223 research outputs found

    Gender Differences in the Mediation Between Childhood Abuse/Neglect and Trauma

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    Childhood abuse/neglect is a consistent concern in the United States and is related to future physical and mental health concerns. Studies have shown that childhood abuse/neglect can result in negative trauma appraisal, difficulties in emotion regulation, and lower levels of self-compassion. However, less is known about how gender impacts the relationship between negative trauma appraisal, difficulties in emotion regulation, and self-compassion with trauma symptoms in those with a history of childhood abuse/neglect. The purpose of this quantitative cross-sectional correlational study was to measure the impact of gender on the mediating variables (negative trauma appraisal, difficulties in emotion regulation, and self-compassion) and the outcome variable of trauma symptoms with a predictor variable of childhood abuse/neglect. Fairbairnian object-relations theory provided the framework for the study. Data were collected from 176 participants who completed an online survey. Data analyses included conditional process analyses with PROCESS-Macro Model 15. The results indicated that gender did not impact the relationships between the mediating variables and trauma symptoms. Although the null hypotheses could not be rejected, noteworthy findings are presented and discussed. The similarities for males and females in this model may have implications for future interventions. Research into trauma symptoms lead to positive social change by assisting in the improvement of interventions, education, and mitigation of future childhood abuse/neglect

    Inhibitory effects associated with use of modified Photinus pyralis and Renilla reniformis luciferase vectors in dual reporter assays and implications for analysis of ISGs

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    Luciferase reporter constructs are widely used for analysis of gene regulation when characterizing promoter and enhancer elements. We report that the recently developed codon-modified Renilla luciferase construct included as an internal standard for cotransfection must be used with great caution with respect to the amount of DNA transfected. Also, the dual-luciferase reporter vectors encoding Photinus pyralis firefly or Renilla reniformis luciferase showed a linear increase in dose-response with increasing amounts of transfected DNA, but at higher levels of transfected DNA, a reduction in expressed levels of luciferase activity resulted. In addition, treatment with type I interferon (IFN) was found to significantly reduce levels of P. pyralis firefly and Renilla luciferase activity. In contrast, cells transfected with a green fluorescent protein (GFP) reporter construct showed no significant IFN-associated change. The reduction in luciferase activity resulting from IFN treatment was not due to IFN-mediated cytotoxicity, as no change in cellular propidium iodide (PI) staining was observed by flow cytometry. IFN treatment did not alter the levels of firefly luciferase activity in cell culture supernatants or the luciferase mRNA levels determined by quantitative real-time RT-PCR analysis. Based on these results, it is probable that the IFN-induced reduction in levels of luciferase activity detected in reporter assays occurs via a posttranscriptional mechanism. Thus, it is important to be aware of these complications when using luciferase reporter systems in general or for analyzing cytokine-mediated responsive regulation of target genes, particularly by the type I IFNs.No Full Tex

    Observational constraints on the neutron star mass distribution

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    Radio observations of neutron star binary pulsar systems have constrained strongly the masses of eight neutron stars. Assuming neutron star masses are uniformly distributed between lower and upper bounds mlm_l and mum_u, the observations determine with 95\% confidence that 1.01<ml/M⊙<1.341.01 < m_l/\text{M}_\odot < 1.34 and 1.43<mu/M⊙<1.641.43 < m_u/\text{M}_\odot < 1.64. These limits give observational support to neutron star formation scenarios that suggest that masses should fall predominantly in the range 1.3<m/M⊙<1.61.3<m/\text{M}_\odot<1.6, and will also be important in the interpretation of binary inspiral observations by the Laser Interferometer Gravitational-wave Observatory.Comment: Postscript, 4 pages, NU-GR-

