Exploring the capabilities approach in a sport for development and peace setting.

Sport for Development and Peace (SDP) has become a popular approach to development. However, critical scholars remain skeptical of SDP’s effectiveness. Utilizing a holistic approach that includes local voices may help a program’s effectiveness. Scholars are searching for a framework flexible enough to accommodate the varied nature of programs. One theoretical approach is the Capabilities Approach, which evaluates well-being based on what people can do and be. This case study explored the Capabilities Approach in an SDP setting. Youth Odyssey, a non-profit organization that works with at-risk youth through adventure programming, was the case. This case study explored what role does an SDP program play in participants achieving their capabilities, focusing on identifying functionings, barriers, and capabilities. Twenty-one interviews, 43 field observations and over 100 document/artifacts provided a holistic analysis of the case through triangulation. RQ1 asked what functionings are being supported by Youth Odyssey? RQ2 explored how does Youth Odyssey help remove barriers for participants? RQ3 asked what capabilities are Youth Odyssey creating for its participants? The findings add to the limited literature exploring SDP using the Capabilities Approach. It highlighted the Capabilities Approach’s potential to use local context and address concerns of critical scholars regarding SDP from a planning/execution/evaluation standpoint. It was one of the first studies to understand the role an SDP organization played in increasing an individual’s functionings, freedoms, and capabilities using qualitative data

Preventing Sexual Violence On Campus: Conducting Background Checks on Student-Athletes

Since a growing number of athletic departments are utilizing background checks, institutions would be prudent to develop a more holistic approach which includes the creation and enforcement of uniform policies and procedures for student and athlete recruitment and acceptance, the promotion and education of issues surrounding sexual violence, and the implementation of prevention education and bystander intervention programming for students and student-athletes once they become a part of the institution. Additionally, institutions should continuously evaluate the policies’ effectiveness, educate and train admissions staff how to interpret and address background check results and university policy, and regularly update programming to evolve as universities’ expectations progress

Sport Management Study Abroad and International Exchange Program Innovation for a Post COVID-19 Era

The globalization of the sport industry has required sport management programs to create strategies for internationalizing students. Study abroad programs are a prominent example of those strategies. The COVID-19 pandemic had a significant impact on study abroad programs in Spring of 2020. Many students had their study abroad experiences either cut short or canceled all together. The purpose of this essay is to discuss how the student learning process can continue during an interruption or cancellation of study abroad and international exchange programs due to a pandemic or other global issues. Using an observational study, we asked the following research questions: RQ1: What can the disruption caused by the COVID-19 pandemic to higher education teach the sport management community to ensure students are able to engage in experiential and transformative learning? RQ2: What strategies can institutions of higher education implement to provide students with continued opportunities to benefit from the types of engagements traditionally associated with international programming? We offer recommendations that will help sport management programs prepare for future interruptions to study abroad experiences. These recommendations aim at fostering experiential and transformative learning despite disruptions to the traditional study abroad experience

Legal Implications of Conducting Background Checks on Intercollegiate Student Athletes

Non

Complete RXTE Spectral Observations of the Black Hole X-ray Nova XTE J1550-564

We report on the X-ray spectral behavior of the exceptionally bright X-ray nova XTE J1550-564 during its 1998-99 outburst. Our study is based on 209 pointed observations using the PCA and HEXTE instruments onboard the Rossi X-ray Timing Explorer spanning 250 days and covering the entire double-peaked eruption that occurred from 1998 September until 1999 May. The spectra are fit to a model including multicolor blackbody disk and power-law components. The source is observed in the very high and high/soft outburst states of black hole X-ray novae. During the very high state, when the power-law component dominated the spectrum, the inner disk radius is observed to vary by more than an order of magnitude; the radius decreased by a factor of 16 in one day during a 6.8 Crab flare. If the larger of these observed radii is taken to be the last stable orbit, then the smaller observed radius would imply that the inner edge of the disk is inside the event horizon! However, we conclude that the apparent variations of the inner disk radius observed during periods of increased power-law emission are probably caused by the failure of the multicolor disk/power-law model; the actual physical radius of the inner disk may remain fairly constant. This interpretation is supported by the fact that the observed inner disk radius remains approximately constant over 120 days in the high state, when the power-law component is weak, even though the disk flux and total flux vary by an order of magnitude. The mass of the black hole inferred by equating the approximately constant inner disk radius observed in the high/soft state with the last stable orbit for a Schwarzschild black hole is M_BH = 7.4 M_sun (D/6 kpc) (cos i)^{-1/2}.Comment: Submitted to ApJ, 20 pages including 6 figures + 4 large table

Strong Water Absorption in the Dayside Emission Spectrum of the Planet HD 189733b

