Inspiring Macro Practice through Rural Social Work: Teaching Notes on Experiential Learning

Experiential learning is the cornerstone of social work education and has been shown to be highly beneficial to students, especially with increased self-confidence in skills, interest in similar work post-graduation, cultural humility, application of theory to practice, problem solving skills, and critical thinking. Additionally, experiential learning opportunities support the nine competencies of social work education and provides students with an opportunity to try out their budding skills with the guidance and supervision of seasoned social workers. This paper discusses an innovative course project that allowed a group of social work students to engage in macro-level social work practice and grant writing with a rural Missouri county that struggles with high poverty rates, health disparities, and the digital divide. Additional topics discussed are the benefits to the community, students, and agency partners; increased interest in macro-level social work; dedication to rural practice; and the overall evaluation of the project

School Social Workers: Important Assets in Rural Areas

As the American educational system continues to evolve and take on more social service responsibilities for students, their families, and the community, the need for school social workers has intensified. However, the demand considerably exceeds developed positions for school social workers. The increase in awareness of childhood trauma, toxic stress, poverty, and potential to spill over into the classroom places schools in a position where they need to be responsive to students’ multi-faceted needs. This conceptual article will discuss the overwhelming need for school social workers, barriers to obtaining school social workers, and the benefits school social workers can bring

Self-Care in Mental Health: A Study on the Effectiveness of Self Care for Overall Mental Wellbeing

Studies have shown that self-care can be very effective in the treatment of different mental health issues. The purpose of this study is to test the effectiveness of three common self-care techniques (sleep, diet, and exercise) on the overall mental health and wellbeing of college students. This research consists of two surveys that collect data on self-care habits and current mental health, interposed by a two-week period of implementing positive changes to one of the self-care methods. This study used voluntary response sampling. The survey was be administered online to students at Georgia Southern University. The survey data was collected and analyzed using SPSS to determine whether the differences between groups of data are statistically significant. The data showed the most significant improvements in the overall mental wellbeing of the participants who improved sleep habits. However, it also showed improvements for the participants who improved diet or exercise habits. This shows that although proper sleep habits make the biggest impact, following any of the three self-care techniques leads to an improvement in overall mental wellbeing

Higher Spin Gravitational Couplings and the Yang--Mills Detour Complex

Gravitational interactions of higher spin fields are generically plagued by inconsistencies. We present a simple framework that couples higher spins to a broad class of gravitational backgrounds (including Ricci flat and Einstein) consistently at the classical level. The model is the simplest example of a Yang--Mills detour complex, which recently has been applied in the mathematical setting of conformal geometry. An analysis of asymptotic scattering states about the trivial field theory vacuum in the simplest version of the theory yields a rich spectrum marred by negative norm excitations. The result is a theory of a physical massless graviton, scalar field, and massive vector along with a degenerate pair of zero norm photon excitations. Coherent states of the unstable sector of the model do have positive norms, but their evolution is no longer unitary and their amplitudes grow with time. The model is of considerable interest for braneworld scenarios and ghost condensation models, and invariant theory.Comment: 19 pages LaTe

The Final Fate of Binary Neutron Stars: What Happens After the Merger?

The merger of two neutron stars usually produces a remnant with a mass significantly above the single (nonrotating) neutron star maximum mass. In some cases, the remnant will be stabilized against collapse by rapid, differential rotation. MHD-driven angular momentum transport eventually leads to the collapse of the remnant's core, resulting in a black hole surrounded by a massive accretion torus. Here we present simulations of this process. The plausibility of generating short duration gamma ray bursts through this scenario is discussed.Comment: 3 pages. To appear in the Proceedings of the Eleventh Marcel Grossmann Meeting, Berlin, Germany, 23-29 July 2006, World Scientific, Singapore (2007

Magnetic Braking and Viscous Damping of Differential Rotation in Cylindrical Stars

Differential rotation in stars generates toroidal magnetic fields whenever an initial seed poloidal field is present. The resulting magnetic stresses, along with viscosity, drive the star toward uniform rotation. This magnetic braking has important dynamical consequences in many astrophysical contexts. For example, merging binary neutron stars can form "hypermassive" remnants supported against collapse by differential rotation. The removal of this support by magnetic braking induces radial fluid motion, which can lead to delayed collapse of the remnant to a black hole. We explore the effects of magnetic braking and viscosity on the structure of a differentially rotating, compressible star, generalizing our earlier calculations for incompressible configurations. The star is idealized as a differentially rotating, infinite cylinder supported initially by a polytropic equation of state. The gas is assumed to be infinitely conducting and our calculations are performed in Newtonian gravitation. Though highly idealized, our model allows for the incorporation of magnetic fields, viscosity, compressibility, and shocks with minimal computational resources in a 1+1 dimensional Lagrangian MHD code. Our evolution calculations show that magnetic braking can lead to significant structural changes in a star, including quasistatic contraction of the core and ejection of matter in the outermost regions to form a wind or an ambient disk. These calculations serve as a prelude and a guide to more realistic MHD simulations in full 3+1 general relativity.Comment: 20 pages, 19 figures, 3 tables, AASTeX, accepted by Ap