2,714 research outputs found
OSTEOARTHRITIC SUBCHONDRAL BONE MARROW HISTOLOGY. LESSONS FROM CHANGES IN ALKAPTONURIA
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Transmission of PhC coupled-resonator waveguide (PhCCRW) structure enhanced via mode matching
A method for increasing the coupling efficiency between ridge optical waveguides and PhCCRWs is described. This increase is achieved via W1 channel waveguide sections, formed within a two-dimensional triangular lattice photonic crystal using mode-matching. The mode-matching is achieved by low quality-factor modified cavities added to both the input and output ports of the PhCCRW. A three dimensional finite-difference time-domain method has been used to simulate light propagation through the modified PhCCRW. We have fabricated PhCCRWs working at 1.5Âľm in silicon-on-insulator material. Measurements and simulations show that the overall transmission is improved by a factor of two
Examining the Role of Environment in a Comprehensive Sample of Compact Groups
(Abridged) Compact groups, with their high number densities, small velocity
dispersions, and an interstellar medium that has not been fully processed,
provide a local analog to conditions of galaxy interactions in the earlier
universe. The frequent and prolonged gravitational encounters that occur in
compact groups affect the evolution of the constituent galaxies in a myriad of
ways, for example gas processing and star formation. Recently, a statistically
significant "gap" has been discovered mid-infrared IRAC colorspace of compact
group galaxies. This gap is not seen in field samples and is a new example of
how the compact group environment may affect the evolution of member galaxies.
In order to investigate the origin and nature of this gap, we have compiled a
sample of 49 compact groups. We find that a statistically significant deficit
of galaxies in this gap region of IRAC colorspace is persistant in this sample,
lending support to the hypothesis that the compact group environment inhibits
moderate SSFRs. We note a curvature in the colorspace distribution, which is
fully consistent with increasing dust temperature as the activity in a galaxy
increases. This full sample of 49 compact groups allows us to subdivide the
data according to physical properties of the groups. An analysis of these
subsamples indicates that neither projected physical diameter nor density show
a trend in colorspace within the values represented by this sample. We
hypothesize that the apparent lack of a trend is due to the relatively small
range of properties in this sample. Thus, the relative influence of stochastic
effects becomes dominant. We analyze spectral energy distributions of member
galaxies as a function of their location in colorspace and find that galaxies
in different regions of MIR colorspace contain dust with varying temperatures
and/or PAH emission.Comment: 24 pages, 13 figures. Accepted for publication in The Astronomical
Journa
Is psychotherapy for depression equally effective in younger and older adults? A meta-regression analysis.
Background: It is well established that psychotherapy is effective in the treatment of depression in younger as well as in older adults. Whether these psychotherapies are equally effective in younger and older age groups has not been examined in meta-analytic research. Methods: We conducted a systematic literature search and included 112 studies with 170 comparisons between a psychotherapy and a control group (with a total of 7,845 participants). Twenty studies with 26 comparisons were aimed at older adults. Results: We found no indication that psychotherapies were more or less effective for older adults compared to younger adults. The effect sizes of both groups of comparisons did not differ significantly from each other (older adults: d = 0.74; 95% CI: 0.49~0.99; younger adults: d = 0.67; 95% CI: 0.58~0.76). In a multivariate meta-regression analysis, in which we controlled for major characteristics of the participants, the interventions and the study designs, no indication of a difference between psychotherapy in younger and older adults was found. Conclusions: There appears to be no significant difference between psychotherapy in younger and older adults, although it is not clear whether this is also true for clinical samples, patients with more severe depression, and the older old
Growth and dislocation studies of β-HMX
Background: The defect structure of organic materials is important as it plays a major role in their crystal growth
properties. It also can play a subcritical role in âhot-spotâ detonation processes of energetics and one such
energetic is cyclotetramethylene-tetranitramine, in the commonly used beta form (β-HMX).
Results: The as-grown crystals grown by evaporation from acetone show prismatic, tabular and columnar habits, all
with {011}, {110}, (010) and (101) faces. Etching on (010) surfaces revealed three different types of etch pits, two of
which could be identified with either pure screw or pure edge dislocations, the third is shown to be an artifact of
the twinning process that this material undergoes. Examination of the {011} and {110} surfaces show only one type
of etch pit on each surface; however their natural asymmetry precludes the easy identification of their Burgers
vector or dislocation type. Etching of cleaved {011} surfaces demonstrates that the etch pits can be associated with
line dislocations. All dislocations appear randomly on the crystal surfaces and do not form alignments characteristic
of mechanical deformation by dislocation slip.