Recent observations of the extrasolar planet HD 189733b did not reveal the presence of water in the emission spectrum of the planet. Yet models of such 'Hot Jupiter' planets predict an abundance of atmospheric water vapour. Validating and constraining these models is crucial for understanding the physics and chemistry of planetary atmospheres in extreme environments. Indications of the presence of water in the atmosphere of HD 189733b have recently been found in transmission spectra, where the planet's atmosphere selectively absorbs the light of the parent star, and in broadband photometry. Here we report on the detection of strong water absorption in a high signal-to-noise, mid-infrared emission spectrum of the planet itself. We find both a strong downturn in the flux ratio below 10 microns and discrete spectral features that are characteristic of strong absorption by water vapour. The differences between these and previous observations are significant and admit the possibility that predicted planetary-scale dynamical weather structures might alter the emission spectrum over time. Models that match the observed spectrum and the broadband photometry suggest that heat distribution from the dayside to the night side is weak. Reconciling this with the high night side temperature will require a better understanding of atmospheric circulation or possible additional energy sources.Comment: 11 pages, 1 figure, published in Natur

The USNO-B Catalog

USNO-B is an all-sky catalog that presents positions, proper motions, magnitudes in various optical passbands, and star/galaxy estimators for 1,042,618,261 objects derived from 3,643,201,733 separate observations. The data were obtained from scans of 7,435 Schmidt plates taken for the various sky surveys during the last 50 years. USNO-B1.0 is believed to provide all-sky coverage, completeness down to V = 21, 0.2 arcsecond astrometric accuracy at J2000, 0.3 magnitude photometric accuracy in up to five colors, and 85% accuracy for distinguishing stars from non-stellar objects. A brief discussion of various issues is given here, but the actual data are available from http://www.nofs.navy.mil and other sites.Comment: Accepted by Astronomical Journa

Hairy Black Holes in String Theory

Solutions of bosonic string theory are constructed which correspond to four-dimensional black holes with axionic quantum hair. The basic building blocks are the renormalization group flows of the CP1 model with a theta term and the SU(1,1)/U(1) WZW coset conformal field theory. However the solutions are also found to have negative energy excitations, and are accordingly expected to decay to the vacuum.Comment: 14 pages (References added

Extraversion and the Rewarding Effects of Alcohol in a Social Context

The personality trait of extraversion has been linked to problematic drinking patterns. Researchers have long hypothesized that such associations are attributable to increased alcohol-reward sensitivity among extraverted individuals, and surveys suggest that individuals high in extraversion gain greater mood enhancement from alcohol than those low in extraversion. Surprisingly, however, alcohol administration studies have not found individuals high in extraversion to experience enhanced mood following alcohol consumption. Of note, prior studies have examined extraverted participants-individuals who selfidentify as being highly social-consuming alcohol in isolation. In the present research, we used a group drinking paradigm to examine whether individuals high in extraversion gained greater reward from alcohol than did those low in extraversion and, further, whether a particular social mechanism (partners' Duchenne smiling) might underlie alcohol reward sensitivity among extraverted individuals. Social drinkers (n ϭ 720) consumed a moderate dose of alcohol, placebo, or control beverage in groups of 3 over the course of 36 min. This social interaction was video-recorded, and Duchenne smiling was coded using the Facial Action Coding System. Results indicated that participants high in extraversion reported significantly more mood enhancement from alcohol than did those low in extraversion. Further, mediated moderation analyses focusing on Duchenne smiling of group members indicated that social processes fully and uniquely accounted for alcohol reward-sensitivity among individuals high in extraversion. Results provide initial experimental evidence that individuals high in extraversion experience increased mood-enhancement from alcohol and further highlight the importance of considering social processes in the etiology of alcohol use disorder

The Use of Microgravity Simulators for Space Research

The spaceflight environment is known to influence biological processes ranging from stimulation of cellular metabolism to possible impacts on cellular damage repair, suppression of immune functions, and bone loss in astronauts. Microgravity is one of the most significant stress factors experienced by living organisms during spaceflight, and therefore, understanding cellular responses to altered gravity at the physiological and molecular level is critical for expanding our knowledge of life in space. Since opportunities to conduct experiments in space are scarce, various microgravity simulators and analogues have been widely used in space biology ground studies. Even though simulated microgravity conditions have produced some, but not all of the biological effects observed in the true microgravity environment, they provide test beds that are effective, affordable, and readily available to facilitate microgravity research. A Micro-g Simulator Center is being developed at Kennedy Space Center (KSC) to offer a variety of microgravity simulators and platforms for Space Biology investigators. Assistance will be provided by both KSC and external experts in molecular biology, microgravity simulation, and engineering. Comparisons between the physical differences in microgravity simulators, examples of experiments using the simulators, and scientific questions regarding the use of microgravity simulators will be discussed