Language Outcomes in Bilingual Individuals with Dementia

Purpose or Research Questions: In people with dementia, how does being bilingual influence the manifestation of dementia related to language skills? Background: Language loss is a paramount component of dementia, and in the case of bilingual speakers, declines in language functioning can occur predominantly in the first language (L1) or in all languages spoken. However, the literature is mixed with regard to whether the two languages decline in tandem or differentially [i.e., one language declines more than the other(s)] (Nanchen et. al, 2016; Ivanova et. al, 2014; Stilwell et. al, 2016). Thus, the present study reviewed the literature in order to (1) determine the nature of the loss in one or more languages in bi- or multilingual individuals with dementia, and (2) to describe the characteristics of that decline with regard to various language domains, including verbal fluency, code-switching, and pragmatic usage, among others. Methods: Researchers utilized six databases to electronically search for articles that met inclusion criteria in February 2017. The initial searches yielded 227 articles after deduplication. The researchers utilized the following inclusion criteria: (1) bilingual or multilingual adult participants, diagnosed with any form of probable dementia; (2) studies including language outcomes (L1/L2 and dominant/non-dominant); (3) studies published in English; (4) study designs comprised of randomized control trials, cohort studies, case studies, systematic reviews, cross-sectional studies, case-control studies, non-randomized control trials, and meta-analyses. Researchers first independently completed title and abstract reviews yielding 61 articles to move to the next round for full-text reviews. Researchers then independently completed full text reviews yielding 15 articles for final inclusion. Anticipated Results: Fifteen studies were included to explore the language outcomes of bilingual and multilingual adults diagnosed with probable dementia of any form. A large majority of studies (n=9), concluded parallel deterioration of all languages spoken by participants. From the included studies, we noted multiple factors reported by the researchers accounting for the parallel or nonparallel deterioration of languages: (1) age of acquisition, (2) proficiency or dominance, (3) and frequency of use. Language declines in each language were also reported to vary longitudinally. Discussion: A review of the literature yielded a complex and, at times, inconclusive picture of the language outcomes in bilingual individuals with dementia. Studies reported contradicting findings as to whether languages declined simultaneously or asynchronously (Salvatierra et. al, 2007; Kowoll et. al, 2015). Our preliminary findings were consistent with the conclusions of a similar systematic review completed by Stilwell et. al in 2016, regarding language outcomes more specifically in patients with probable Alzheimer's disease, a form of dementia. Further research into the language outcomes of bilingual and multilingual adults with dementia will allow for a better understanding of the progression of their language decline due to neurodegenerative disease

Positive affect as coercive strategy: conditionality, activation and the role of psychology in UK government workfare programmes

Eligibility for social security benefits in many advanced economies is dependent on unemployed and underemployed people carrying out an expanding range of job search, training and work preparation activities, as well as mandatory unpaid labour (workfare). Increasingly, these activities include interventions intended to modify attitudes, beliefs and personality, notably through the imposition of positive affect. Labour on the self in order to achieve characteristics said to increase employability is now widely promoted. This work and the discourse on it are central to the experience of many claimants and contribute to the view that unemployment is evidence of both personal failure and psychological deficit. The use of psychology in the delivery of workfare functions to erase the experience and effects of social and economic inequalities, to construct a psychological ideal that links unemployment to psychological deficit, and so to authorise the extension of state—and state-contracted—surveillance to psychological characteristics. This paper describes the coercive and punitive nature of many psycho-policy interventions and considers the implications of psycho-policy for the disadvantaged and excluded populations who are its primary targets. We draw on personal testimonies of people experiencing workfare, policy analysis and social media records of campaigns opposed to workfare in order to explore the extent of psycho-compulsion in workfare. This is an area that has received little attention in the academic literature but that raises issues of ethics and professional accountability and challenges the field of medical humanities to reflect more critically on its relationship to psychology

The benefit sanction: a correctional device or a weapon of disgust?