Conclusions: Crystals of β-HMX grown from acetone show good morphological agreement with that predicted by
modelling, with three distinct crystal habits observed depending upon the supersaturation of the growth solution.
Prismatic habit was favoured at low supersaturation, while tabular and columnar crystals were predominant at
higher super saturations. The twin plane in β-HMX was identified as a (101) reflection plane. The low plasticity of
β-HMX is shown by the lack of etch pit alignments corresponding to mechanically induced dislocation arrays.
On untwinned {010} faces, two types of dislocations exist, pure edge dislocations with b = [010] and pure screw
dislocations with b = [010]. On twinned (010) faces, a third dislocation type exists and it is proposed that these pits
are associated with pure screw dislocations with b = [010]
Fecal Enterobacteriales enrichment is associated with increased in vivo intestinal permeability in humans
Type 2 diabetes (T2D) has been linked with increased intestinal permeability, but the clinical significance of this phenomenon remains unknown. The objective of this study was to investigate the potential link between glucose control, intestinal permeability, diet and intestinal microbiota in patients with T2D. Thirtyâtwo males with wellâcontrolled T2D and 30 ageâmatched male controls without diabetes were enrolled in a caseâcontrol study. Metabolic parameters, inflammatory markers, endotoxemia, and intestinal microbiota in individuals subdivided into high (HP) and normal (LP) colonic permeability groups, were the main outcomes. In T2D, the HP group had significantly higher fasting glucose (P = 0.034) and plasma nonesterified fatty acid levels (P = 0.049) compared with the LP group. Increased colonic permeability was also linked with altered abundances of selected microbial taxa. The microbiota of both T2D and control HP groups was enriched with Enterobacteriales. In conclusion, high intestinal permeability was associated with poorer fasting glucose control in T2D patients and changes in some microbial taxa in both T2D patients and nondiabetic controls. Therefore, enrichment in the gramânegative order Enterobacteriales may characterize impaired colonic permeability prior to/independently from a disruption in glucose tolerance
Mid-Infrared Evidence for Accelerated Evolution in Compact Group Galaxies
We find evidence for accelerated evolution in compact group galaxies from the
distribution in mid-infrared colorspace of 42 galaxies from 12 Hickson Compact
Groups (HCGs) compared to the the distributions of several other samples
including the LVL+SINGS galaxies, interacting galaxies, and galaxies from the
Coma Cluster. We find that the HCG galaxies are not uniformly distributed in
colorspace, as well as quantitative evidence for a gap. Galaxies in the infall
region of the Coma cluster also exhibit a non-uniform distribution and a less
well defined gap, which may reflect a similarity with the compact group
environment. Neither the Coma Center or interacting samples show evidence of a
gap, leading us to speculate that the gap is unique to the environment of high
galaxy density where gas has not been fully processed or stripped.Comment: To appear in the Proceedings of the Galaxy Wars: Stellar Populations
and Star Formation in Interacting Galaxies Conferenc
High Prevalence of False Chordae Tendinae in Patients Without Left Ventricular Tachycardia
Peer Reviewedhttp://deepblue.lib.umich.edu/bitstream/2027.42/74774/1/j.1540-8159.2007.00628.x.pd
Close to Uniform Prime Number Generation With Fewer Random Bits
In this paper, we analyze several variants of a simple method for generating
prime numbers with fewer random bits. To generate a prime less than ,
the basic idea is to fix a constant , pick a
uniformly random coprime to , and choose of the form ,
where only is updated if the primality test fails. We prove that variants
of this approach provide prime generation algorithms requiring few random bits
and whose output distribution is close to uniform, under less and less
expensive assumptions: first a relatively strong conjecture by H.L. Montgomery,
made precise by Friedlander and Granville; then the Extended Riemann
Hypothesis; and finally fully unconditionally using the
Barban-Davenport-Halberstam theorem. We argue that this approach has a number
of desirable properties compared to previous algorithms.Comment: Full version of ICALP 2014 paper. Alternate version of IACR ePrint
Report 2011/48
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