1,053 research outputs found

    Apparent equilibrium shifts and hot-spot formation for catalytic reactions induced by microwave dielectric heating

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    Microwave dielectric heating of the gas phase decomposition of H2S catalysed by metal sulfides on a -Al2O3 support results in significant apparent shifts in the equilibrium constant, which have been attributed to the development of hot-spots in the catalytic beds; X-ray diffraction and electron microscopy measurements have indicated the formation of hot-spots with dimensions of 90–1000 µm and which involve not only the active phase, but also the support

    Toward the synthesis of an acetal-free Tn antigen anti-cancer vaccine candidate

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    Cancer vaccines are a promising approach to cancer treatment by activating the immune system towards cancer cells. The challenge, however, comes with the identification of biomarkers correlated with cancer. Unfortunately, many oncotargets are simply upregulated in cancer; these are inappropriate vaccine targets as they are also present on healthy cells and therefore would ultimately initiate a very dangerous systemic immune response. In contrast, Tumor-Associated Carbohydrate Antigens (TACAs) are not found in healthy adult tissue but are found on over 90% of biopsied carcinomas. When incorporated into glycopeptides or other immunogenic scaffolds, these carbohydrate antigens have formed the basis of the development of anti-tumor immunotherapies through the induction of a specific immune response against cancer cells. However, despite promising preliminary data, none of these candidates have reached the clinic. Our hypothesis is that the carbohydrates on the vaccines may not survive antigen processing, and so more stable versions of these materials are required to create viable vaccines. Our approach is to incorporate TACAs lacking the labile glycosidic bond: acetal-free carbohydrates (AFCs). This project aims to remove the unstable acetal functional group to yield a more robust carbohydrate structure that can then be incorporated into a vaccine candidate. In this presentation, two synthetic pathways will be described: conversion of a carbohydrate to a carbasugar through a rearrangement, and de novo synthesis from noncarbohydrate materials

    SIDM on FIRE: Hydrodynamical Self-Interacting Dark Matter simulations of low-mass dwarf galaxies

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    We compare a suite of four simulated dwarf galaxies formed in 1010M^{10} M_{\odot} haloes of collisionless Cold Dark Matter (CDM) with galaxies simulated in the same haloes with an identical galaxy formation model but a non-zero cross-section for dark matter self-interactions. These cosmological zoom-in simulations are part of the Feedback In Realistic Environments (FIRE) project and utilize the FIRE-2 model for hydrodynamics and galaxy formation physics. We find the stellar masses of the galaxies formed in Self-Interacting Dark Matter (SIDM) with σ/m=1cm2/g\sigma/m= 1\, cm^2/g are very similar to those in CDM (spanning M105.77.0MM_{\star} \approx 10^{5.7 - 7.0} M_{\odot}) and all runs lie on a similar stellar mass -- size relation. The logarithmic dark matter density slope (α=dlogρ/dlogr\alpha=d\log \rho / d\log r) in the central 250500250-500 pc remains steeper than α=0.8\alpha= -0.8 for the CDM-Hydro simulations with stellar mass M106.6MM_{\star} \sim 10^{6.6} M_{\odot} and core-like in the most massive galaxy. In contrast, every SIDM hydrodynamic simulation yields a flatter profile, with α>0.4\alpha >-0.4. Moreover, the central density profiles predicted in SIDM runs without baryons are similar to the SIDM runs that include FIRE-2 baryonic physics. Thus, SIDM appears to be much more robust to the inclusion of (potentially uncertain) baryonic physics than CDM on this mass scale, suggesting SIDM will be easier to falsify than CDM using low-mass galaxies. Our FIRE simulations predict that galaxies less massive than M<3×106MM_{\star} < 3 \times 10^6 M_{\odot} provide potentially ideal targets for discriminating models, with SIDM producing substantial cores in such tiny galaxies and CDM producing cusps.Comment: 10 Pages, 7 figures, submitted to MNRA

    Bibliografía

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    Reaction of the anion-deficient, cation-ordered perovskite phase Ba<sub>2</sub>YFeO<sub>5</sub> with 80 atm of oxygen pressure at 410 °C results in the formation of the Fe<sup>4+</sup> phase Ba<sub>2</sub>YFeO<sub>5.5</sub>. The topochemical insertion of oxide ions lifts the inversion symmetry of the centrosymmetric host phase, Ba<sub>2</sub>YFeO<sub>5</sub> (space group <i>P</i>2<sub>1</sub>/<i>n</i>), to yield a noncentrosymmetric (NCS) phase Ba<sub>2</sub>YFeO<sub>5.5</sub> (space group <i>Pb</i>2<sub>1</sub><i>m</i> (No. 26), <i>a</i> = 12.1320(2) Å, <i>b</i> = 6.0606(1) Å, <i>c</i> = 8.0956(1) Å, <i>V</i> = 595.257(2) Å<sup>3</sup>) confirmed by the observation of second-harmonic generation. Dielectric and PUND ferroelectric measurements, however, show no evidence for a switchable ferroelectric polarization, limiting the material to pyroelectric behavior. Magnetization and low-temperature neutron diffraction data indicate that Ba<sub>2</sub>YFeO<sub>5.5</sub> undergoes a magnetic transition at 20 K to adopt a state which exhibits a combination of ferromagnetic and antiferromagnetic order. The symmetry breaking from centrosymmetric to polar noncentrosymmetric, which occurs during the topochemical oxidation process is discussed on the basis of induced lattice strain and an electronic instability and represents a new strategy for the preparation of NCS materials that readily incorporate paramagnetic transition metal centers

