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Influence of water on tribolayer growth when lubricating steel with a fluorinated phosphonium dicyanamide ionic liquid
This work aims to elucidate the role of environmental humidity on the tribological behavior of steel surfaces lubricated with an ionic liquid comprised of a fluorinated phosphonium cation-tributyl-3,3,4,4,5,5,6,6,7,7,8,8,8-tridecafluoro-octyl-phosphonium-and a dicyanamide anion (i.e. N(CN) 2 - ). Ball-on-disk tribotests were carried out at room temperature and at various levels of relative humidity (RH). Water was found to be required to promote the formation of a tribofilm over the contact area. The reaction layer exhibited a patchy morphology, which resembles that observed formed with conventional antiwear additives such as ZnDTP. A surface-chemical analysis of the tribofilm indicated that the tribofilm is composed of fluorides, oxides, and phosphates, pointing to a stress-induced degradation of the ions and corrosion of the sliding counterparts, which is enabled by the presence of water at the sliding interface. © 2019 by the authors
Financial impact of breast cancer in black versus white women
Purpose Racial variation in the financial impact of cancer may contribute to observed differences in the use of guideline-recommended treatments. We describe racial differences with regard to the financial impact of breast cancer in a large population-based prospective cohort study. Methods The Carolina Breast Cancer Study oversampled black women and women younger than age 50 years with incident breast cancer in North Carolina from 2008 to 2013. Participants provided medical records and data regarding demographics, socioeconomic status, and financial impact of cancer at 5 and 25 months postdiagnosis. We report unadjusted and adjusted financial impact at 25 months postdiagnosis by race. Results The sample included 2,494 women who completed follow-up surveys (49% black, 51% white). Since diagnosis, 58% of black women reported any adverse financial impact of cancer (v 39% of white women; P, .001). In models adjusted for age, stage at diagnosis, and treatment received, black women were more likely to report adverse financial impact attributable to cancer (adjusted risk difference [aRD], +14 percentage points; P, .001), including income loss (aRD, +10 percentage points; P, .001), health care–related financial barriers (aRD, +10 percentage points; P, .001), health care–related transportation barriers (aRD, +10 percentage points; P, .001), job loss (aRD, 6 percentage points; P, .001), and loss of health insurance (aRD, +3 percentage points; P, .001). The effect of race was attenuated when socioeconomic factors were included but remained significant for job loss, transportation barriers, income loss, and overall financial impact. Conclusion Compared with white women, black women with breast cancer experience a significantly worse financial impact. Disproportionate financial strain may contribute to higher stress, lower treatment compliance, and worse outcomes by race. Policies that help to limit the effect of cancer-related financial strain are needed
Saturn's icy satellites and rings investigated by Cassini - VIMS. III. Radial compositional variability
In the last few years Cassini-VIMS, the Visible and Infared Mapping
Spectrometer, returned to us a comprehensive view of the Saturn's icy
satellites and rings. After having analyzed the satellites' spectral properties
(Filacchione et al. (2007a)) and their distribution across the satellites'
hemispheres (Filacchione et al. (2010)), we proceed in this paper to
investigate the radial variability of icy satellites (principal and minor) and
main rings average spectral properties. This analysis is done by using 2,264
disk-integrated observations of the satellites and a 12x700 pixels-wide rings
radial mosaic acquired with a spatial resolution of about 125 km/pixel. The
comparative analysis of these data allows us to retrieve the amount of both
water ice and red contaminant materials distributed across Saturn's system and
the typical surface regolith grain sizes. These measurements highlight very
striking differences in the population here analyzed, which vary from the
almost uncontaminated and water ice-rich surfaces of Enceladus and Calypso to
the metal/organic-rich and red surfaces of Iapetus' leading hemisphere and
Phoebe. Rings spectra appear more red than the icy satellites in the visible
range but show more intense 1.5-2.0 micron band depths. The correlations among
spectral slopes, band depths, visual albedo and phase permit us to cluster the
saturnian population in different spectral classes which are detected not only
among the principal satellites and rings but among co-orbital minor moons as
well. Finally, we have applied Hapke's theory to retrieve the best spectral
fits to Saturn's inner regular satellites using the same methodology applied
previously for Rhea data discussed in Ciarniello et al. (2011).Comment: 44 pages, 27 figures, 7 tables. Submitted to Icaru
Near-Infrared Spectral Monitoring of Triton with IRTF/SpeX II: Spatial Distribution and Evolution of Ices
This report arises from an ongoing program to monitor Neptune's largest moon
Triton spectroscopically in the 0.8 to 2.4 micron range using IRTF/SpeX. Our
objective is to search for changes on Triton's surface as witnessed by changes
in the infrared absorption bands of its surface ices N2, CH4, H2O, CO, and CO2.
