FATHERS’ RELIGIOUS INVOLVEMENT AND EARLY CHILDHOOD BEHAVIOR

Previous research suggests that many men increase their religious involvement after the birth of a new child. This study extends this research by examining whether fathers maintain a higher rate of religious participation as children get older and how fathers’ religiosity may influence children’s behavior. Results suggest that many fathers maintain a higher level of religious participation during the early years of their child’s life. Although fathers’ religious involvement does not appear to directly influence children’s behavior, there is evidence that fathers’ religiosity moderates the influence of other family characteristics on children. Parental relationship quality and mothers’ religiosity are associated with fewer problem behaviors among children when fathers believe that religion is important to family life. Results also suggest that being raised by a non-religious father is associated with increased externalizing problem behavior among young children. Overall, this study suggests that religious communities may be a source of support that encourages fathers to be more active in their family life and promote positive development among children.religion, behavior, religious attendance, fathers, mothers, children

Directions For A New Aestheticism

The idea of a new aestheticism is now explicit in both philosophical aesthetics and cultural theory with the publication of Gary Iseminger's The Aesthetic Function of Art and an anthology of essays edited by John Joughin and Simon Malpas critiquing the anti-aestheticism of literary theory. Both are significant in marking a wider trend reacting to, broadly speaking, intellectualised and historicised accounts of art, refocusing on the idea of appreciation itself, and working away from the emphasis on ideology and disregard for the particularity of works in, especially, literary theory. This broader context also includes renewed debates running within philosophical aesthetics about non-perceptual aesthetic properties and the aesthetic experience of conceptual artworks, and about beauty in art, considerations that have engaged two philosophers normally identified by their commitment to art theoretical and historical (and by extension, non-aesthetic) accounts of artistic making and viewing, namely Noël Carroll and Arthur Danto. So Carroll acknowledges that what's at stake is an aesthetic theory of art that is potentially 'back in business', while Danto's 'surprising' theoretic re-engagement with the concept of beauty has been noted by Diarmuid Costello

A Semi-Analytic dynamical friction model that reproduces core stalling

We present a new semi-analytic model for dynamical friction based on Chandrasekhar's formalism. The key novelty is the introduction of physically motivated, radially varying, maximum and minimum impact parameters. With these, our model gives an excellent match to full N-body simulations for isotropic background density distributions, both cuspy and shallow, without any fine-tuning of the model parameters. In particular, we are able to reproduce the dramatic core-stalling effect that occurs in shallow/constant density cores, for the first time. This gives us new physical insight into the core-stalling phenomenon. We show that core stalling occurs in the limit in which the product of the Coulomb logarithm and the local fraction of stars with velocity lower than the infalling body tends to zero. For cuspy backgrounds, this occurs when the infalling mass approaches the enclosed background mass. For cored backgrounds, it occurs at larger distances from the centre, due to a combination of a rapidly increasing minimum impact parameter and a lack of slow moving stars in the core. This demonstrates that the physics of core-stalling is likely the same for both massive infalling objects and low-mass objects moving in shallow density backgrounds. We implement our prescription for dynamical friction in the direct summation code NBODY6 as an analytic correction for stars that remain within the Roche volume of the infalling object. This approach is computationally efficient, since only stars in the inspiralling system need to be evolved with direct summation. Our method can be applied to study a variety of astrophysical systems, including young star clusters orbiting near the Galactic Centre; globular clusters moving within the Galaxy; and dwarf galaxies orbiting within dark matter halos.Comment: 16 pages, 21 figures, Accepted for publication in MNRA

Religious Heterogamy and Relationship Stability: A Comparison of Married and Cohabiting Unions

Many studies have explored dynamics within religiously heterogamous marriages, but little is known about religiously heterogamous cohabiting unions. Using data from the Fragile Families Study, this study examines the influence of religious heterogamy on union stability among married and cohabiting couples. Results suggest that religious heterogamy is more common in cohabiting unions than marriages. Results also suggest that cohabiting unions are more likely to dissolve than marriages, and the risk of separation is higher for religiously heterogamous cohabiting unions (especially those in which one partner is religious and the other is not) than religiously heterogamous marriages. Finally, there is evidence showing that some religiously heterogamous cohabiting couples have a higher risk of relationship dissolution than religious heterogamous married couples due to lower relationship quality. Overall, this study extends the religion and family literature by showing that religious differences may lead to greater instability for cohabiting relationships than marriages.religion, behavior, religious attendance, fathers, mothers, children

