10,156 research outputs found
OBSTACLES TO SUCCESS IN THE WORKPLACE FOR PEOPLE WITH DISABILITIES: A REVIEW AND RESEARCH AGENDA
Our objectives in this paper were to summarize research relevant to obstacles that people with disabilities (PWD) face in the workplace and to identify directions for future research on the topic. We included review, theoretical, and empirical articles in mainstream management journals and those in psychology or rehabilitation journals if they had clear workplace implications. We argue that obstacles identified in prior research may only partially reflect organizational reality. This is because of the heavy reliance on laboratory studies, which we urge researchers to replicate in organizational settings. Better understanding of obstacles will lead to more evidence-based solutions where the payoff is a less exclusionary world in which more individuals are provided opportunities to use their talent for the benefit of all. .Disability, Workplace obstacles, Review
Prediction of biopore- and matrix-dominated flow from X-ray CT-derived macropore network characteristics
Peer reviewedPublisher PD
Bimodal distribution of the autocorrelation function in gamma-ray bursts
Autocorrelation functions (ACFs) are studied for a sample of 16 long
gamma-ray bursts (GRBs) with known redshift z, that were observed by the BATSE
and Konus experiments. When corrected for cosmic time dilation, the ACF shows a
bimodal distribution. A narrow width class (11 bursts) has at half-maximum a
mean width of 1.6 s with a relative dispersion of 32%, while a broad width
class (5 bursts) has a width of 7.5 s with a 4% dispersion. The separation
between the two mean values is highly significant (> 7 standard deviations).
This temporal property could be used on the large existing database of GRBs
with unknown redshift. The broad width set shows a very good linear correlation
between width at half-maximum and (1+z), with a correlation coefficient R=0.995
and a probability of chance alignment <0.0004. The potential application of
this correlation to cosmology studies is discussed, using it in combination
with recently proposed luminosity indicators.Comment: 7 pages, 7 figures. Accepted for publication in A&
The Non-Relativistic Evolution of GRBs 980703 and 970508: Beaming-Independent Calorimetry
We use the Sedov-Taylor self-similar solution to model the radio emission
from the gamma-ray bursts (GRBs) 980703 and 970508, when the blastwave has
decelerated to non-relativistic velocities. This approach allows us to infer
the energy independent of jet collimation. We find that for GRB 980703 the
kinetic energy at the time of the transition to non-relativistic evolution,
t_NR ~ 40 d, is E_ST ~ (1-6)e51 erg. For GRB 970508 we find E_ST ~ 3e51 erg at
t_NR ~ 100 d, nearly an order of magnitude higher than the energy derived in
Frail, Waxman and Kulkarni (2000). This is due primarily to revised
cosmological parameters and partly to the maximum likelihood fit we use here.
Taking into account radiative losses prior to t_NR, the inferred energies agree
well with those derived from the early, relativistic evolution of the
afterglow. Thus, the analysis presented here provides a robust,
geometry-independent confirmation that the energy scale of cosmological GRBs is
about 5e51 erg, and additionally shows that the central engine in these two
bursts did not produce a significant amount of energy in mildly relativistic
ejecta at late time. Furthermore, a comparison to the prompt energy release
reveals a wide dispersion in the gamma-ray efficiency, strengthening our
growing understanding that E_gamma is a not a reliable proxy for the total
energy.Comment: Submitted to ApJ; 13 pages, 6 figures, 1 table; high-resolution
figures can be found at: http://www.astro.caltech.edu/~ejb/NR
Atomic data for S II - Toward Better Diagnostics of Chemical Evolution in High-redshift Galaxies
Absorption-line spectroscopy is a powerful tool used to estimate element
abundances in the nearby as well as distant universe. The accuracy of the
abundances thus derived is, naturally, limited by the accuracy of the atomic
data assumed for the spectral lines. We have recently started a project to
perform the new extensive atomic data calculations used for optical/UV spectral
lines in the plasma modeling code Cloudy using state-of-the-art quantal
calculations. Here we demonstrate our approach by focussing on S II, an ion
used to estimate metallicities for Milky Way interstellar clouds as well as
distant damped Lyman-alpha (DLA) and sub-DLA absorber galaxies detected in the
spectra of quasars and gamma-ray bursts (GRBs). We report new extensive