    Binary inspiral, gravitational radiation, and cosmology

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    Observations of binary inspiral in a single interferometric gravitational wave detector can be cataloged according to signal-to-noise ratio ρ\rho and chirp mass M\cal M. The distribution of events in a catalog composed of observations with ρ\rho greater than a threshold ρ0\rho_0 depends on the Hubble expansion, deceleration parameter, and cosmological constant, as well as the distribution of component masses in binary systems and evolutionary effects. In this paper I find general expressions, valid in any homogeneous and isotropic cosmological model, for the distribution with ρ\rho and M\cal M of cataloged events; I also evaluate these distributions explicitly for relevant matter-dominated Friedmann-Robertson-Walker models and simple models of the neutron star mass distribution. In matter dominated Friedmann-Robertson-Walker cosmological models advanced LIGO detectors will observe binary neutron star inspiral events with ρ>8\rho>8 from distances not exceeding approximately 2 Gpc2\,\text{Gpc}, corresponding to redshifts of 0.480.48 (0.26) for h=0.8h=0.8 (0.50.5), at an estimated rate of 1 per week. As the binary system mass increases so does the distance it can be seen, up to a limit: in a matter dominated Einstein-deSitter cosmological model with h=0.8h=0.8 (0.50.5) that limit is approximately z=2.7z=2.7 (1.7) for binaries consisting of two 10 M⊙10\,\text{M}_\odot black holes. Cosmological tests based on catalogs of the kind discussed here depend on the distribution of cataloged events with ρ\rho and M\cal M. The distributions found here will play a pivotal role in testing cosmological models against our own universe and in constructing templates for the detection of cosmological inspiraling binary neutron stars and black holes.Comment: REVTeX, 38 pages, 9 (encapsulated) postscript figures, uses epsf.st

    1994-95 Advisory Council on Social Security Technical Panel on Assumptions and Methods Final Report

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    The Panel\u27s major conclusions are: The intermediate projection of the Trustees Report for the Old-Age. Survivors. and Disability Insurance (OASDI) program provide a reasonable evaluation of the financial status. Although the Panel suggests that modifications be considered in various specific assumptions, the overall effect of those suggestions would not significantly change the financial status evaluation. There should be evolutionary implementation of procedures to indicate more adequately the uncertainties involved in the projections. Even though such uncertainties are unavoidable, stochastic analysis should be used to examine more explicitly the probabilities of alternative projections. It is emphasized that there should be an extended period during which the new procedures would supplement, rather than replace, the current methods of considering high-cost and low-cost projections and individual assumption sensitivity analysis. Evaluation of the long-range financial status should put less emphasis on the 75-year actuarial balance and the test of long-range close actuarial balance. Prior to enactment of legislation reforming the program, primary emphasis should be on the projected date the Trust Fund Ratio would fall below 100 percent; when definitive legislative revisions are adopted, subsequent long-range evaluation should compare up-dated projections with the intended results of the legislation. There should be a substantial expansion of SSA\u27s resources and its interaction with experts in related areas: increased recognition should be given to the interrelationships between OASDI and many public and private programs as well as other aspects of the economy. Social Security Administration (SSA) staff does high quality work, but is relatively small and works with inadequate resources. In addition to internal expansion, there should be greater use of outside consultants and contractual research; periodic comprehensive review by technical panels should be supplemented by ongoing arrangements for advice on specific matters

    Exploring the ‘active mechanisms’ for engaging rural-dwelling older men with dementia in a community technological initiative

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    Research has suggested ecopsychosocial initiatives can promote a sense of well-being and inclusion in people with dementia. However, few studies have elucidated the ‘active mechanisms’ whereby such initiatives can achieve these outcomes, so hindering their generalisability. This is particularly pertinent when seeking to support community-dwelling older men with dementia who are reluctant to engage with traditional health and social care initiatives. This paper reports on a study that drew from the principles of Participatory Action Research to explore the ‘active mechanisms’ of a technological initiative for older men (65+ years) with dementia in rural England. An individually-tailored, male-only initiative, using off-the-shelf computer game technology (e.g. iPad, Nintendo Wii and Microsoft Kinect) was delivered over a nine week period. Multiple qualitative methods were employed including; focus groups, open interviews and extensive reflexive field-notes, to gather data from the perspective of twenty-two men, fifteen care partners and five community volunteers. The data were analysed thematically and interpreted using a masculinity lens. Three mechanisms contributed to the initiative’s success: the use of the technology; the male-only environment; and the empowering approach adopted. The paper argues that initiatives aimed at community-dwelling older men with dementia would be advised to consider these gendered experiences and ensure participants can maximise their masculine capital when participating in them, by providing enabling activities, non-threatening environments and empowering approaches of delivery