We have recorded infrared spectra of Triton on 53 nights over the ten
apparitions from 2000 through 2009. The data generally confirm our previously
reported diurnal spectral variations of the ice absorption bands (Grundy &
Young 2004). Nitrogen ice shows a large amplitude variation, with much stronger
absorption on Triton's Neptune-facing hemisphere. We present evidence for
seasonal evolution of Triton's N2 ice: the 2.15 micron absorption band appears
to be diminishing, especially on the Neptune-facing hemisphere. Although it is
mostly dissolved in N2 ice, Triton's CH4 ice shows a very different
longitudinal variation from the N2 ice, challenging assumptions of how the two
ices behave. Unlike Triton's CH4 ice, the CO ice does exhibit longitudinal
variation very similar to the N2 ice, implying that CO and N2 condense and
sublimate together, maintaining a consistent mixing ratio. Absorptions by H2O
and CO2 ices show negligible variation as Triton rotates, implying very uniform
and/or high latitude spatial distributions for those two non-volatile ices.Comment: 22 pages, 13 figures, 5 tables, to appear in Icaru
Choosing how to choose : Institutional pressures affecting the adoption of personnel selection procedures
The gap between science and practice in personnel selection is an ongoing concern of human resource management. This paper takes Oliver´s framework of organizations´ strategic responses to institutional pressures as a basis for outlining the diverse economic and social demands that facilitate or inhibit the application of scientifically recommended selection procedures. Faced with a complex network of multiple requirements, practitioners make more diverse choices in response to any of these pressures than has previously been acknowledged in the scientific literature. Implications for the science-practitioner gap are discussed
Planck 2015 results. XXVII. The Second Planck Catalogue of Sunyaev-Zeldovich Sources
We present the all-sky Planck catalogue of Sunyaev-Zeldovich (SZ) sources detected from the 29 month full-mission data. The catalogue (PSZ2) is the largest SZ-selected sample of galaxy clusters yet produced and the deepest all-sky catalogue of galaxy clusters. It contains 1653 detections, of which 1203 are confirmed clusters with identified counterparts in external data-sets, and is the first SZ-selected cluster survey containing > confirmed clusters. We present a detailed analysis of the survey selection function in terms of its completeness and statistical reliability, placing a lower limit of 83% on the purity. Using simulations, we find that the Y5R500 estimates are robust to pressure-profile variation and beam systematics, but accurate conversion to Y500 requires. the use of prior information on the cluster extent. We describe the multi-wavelength search for counterparts in ancillary data, which makes use of radio, microwave, infra-red, optical and X-ray data-sets, and which places emphasis on the robustness of the counterpart match. We discuss the physical properties of the new sample and identify a population of low-redshift X-ray under- luminous clusters revealed by SZ selection. These objects appear in optical and SZ surveys with consistent properties for their mass, but are almost absent from ROSAT X-ray selected samples
Social Media and the Politics of Gender, Race and Identity: The case of Serena Williams.
This study investigates issues of gender, race and identity, as enacted through social media, focusing on the abuse experienced by tennis player Serena Williams during the 2015 Wimbledon Championships. A netnographic analysis of discriminatory or abusive comments relating to Williams were collected from 24 sites on two social media platforms, Facebook and Twitter. These platforms are popular sites commonly used for fan/athlete interaction. Williams identifies as female and African American, therefore intersectionality is adopted to examine the representation of Williams in social media spaces. Several pertinent themes were uncovered relating to Williams including ‘Gender questioning’, ‘Accusations of performance enhancing drugs use’ and ‘Racism’. Such themes showed a simultaneous overlapping of multiple forms of oppression encountered by Williams, reinforcing the notion of the black female athlete as ‘other’ in virtual spaces. Such oppression is perpetuated by the online environment
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