calculations of a large number of energy levels of S II, and the line strengths
of the resulting radiative transitions. Our calculations are based on the
configuration interaction approach within a numerical Hartree-Fock framework,
and utilize both non-ralativistic and quasirelativistic one-electron radial
orbitals. The results of these new atomic calculations are then incorporated
into Cloudy and applied to a lab plasma, and a typical DLA, for illustrative
purposes. The new results imply relatively modest changes (~0.04 dex) to the
metallicities estimated from S II in past studies. These results will be
readily applicable to other studies of S II in the Milky Way and other
galaxies.Comment: Accepted for publication in The Astrophysical Journal; 34 pages, 10
figure
Simulations of Oligomeric Intermediates in Prion Diseases
We extend our previous stochastic cellular automata based model for areal
aggregation of prion proteins on neuronal surfaces. The new anisotropic model
allow us to simulate both strong beta-sheet and weaker attachment bonds between
proteins. Constraining binding directions allows us to generate aggregate
structures with the hexagonal lattice symmetry found in recently observed in
vitro experiments. We argue that these constraints on rules may correspond to
underlying steric constraints on the aggregation process. We find that monomer
dominated growth of the areal aggregate is too slow to account for some
observed doubling time-to-incubation time ratios inferred from data, and so
consider aggregation dominated by relatively stable but non-infectious
oligomeric intermediates. We compare a kinetic theory analysis of oligomeric
aggregation to spatially explicit simulations of the process. We find that with
suitable rules for misfolding of oligomers, possibly due to water exclusion by
the surrounding aggregate, the resulting oligomeric aggregation model maps onto
our previous monomer aggregation model. Therefore it can produce some of the
same attractive features for the description of prion incubation time data. We
propose experiments to test the oligomeric aggregation model.Comment: 8 pages, 10 figures For larger versions of several figures, see
http://asaph.ucdavis.edu/~dmobley and click on the prion paper lin
Atomic data for Zn II - Improving Spectral Diagnostics of Chemical Evolution in High-redshift Galaxies
Damped Lyman-alpha (DLA) and sub-DLA absorbers in quasar spectra provide the
most sensitive tools for measuring element abundances of distant galaxies.
Estimation of abundances from absorption lines depends sensitively on the
accuracy of the atomic data used. We have started a project to produce new
atomic spectroscopic parameters for optical/UV spectral lines using
state-of-the-art computer codes employing very broad configuration interaction
basis. Here we report our results for Zn II, an ion used widely in studies of
the interstellar medium (ISM) as well as DLA/sub-DLAs. We report new
calculations of many energy levels of Zn II, and the line strengths of the
resulting radiative transitions. Our calculations use the configuration
interaction approach within a numerical Hartree-Fock framework. We use both
non-relativistic and quasi-relativistic one-electron radial orbitals. We have
incorporated the results of these atomic calculations into the plasma
simulation code Cloudy, and applied them to a lab plasma and examples of a DLA
and a sub-DLA. Our values of the Zn II {\lambda}{\lambda} 2026, 2062 oscillator
strengths are higher than previous values by 0.10 dex. Cloudy calculations for
representative absorbers with the revised Zn atomic data imply ionization
corrections lower than calculated before by 0.05 dex. The new results imply Zn
metallicities should be lower by 0.1 dex for DLAs and by 0.13-0.15 dex for
sub-DLAs than in past studies. Our results can be applied to other studies of
Zn II in the Galactic and extragalactic ISM.Comment: accepted The Astrophysical Journa
Novel Design of VCO with Output Peak to Peak Control
Voltage controlled oscillator is widely used in many electronics devices. It is used to generate the signals for broadcast by radio and television transmitters, clock signals that regulate computers and quartz clocks, and the sounds produced by electronic beepers and video games. In this paper we propose a novel way to modify the existing VCO and provide an enhancement to control the output voltage level which can be used in any application of varying required voltage level. The simulation is done using tanner using 250nm dimension
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