    Aperture synthesis for gravitational-wave data analysis: Deterministic Sources

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    Gravitational wave detectors now under construction are sensitive to the phase of the incident gravitational waves. Correspondingly, the signals from the different detectors can be combined, in the analysis, to simulate a single detector of greater amplitude and directional sensitivity: in short, aperture synthesis. Here we consider the problem of aperture synthesis in the special case of a search for a source whose waveform is known in detail: \textit{e.g.,} compact binary inspiral. We derive the likelihood function for joint output of several detectors as a function of the parameters that describe the signal and find the optimal matched filter for the detection of the known signal. Our results allow for the presence of noise that is correlated between the several detectors. While their derivation is specialized to the case of Gaussian noise we show that the results obtained are, in fact, appropriate in a well-defined, information-theoretic sense even when the noise is non-Gaussian in character. The analysis described here stands in distinction to ``coincidence analyses'', wherein the data from each of several detectors is studied in isolation to produce a list of candidate events, which are then compared to search for coincidences that might indicate common origin in a gravitational wave signal. We compare these two analyses --- optimal filtering and coincidence --- in a series of numerical examples, showing that the optimal filtering analysis always yields a greater detection efficiency for given false alarm rate, even when the detector noise is strongly non-Gaussian.Comment: 39 pages, 4 figures, submitted to Phys. Rev.

    Care home practitioners’ perceptions of the barriers and facilitators for using off-the-shelf gaming technology with people with dementia

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    Off-the-shelf digital gaming technology has been shown to support the well-being of people with dementia. Yet, to date, it is rarely adopted within dementia care practice, particularly within care homes. Drawing on a descriptive, qualitative approach, this is the first study that has sought to explore care home practitioners’ perceptions of the barriers and facilitators for using gaming technology within their workplace. Data were collected across eight focus groups in the south of England with a total of 39 care home workers. These were analysed inductively following the 6-stage thematic process as outlined by Braun and Clarke (2006). Three themes, constructed from the data suggested, the care environment, staff knowledge and skills for inclusive gaming, and staff perceptions about capabilities (their own and those of people with dementia) inhibited or facilitated the use of gaming technology in care homes. The findings were interpreted through a combination of the Capability, Opportunity, Motivation and Behaviour model and the Theoretical Domains Framework to provide theory-based insights into the mechanisms for supporting behaviour change and implementation within the care home context. We argue for the need to target wider institutional barriers alongside providing inclusive training for care staff on incorporating gaming technology within their person-centred care approaches. Through these mechanisms, they can be provided with the capabilities, opportunities and motivation to integrate gaming technology within their practice, and thus facilitate the process of culture change within care homes

    Gravitational Waves from a Compact Star in a Circular, Inspiral Orbit, in the Equatorial Plane of a Massive, Spinning Black Hole, as Observed by LISA

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    Results are presented from high-precision computations of the orbital evolution and emitted gravitational waves for a stellar-mass object spiraling into a massive black hole in a slowly shrinking, circular, equatorial orbit. The focus of these computations is inspiral near the innermost stable circular orbit (isco)---more particularly, on orbits for which the angular velocity Omega is 0.03 < Omega/Omega_{isco} < 1. The computations are based on the Teukolsky-Sasaki-Nakamura formalism, and the results are tabulated in a set of functions that are of order unity and represent relativistic corrections to low-orbital-velocity formulas. These tables can form a foundation for future design studies for the LISA space-based gravitational-wave mission. A first survey of applications to LISA is presented: Signal to noise ratios S/N are computed and graphed as functions of the time-evolving gravitational-wave frequency for representative values of the hole's mass M and spin a and the inspiraling object's mass \mu, with the distance to Earth chosen to be r_o = 1 Gpc. These S/N's show a very strong dependence on the black-hole spin, as well as on M and \mu. A comparison with predicted event rates shows strong promise for detecting these waves, but not beyond about 1Gpc if the inspiraling object is a white dwarf or neutron star. This argues for a modest lowering of LISA's noise floor. A brief discussion is given of the prospects for extracting information from the observed wavesComment: Physical Review D, in press; 21 pages, 9 figures, 10 tables it is present in the RevTeX fil
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