In times of health reform, fiscal restraint and population aging, it becomes increasingly imperative to understand what must be done to better link research and policy in the health area. In this paper, the major determinants of healthy aging are discussed in terms of current conceptual frameworks of health, measurement, methodologies, and data sources. In order to maximize the benefit for the health of current and future Canadian seniors, policy recommendations are made to Statistics Canada, Health Canada, and the Seniors Independence Research Program (SIRP) which cover a range of issues related to measurement and data sources, health services, health status, economic status, and education.

Gravitational waves from coalescing neutron stars encode information about nuclear matter at extreme densities, inaccessible by laboratory experiments. The late inspiral is influenced by the presence of tides, which depend on the neutron star equation of state. Neutron star mergers are expected to often produce rapidly rotating remnant neutron stars that emit gravitational waves. These will provide clues to the extremely hot post-merger environment. This signature of nuclear matter in gravitational waves contains most information in the 2–4 kHz frequency band, which is outside of the most sensitive band of current detectors. We present the design concept and science case for a Neutron Star Extreme Matter Observatory (NEMO): a gravitational-wave interferometer optimised to study nuclear physics with merging neutron stars. The concept uses high-circulating laser power, quantum squeezing, and a detector topology specifically designed to achieve the high-frequency sensitivity necessary to probe nuclear matter using gravitational waves. Above 1 kHz, the proposed strain sensitivity is comparable to full third-generation detectors at a fraction of the cost. Such sensitivity changes expected event rates for detection of post-merger remnants from approximately one per few decades with two A+ detectors to a few per year and potentially allow for the first gravitational-wave observations of supernovae, isolated neutron stars, and other exotica.

This study used a single case experimental design to investigate the use of the Unified Protocol for Transdiagnostic Treatment of Emotional Disorders (UP) among a sample of individuals with depression and anxiety who also presented with borderline personality disorder (BPD). Eight women received individual treatment with the UP over the course of 14–16 treatment sessions, and were assessed for anxiety and depression severity on a weekly basis over a 2–6 week baseline period and throughout treatment. Three of the eight participants demonstrated reliable pre- to post-treatment clinical improvements on depression and stress scales, and one participant demonstrated a reliable reduction on an anxiety scale. Two participants demonstrated a reliable improvement in overall anxiety. The results indicate that the UP applied to individuals diagnosed with primary BPD may lead to clinical improvement in depression, stress and anxiety for some individuals. However, the majority of individuals with BPD in our sample did not show strong improvement, and this suggests the need for additional sessions of UP or an intervention that focuses on the symptoms of BPD specifically for some women.

Inorganic calcite precipitation experiments were conducted to determine whether inducing specific orientations of calcite crystal growth can cause the enrichment of cations larger than Ca. Malonic acid (CH2(COOH)), a di-carboxylic acid, was used to poison growth on acute kink sites, promoting growth on obtuse kink sites, causing calcite crystals elongated along their c-axes to form in a mechanism similar to that seeninthe growth of E. huxleyi coccoliths. Calcite was precipitated with a range of malonic acid concentrations (0 to 10-1 M), and 9x10-5 M of either SrCl2 or MgCl2. The results show that calcite crystals precipitated in the presence of large malonic acid concentrations show significant elongation along the c axis, and suggest that increasing malonate concentrations corresponded with increasing DSr. Experiments with 10-1 M malonic acid caused elevated DSr comparable to that predicted for E. huxleyi coccolith calcite (Langer et al., 2006).

Despite extensive research on organizational virtue, our understanding about factors that promote virtue within organizations remains unclear. Drawing on upper echelon theory, we examine the relationship between five top management team (TMT) characteristics and organizational virtue orientation (OVO)—the integrated set of values and beliefs that support ethical traits and virtuous behaviors of an organization. Specifically, we utilize prospectuses of initial public offering (IPO) firms and 10-K post-IPO filings to explore how TMT composition with respect to member age, tenure, education, functional background, and gender influences OVO. Additionally, we examine the moderating effects of organizational size, and argue that the more expansive structures and processes associated with larger organizations diminish the main relationships. Our findings, using two sources of data, are consistent, but somewhat mixed in their support for our hypotheses. Overall, TMT characteristics do appear to influence OVO, but in more complex and counterintuitive ways than initially expected.

The Iranian Empire emerged in the third century in the interstices of the Silk Road that increasingly linked the markets of the Mediterranean and the Near East with South, Central, and East Asia. The ensuing four centuries of Iranian rule corresponded with the heyday of trans-Eurasian trade, as the demand of moneyed imperial elites across the continent for one another's high-value commodities stimulated the development of long-distance networks. Despite its position at the nexus of trans-continental and trans-oceanic commerce, accounts of Iran in late antiquity relegate trade to a marginal role in its political economy. The present article seeks to foreground the contribution of trans-continental mercantile networks to the formation of Iran and to argue that its development depended as much on the political economies of its western and eastern neighbours as on internal Near Eastern factors.