A semi-analytic dynamical friction model for cored galaxies

We present a dynamical friction model based on Chandrasekhar's formula that reproduces the fast inspiral and stalling experienced by satellites orbiting galaxies with a large constant density core. We show that the fast inspiral phase does not owe to resonance. Rather, it owes to the background velocity distribution function for the constant density cores being dissimilar from the usually-assumed Maxwellian distribution. Using the correct background velocity distribution function and the semi-analytic model from Petts et al. (2015), we are able to correctly reproduce the infall rate in both cored and cusped potentials. However, in the case of large cores, our model is no longer able to correctly capture core-stalling. We show that this stalling owes to the tidal radius of the satellite approaching the size of the core. By switching off dynamical friction when rt(r) = r (where rt is the tidal radius at the satellite's position) we arrive at a model which reproduces the N-body results remarkably well. Since the tidal radius can be very large for constant density background distributions, our model recovers the result that stalling can occur for Ms/Menc << 1, where Ms and Menc are the mass of the satellite and the enclosed galaxy mass, respectively. Finally, we include the contribution to dynamical friction that comes from stars moving faster than the satellite. This next-to-leading order effect becomes the dominant driver of inspiral near the core region, prior to stalling.Comment: 13 pages, 12 figures, resubmitted to MNRAS after responding to feedback from the refere

Will the NHS continue to function in an influenza pandemic? A survey of healthcare workers in the West Midlands, UK

If UK healthcare services are to respond effectively to pandemic influenza, levels of absenteeism amongst healthcare workers (HCWs) must be minimised. Current estimates of the likelihood that HCWs will continue to attend work during a pandemic are subject to scientific and predictive uncertainty, yet an informed evidence base is needed if contingency plans addressing the issues of HCW absenteeism are to be prepared

Concurrent formation of supermassive stars and globular clusters : implications for early self-enrichment

19 pages, 5 figures, accepted to MNRAS (shortened abstract and included feedback from the community)We present a model for the concurrent formation of globular clusters (GCs) and supermassive stars (SMSs, ≳10 3M ⊙) to address the origin of the HeCNONaMgAl abundance anomalies in GCs. GCs form in converging gas flows and accumulate low-angular momentum gas, which accretes on to protostars. This leads to an adiabatic contraction of the cluster and an increase of the stellar collision rate. A SMS can form via runaway collisions if the cluster reaches sufficiently high density before two-body relaxation halts the contraction. This condition is met if the number of stars ≳10 6 and the gas accretion rate ≳10 5M ⊙ Myr -1, reminiscent of GC formation in high gas-density environments, such as - but not restricted to - the early Universe. The strong SMS wind mixes with the inflowing pristine gas, such that the protostars accrete diluted hot-hydrogen burning yields of the SMS. Because of continuous rejuvenation, the amount of processed material liberated by the SMS can be an order of magnitude higher than its maximum mass. This 'conveyor-belt' production of hot-hydrogen burning products provides a solution to the mass budget problem that plagues other scenarios. Additionally, the liberated material is mildly enriched in helium and relatively rich in other hot-hydrogen burning products, in agreement with abundances of GCs today. Finally, we find a super-linear scaling between the amount of processed material and cluster mass, providing an explanation for the observed increase of the fraction of processed material with GC mass. We discuss open questions of this new GC enrichment scenario and propose observational tests.Peer reviewe

The Tagliamento River: A model ecosystem of European importance

In NE Italy is a remarkable floodplain river that retains the dynamic nature and morphological complexity that must have characterized most Alpine rivers in the pristine stage. This river system, the Fiume Tagliamento, constitutes an invaluable resource not only as a reference site for the Alps, but as a model ecosystem for large European rivers. The Tagliamento has a number of attributes that have not been given due consideration in river ecology: (i) an immense corridor of more than 150 km2 that connects the land and the sea and two biomes, the Alps and the Mediterranean; (ii) unconstrained floodplain segments characterised by a dynamic mosaic of aquatic/terrestrial habitats; and (iii) a large number of vegetated islands (ca. 700). We believe it is critical to understand the functional roles of these endangered attributes in order to effectively engage in river conservation and management programmes. The Tagliamento River in Italy offers the rare opportunity to investigate natural processes at a scale that can be studied almost nowhere else in Europ

A conceptual framework for negotiating public involvement in municipal waste management decision-making in the UK

The technical expertise that politicians relied on in the past to produce cost-effective and environmentally sound solutions no longer provides sufficient justification to approve waste facilities. Local authorities need to find more effective ways to involve stakeholders and communities in decision-making since public acceptance of municipal waste facilities is integral to delivering effective waste strategies. This paper presents findings from a research project that explored attitudes towards greater levels of public involvement in UK waste management decision-making. The study addressed questions of perception, interests, the decision context, the means of engagement and the necessary resources and capacity for adopting a participatory decision process. Adopting a mixed methods approach, the research produced an empirical framework for negotiating the mode and level of public involvement in waste management decision-making. The framework captures and builds on theories of public involvement and the experiences of practitioners, and offers guidance for integrating analysis and deliberation with public groups in different waste management decision contexts. Principles in the framework operate on the premise that the decision about ‘more’ and ‘better’ forms of public involvement can be negotiated, based on the nature of the waste problem and wider social context of decision-making. The collection of opinions from the wide range of stakeholders involved in the study has produced new insights for the design of public engagement processes that are context-dependent and ‘fit-for-purpose’; these suggest a need for greater inclusivity in the case of contentious technologies and high levels of uncertainty regarding decision outcomes