    Quantity, composition, and source of sediment collected in sediment traps along the fringing coral reef off Molokai, Hawaii

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    This paper is not subject to U.S. copyright. The definitive version was published in Marine Pollution Bulletin 52 (2006): 1034-1047, doi:10.1016/j.marpolbul.2006.01.008.Sediment traps were used to evaluate the frequency, cause, and relative intensity of sediment mobility/resuspension along the fringing coral reef off southern Molokai (February 2000–May 2002). Two storms with high rainfall, floods, and exceptionally high waves resulted in sediment collection rates > 1000 times higher than during non-storm periods, primarily because of sediment resuspension by waves. Based on quantity and composition of trapped sediment, floods recharged the reef flat with land-derived sediment, but had a low potential for burying coral on the fore reef when accompanied by high waves. The trapped sediments have low concentrations of anthropogenic metals. The magnetic properties of trapped sediment may provide information about the sources of land-derived sediment reaching the fore reef. The high trapping rate and low sediment cover indicate that coral surfaces on the fore reef are exposed to transient resuspended sediment, and that the traps do not measure net sediment accumulation on the reef surface

    ᴅ-Mannose for prevention of recurrent urinary tract infection among women: a randomized clinical trial

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    Importance: Recurrent urinary tract infection (UTI) is a common debilitating condition in women, with limited prophylactic options. d-Mannose has shown promise in trials based in secondary care, but effectiveness in placebo-controlled studies and community settings has not been established. Objective: To determine whether d-mannose taken for 6 months reduces the proportion of women with recurrent UTI experiencing a medically attended UTI. Design, Setting, and Participants: This 2-group, double-blind randomized placebo-controlled trial took place across 99 primary care centers in the UK. Participants were recruited between March 28, 2019, and January 31, 2020, with 6 months of follow-up. Participants were female, 18 years or older, living in the community, and had evidence in their primary care record of consultations for at least 2 UTIs in the preceding 6 months or 3 UTIs in 12 months. Invitation to participate was made by their primary care center. A total of 7591 participants were approached, 830 responded, and 232 were ineligible or did not proceed to randomization. Statistical analysis was reported in December 2022. Intervention: Two grams daily of d-mannose powder or matched volume of placebo powder. Main Outcomes and Measures: The primary outcome measure was the proportion of women experiencing at least 1 further episode of clinically suspected UTI for which they contacted ambulatory care within 6 months of study entry. Secondary outcomes included symptom duration, antibiotic use, time to next medically attended UTI, number of suspected UTIs, and UTI-related hospital admissions. Results: Of 598 women eligible (mean [range] age, 58 [18-93] years), 303 were randomized to d-mannose (50.7%) and 295 to placebo (49.3%). Primary outcome data were available for 583 participants (97.5%). The proportion contacting ambulatory care with a clinically suspected UTI was 150 of 294 (51.0%) in the d-mannose group and 161 of 289 (55.7%) in the placebo group (risk difference, −5%; 95% CI, −13% to 3%; P = .26). Estimates were similar in per protocol analyses, imputation analyses, and preplanned subgroups. There were no statistically significant differences in any secondary outcome measures. Conclusions and Relevance: In this randomized clinical trial, daily d-mannose did not reduce the proportion of women with recurrent UTI in primary care who experienced a subsequent clinically suspected UTI. d-Mannose should not be recommended for prophylaxis in this patient group. Trial Registration: isrctn.org Identifier: ISRCTN1328351

    Type II Critical Collapse of a Self-Gravitating Nonlinear σ\sigma-Model

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    We report on the existence and phenomenology of type II critical collapse within the one-parameter family of SU(2) σ\sigma-models coupled to gravity. Numerical investigations in spherical symmetry show discretely self-similar (DSS) behavior at the threshold of black hole formation for values of the dimensionless coupling constant \ccbeta ranging from 0.2 to 100; at 0.18 we see small deviations from DSS. While the echoing period Δ\Delta of the critical solution rises sharply towards the lower limit of this range, the characteristic mass scaling has a critical exponent γ\gamma which is almost independent of \ccbeta, asymptoting to 0.1185±0.00050.1185 \pm 0.0005 at large \ccbeta. We also find critical scaling of the scalar curvature for near-critical initial data. Our numerical results are based on an outgoing-null-cone formulation of the Einstein-matter equations, specialized to spherical symmetry. Our numerically computed initial-data critical parameters pp^* show 2nd order convergence with the grid resolution, and after compensating for this variation in pp^*, our individual evolutions are uniformly 2nd order convergent even very close to criticality.Comment: 23 pages, includes 10 postscript figure files, uses REVTeX, epsf, psfrag, and AMS math fonts (amstex + amssymb); to appear in PRD15. Summary of revisions from v2: fix wrong formula in figure 6 caption and y-axis label, also minor wording changes and update publication status of refs 5-
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