The benefit sanction is a dominant activation policy in Britain’s ‘welfare-to-work’ regime. While policymakers believe in their necessity to correct behaviour, research shows benefit sanctions cause additional harm to Britain’s marginalised groups. Drawing upon a small-scale qualitative study, this article first navigates new territory, mapping the ways stigma emerges from the state – channelled through the benefit sanction – and manifests in the lives of sanctioned claimants. Acknowledging wider evidence, the sanction is then argued to have failed as a correctional device. Rather, taking into account Britain’s current politico-economic climate, the sanction appears as a weapon used to incite negative emotion in an attempt to police the boundaries of the labour market, while frequently abandoning some of the UK’s most vulnerable citizens

The cell cycle of Leishmania: morphogenetic events and their implications for parasite biology

The cell cycle is central to understanding fundamental biology of Leishmania, a group of human-infective protozoan parasites. Leishmania have two main life cycle morphologies: the intracellular amastigote in the mammalian host and the promastigote in the fly. We have produced the first comprehensive and quantitative description of a Leishmania promastigote cell cycle taking a morphometric approach to position any cell within the cell cycle based on its length and DNA content. We describe timings of cell cycle phases and rates of morphological changes; kinetoplast and nucleus S phase, division and position, cell body growth and morphology changes, flagellum growth and basal body duplication. We have shown that Leishmania mexicana undergoes large changes in morphology through the cell cycle and that the wide range of morphologies present in cultures during exponential growth represent different cell cycle stages. We also show promastigote flagellum growth occurs over multiple cell cycles. There are clear implications for the mechanisms of flagellum length regulation, life cycle stage differentiation and trypanosomatid division in general. This data set therefore provides a platform which will be of use for post-genomic analyses of Leishmania cell biology in relation to differentiation and infection

All-sky search for periodic gravitational waves in LIGO S4 data

We report on an all-sky search with the LIGO detectors for periodic gravitational waves in the frequency range 50-1000 Hz and with the frequency's time derivative in the range -1.0E-8 Hz/s to zero. Data from the fourth LIGO science run (S4) have been used in this search. Three different semi-coherent methods of transforming and summing strain power from Short Fourier Transforms (SFTs) of the calibrated data have been used. The first, known as "StackSlide", averages normalized power from each SFT. A "weighted Hough" scheme is also developed and used, and which also allows for a multi-interferometer search. The third method, known as "PowerFlux", is a variant of the StackSlide method in which the power is weighted before summing. In both the weighted Hough and PowerFlux methods, the weights are chosen according to the noise and detector antenna-pattern to maximize the signal-to-noise ratio. The respective advantages and disadvantages of these methods are discussed. Observing no evidence of periodic gravitational radiation, we report upper limits; we interpret these as limits on this radiation from isolated rotating neutron stars. The best population-based upper limit with 95% confidence on the gravitational-wave strain amplitude, found for simulated sources distributed isotropically across the sky and with isotropically distributed spin-axes, is 4.28E-24 (near 140 Hz). Strict upper limits are also obtained for small patches on the sky for best-case and worst-case inclinations of the spin axes.Comment: 39 pages, 41 figures An error was found in the computation of the C parameter defined in equation 44 which led to its overestimate by 2^(1/4). The correct values for the multi-interferometer, H1 and L1 analyses are 9.2, 9.7, and 9.3, respectively. Figure 32 has been updated accordingly. None of the upper limits presented in the paper were affecte