The Omani basement is located spatially distant from the dominantly juvenile Arabian–Nubian Shield (ANS) to its west, and its relationship to the amalgamation of those arc terranes has yet to be properly constrained. The Jebel Ja'alan (NE Oman) basement inlier provides an excellent opportunity to better understand the Neoproterozoic tectonic geography of Oman and its relationship to the ANS. To understand the origin of this basement inlier, we present new radiogenic isotopic data from igneous bodies in Jebel Ja'alan. U–Pb and 40Ar/39Ar geochronological data are used to constrain the timing of magmatism and metamorphism in the jebel. Positive εHf and εNd values indicate a juvenile origin for the igneous lithologies. Phase equilibria modelling is used to constrain the metamorphic conditions recorded by basement. Pressure–temperature (P–T) pseudosections show that basement schists followed a clockwise P–T path, reaching peak metamorphic conditions of c. 650–700°C at 4–7.5 kbar, corresponding to a thermal gradient of c. 90–160°C/kbar. From the calculated thermal gradient, in conjunction with collected trace-element data, we interpret that the Jebel Ja'alan basement formed in an arc environment. Geochronological data indicate that this juvenile arc formed during Tonian time and is older than basement further west in Oman. We argue that the difference in timing is related to westwards arc accretion and migration, which implies that the Omani basement represents its own tectonic domain separate to the ANS and may be the leading edge of the Neoproterozoic accretionary margin of India.

A model of the growth and decay of the Antarctic Peninsula Ice Sheet during the last glacial/interglacial cycle is used to identify the main controls on ice sheet behavior. Using as input glaciological assumptions derived by W. F. Budd and I. N. Smith (1982, Annals of Glaciology 3, 42–49), bedrock topography, isostatic compensation, and mass balance relationships, the model is driven by sea-level change over the last 40,000 yr in association with assumed changes in the rate of melting beneath ice shelves. An ice sheet dome over 3.5 km thick grows on the offshore shelf and straits west of the Antarctic Peninsula and reaches a maximum at 18,000 yr B.P. Collapse begins at 14,000 yr B.P. but becomes rapid and continuous after 10,000 yr B.P. The present stable ice cover is achieved at 6500 yr B.P. Ice growth and decay are characterized by thresholds which separate periods of steady state from periods of rapid transition; the thresholds usually relate to topography. Tests show that ice sheet behavior is most sensitive to sea-level change, basal marine melting, and accumulation and is less sensitive to isostasy, spatial variation in accumulation, calving rates, and ice flow parameterization. Tests of the model against field evidence show good agreement in places, as well as discrepancies which require further work.

At least in conventional hydrostatic ice-sheet models, the numerical error associated with grounding line dynamics can be reduced by modifications to the discretization scheme. These involve altering the integration formulae for the basal traction and/or driving stress close to the grounding line and exhibit lower – if still first-order – error in the MISMIP3d experiments. MISMIP3d may not represent the variety of real ice streams, in that it lacks strong lateral stresses, and imposes a large basal traction at the grounding line. We study resolution sensitivity in the context of extreme forcing simulations of the entire Antarctic ice sheet, using the BISICLES adaptive mesh ice-sheet model with two schemes: the original treatment, and a scheme, which modifies the discretization of the basal traction. The second scheme does indeed improve accuracy – by around a factor of two – for a given mesh spacing, but $\lesssim 1$ km resolution is still necessary. For example, in coarser resolution simulations Thwaites Glacier retreats so slowly that other ice streams divert its trunk. In contrast, with $\lesssim 1$ km meshes, the same glacier retreats far more quickly and triggers the final phase of West Antarctic collapse a century before any such diversion can take place.

In the Iranian Empire (226–636 CE), jurists drawn from the ranks of the Zoroastrian priestly elite developed a complex of institutions designed to guarantee the reproduction of aristocratic males as long as the empire endured. To overcome the high rate of mortality characteristic of preindustrial demographic regimes, they aimed to maximize the fertility rate without compromising their endogamous ideals through the institutions of reproductive coercion, temporary marriage, and “substitute-successorship.” Occupying a position between the varieties of monogamy and polygyny hitherto practiced in the Ancient Near East, the Iranian organization of sex enabled elites not only to reproduce their patrilineages reliably across multiple generations, but also to achieve an appropriate ratio of resources to number of offspring. As the backbone of this juridical architecture, the imperial court became the anchor of aristocratic power, and ruling and aristocratic dynasties became increasingly intertwined and interdependent, forming the patrilineal networks of the “Iranians”—the agents and beneficiaries of Iranian imperialism. The empire's aristocratic structure took shape through a sexual economy: the court created and circulated sexual and reproductive incentives that incorporated elite males into its network that was, thanks to its politically enhanced inclusive fitness, reliable and reproducible. In demonstrating the centrality of Zoroastrian cosmology to the construction and operation of the relevant juridical institutions, I seek to join the approaches of evolutionary biology and cultural anthropology to reproduction that have been pursued in opposition, to account for the historical role of sex in the consolidation of the Iranian Empire.