support persons, stratified by patient-reported race/ethnicity, language, sex, age, and education. A multivariate regression model was constructed using race and language, controlling for site and patient sex, education and age. Additionally, sitesâ policies explicitly allowing support persons were correlated to reports of allowance of support persons. Among 1,196 respondents, 17% reported not being allowed a support person or being unsure. African American patients had 2.4 times greater odds of reporting non-allowance of support than their white counterparts, while speakers of a language other than English or Spanish had 3.9 times greater odds. There were no significant differences noted between sites with a policy allowing patient support persons and those with no policy or one in development. Most patients report being allowed a support person, but African Americans and those speaking a language other than English or Spanish have greater odds of reporting not being allowed a support person. Reliable methods of informing all patients of this right are needed
Spectral Energy Distributions of T Tauri and Herbig Ae Disks: Grain Mineralogy, Parameter Dependences, and Comparison with ISO LWS Observations
We improve upon the radiative, hydrostatic equilibrium models of passive
circumstellar disks constructed by Chiang & Goldreich (1997). New features
include (1) account for a range of particle sizes, (2) employment of
laboratory-based optical constants of representative grain materials, and (3)
numerical solution of the equations of radiative and hydrostatic equilibrium
within the original 2-layer (disk surface + disk interior) approximation. We
explore how the spectral energy distribution (SED) of a face-on disk depends on
grain size distributions, disk geometries and surface densities, and stellar
photospheric temperatures. Observed SEDs of 3 Herbig Ae and 2 T Tauri stars,
including spectra from the Long Wavelength Spectrometer (LWS) aboard the
Infrared Space Observatory (ISO), are fitted with our models. Silicate emission
bands from optically thin, superheated disk surface layers appear in nearly all
systems. Water ice emission bands appear in LWS spectra of 2 of the coolest
stars. Infrared excesses in several sources are consistent with vertical
settling of photospheric grains. While this work furnishes further evidence
that passive reprocessing of starlight by flared disks adequately explains the
origin of infrared-to-millimeter wavelength excesses of young stars, we
emphasize how the SED alone does not provide sufficient information to
constrain particle sizes and disk masses uniquely.Comment: Accepted to ApJ, 35 pages inc. 14 figures, AAS preprin
Collisionless Damping of Fast MHD Waves in Magneto-rotational Winds
We propose collisionless damping of fast MHD waves as an important mechanism
for the heating and acceleration of winds from rotating stars. Stellar rotation
causes magnetic field lines anchored at the surface to form a spiral pattern
and magneto-rotational winds can be driven. If the structure is a magnetically
dominated, fast MHD waves generated at the surface can propagate almost
radially outward and cross the field lines. The propagating waves undergo
collisionless damping owing to interactions with particles surfing on magnetic
mirrors that are formed by the waves themselves. The damping is especially
effective where the angle between the wave propagation and the field lines
becomes moderately large ( to ). The angle tends naturally
to increase into this range because the field in magneto-rotational winds
develops an increasingly large azimuthal component. The dissipation of the wave
energy produces heating and acceleration of the outflow. We show using
specified wind structures that this damping process can be important in both
solar-type stars and massive stars that have moderately large rotation rates.
This mechanism can play a role in coronae of young solar-type stars which are
rapidly rotating and show X-ray luminosities much larger than the sun. The
mechanism could also be important for producing the extended X-ray emitting
regions inferred to exist in massive stars of spectral type middle B and later.Comment: 12 pages, including 7 figures, accepted for publication in Ap
Next-to-leading order QCD corrections to Higgs boson production in association with a photon via weak-boson fusion at the LHC
Higgs boson production in association with a hard central photon and two
forward tagging jets is expected to provide valuable information on Higgs boson
couplings in a range where it is difficult to disentangle weak-boson fusion
processes from large QCD backgrounds. We present next-to-leading order QCD
corrections to Higgs production in association with a photon via weak-boson
fusion at a hadron collider in the form of a flexible parton-level Monte Carlo
program. The QCD corrections to integrated cross sections are found to be small
for experimentally relevant selection cuts, while the shape of kinematic
distributions can be distorted by up to 20% in some regions of phase space.
Residual scale uncertainties at next-to-leading order are at the few-percent
level.Comment: 17 pages, 7 figures, 1 tabl
Exploring alternative symmetry breaking mechanisms at the LHC with 7, 8 and 10 TeV total energy
In view of the annnouncement that in 2012 the LHC will run at 8 TeV, we study
the possibility of detecting signals of alternative mechanisms of ElectroWeak
Symmetry Breaking, described phenomenologically by unitarized models, at
energies lower than 14 TeV. A complete calculation with six fermions in the
final state is performed using the PHANTOM event generator. Our results
indicate that at 8 TeV some of the scenarios with TeV scale resonances are
likely to be identified while models with no resonances or with very heavy ones
will be inaccessible, unless the available luminosity will be much higher than
expected
Prediction of larynx function using multichannel surface EMG classification
Total laryngectomy (TL) affects critical functions such as swallowing, coughing and speaking. An artificial, bioengineered larynx (ABL), operated via myoelectric signals, may improve quality of life for TL patients. To evaluate the efficacy of using surface electromyography (sEMG) as a control signal to predict instances of swallowing, coughing and speaking, sEMG was recorded from submental, intercostal and diaphragm muscles. The cohort included TL and control participants. Swallowing, coughing, speaking and movement actions were recorded, and a range of classifiers were investigated for prediction of these actions. Our algorithm achieved F1-scores of 76.0 ± 4.4 % (swallows), 93.8 ± 2.8 % (coughs) and 70.5 ± 5.4 % (speech) for controls, and 67.7 ± 4.4 % (swallows), 71.0 ± 9.1 % (coughs) and 78.0 ± 3.8 % (speech) for TLs, using a random forest (RF) classifier. 75.1 ± 6.9 % of swallows were detected within 500 ms of onset in the controls, and 63.1 ± 6.1 % in TLs. sEMG can be used to predict critical larynx movements, although a viable ABL requires improvements. Results are particularly encouraging as they encompass a TL cohort. An ABL could alleviate many challenges faced by laryngectomees. This study represents a promising step toward realising such a device
MACHO 311.37557.169: A VY Scl star
Optical surveys, such as the MACHO project, often uncover variable stars
whose classification requires followup observations by other instruments. We
performed X-ray spectroscopy and photometry of the unusual variable star MACHO
311.37557.169 with \XMM\ in April 2018, supplemented by archival X-ray and
optical spectrographic data. The star has a bolometric X-ray luminosity of
about erg s cm and a heavily absorbed
two-temperature plasma spectrum. The shape of its light curve, its overall
brightness, its X-ray spectrum, and the emission lines in its optical spectrum
suggest that it is most likely a VY~Scl cataclysmic variable.Comment: 7 pages, 5 figure
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