Search for gravitational waves from binary inspirals in S3 and S4 LIGO data

We report on a search for gravitational waves from the coalescence of compact binaries during the third and fourth LIGO science runs. The search focused on gravitational waves generated during the inspiral phase of the binary evolution. In our analysis, we considered three categories of compact binary systems, ordered by mass: (i) primordial black hole binaries with masses in the range 0.35 M(sun) < m1, m2 < 1.0 M(sun), (ii) binary neutron stars with masses in the range 1.0 M(sun) < m1, m2 < 3.0 M(sun), and (iii) binary black holes with masses in the range 3.0 M(sun)< m1, m2 < m_(max) with the additional constraint m1+ m2 < m_(max), where m_(max) was set to 40.0 M(sun) and 80.0 M(sun) in the third and fourth science runs, respectively. Although the detectors could probe to distances as far as tens of Mpc, no gravitational-wave signals were identified in the 1364 hours of data we analyzed. Assuming a binary population with a Gaussian distribution around 0.75-0.75 M(sun), 1.4-1.4 M(sun), and 5.0-5.0 M(sun), we derived 90%-confidence upper limit rates of 4.9 yr^(-1) L10^(-1) for primordial black hole binaries, 1.2 yr^(-1) L10^(-1) for binary neutron stars, and 0.5 yr^(-1) L10^(-1) for stellar mass binary black holes, where L10 is 10^(10) times the blue light luminosity of the Sun.Comment: 12 pages, 11 figure

Search for Gravitational Wave Bursts from Soft Gamma Repeaters

We present the results of a LIGO search for short-duration gravitational waves (GWs) associated with Soft Gamma Repeater (SGR) bursts. This is the first search sensitive to neutron star f-modes, usually considered the most efficient GW emitting modes. We find no evidence of GWs associated with any SGR burst in a sample consisting of the 27 Dec. 2004 giant flare from SGR 1806-20 and 190 lesser events from SGR 1806-20 and SGR 1900+14 which occurred during the first year of LIGO's fifth science run. GW strain upper limits and model-dependent GW emission energy upper limits are estimated for individual bursts using a variety of simulated waveforms. The unprecedented sensitivity of the detectors allows us to set the most stringent limits on transient GW amplitudes published to date. We find upper limit estimates on the model-dependent isotropic GW emission energies (at a nominal distance of 10 kpc) between 3x10^45 and 9x10^52 erg depending on waveform type, detector antenna factors and noise characteristics at the time of the burst. These upper limits are within the theoretically predicted range of some SGR models.Comment: 6 pages, 1 Postscript figur

Quantum state preparation and macroscopic entanglement in gravitational-wave detectors

Long-baseline laser-interferometer gravitational-wave detectors are operating at a factor of 10 (in amplitude) above the standard quantum limit (SQL) within a broad frequency band. Such a low classical noise budget has already allowed the creation of a controlled 2.7 kg macroscopic oscillator with an effective eigenfrequency of 150 Hz and an occupation number of 200. This result, along with the prospect for further improvements, heralds the new possibility of experimentally probing macroscopic quantum mechanics (MQM) - quantum mechanical behavior of objects in the realm of everyday experience - using gravitational-wave detectors. In this paper, we provide the mathematical foundation for the first step of a MQM experiment: the preparation of a macroscopic test mass into a nearly minimum-Heisenberg-limited Gaussian quantum state, which is possible if the interferometer's classical noise beats the SQL in a broad frequency band. Our formalism, based on Wiener filtering, allows a straightforward conversion from the classical noise budget of a laser interferometer, in terms of noise spectra, into the strategy for quantum state preparation, and the quality of the prepared state. Using this formalism, we consider how Gaussian entanglement can be built among two macroscopic test masses, and the performance of the planned Advanced LIGO interferometers in quantum-state preparation

Searching for a Stochastic Background of Gravitational Waves with LIGO

The Laser Interferometer Gravitational-wave Observatory (LIGO) has performed the fourth science run, S4, with significantly improved interferometer sensitivities with respect to previous runs. Using data acquired during this science run, we place a limit on the amplitude of a stochastic background of gravitational waves. For a frequency independent spectrum, the new limit is $\Omega_{\rm GW} < 6.5 \times 10^{-5}$. This is currently the most sensitive result in the frequency range 51-150 Hz, with a factor of 13 improvement over the previous LIGO result. We discuss complementarity of the new result with other constraints on a stochastic background of gravitational waves, and we investigate implications of the new result for different models of this background.Comment: 37 pages, 16 figure