381 research outputs found

    Effects of musically-induced emotions on choice reaction time performance

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    The main objective of the current study was to examine the impact of musically-induced emotions on athletes’ subsequent choice reaction time (CRT) performance. A random sample of 54 tennis players listened to researcher-selected music whose tempo and intensity were modified to yield six different music excerpts (three tempi x two intensities) before completing a CRT task. Affective responses, heart rate (HR), and RTs for each condition were contrasted with white noise and silence conditions. As predicted, faster music tempi elicited more pleasant and aroused emotional states; and higher music intensity yielded both higher arousal (p < .001) and faster subsequent CRT performance (p < .001). White noise was judged significantly less pleasant than all experimental conditions (p < .001); and silence was significantly less arousing than all but one experimental condition (p < .001). The implications for athletes’ use of music as part of a preevent routine when preparing for reactive tasks are discussed

    Prolonged hospitalization effects on psychosocial development in chronic illness pediatric patients

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    Prolonged hospitalization effects on psychosocial development in chronic illness pediatric populations Abstract Courtney Cumberland, Sophie Kinrade, Megan Pringle, and Zoe Quarles Background/Objective: Frequent and extensive hospitalizations have a negative impact on the psychosocial development of children in the most formative years of their lives. This problem is most evident in children who have chronic disease or health conditions that require multiple hospital stays and interventions. This topic can be considered broad because of the extensive variety of chronic conditions and how that determines a child\u27s length of stay. This study aims to identify whether patient-to-patient interaction impacts the psychosocial development in children who experience these extended and repetitive hospitalizations. Methods: Research was guided by the John Hopkins Evidence-Based Practice Model. Google Scholar, EBSCOHost, and PubMed were the databases used to search for key terms which included “prolonged hospitalization”, “chronic illnesses”, “psychosocial development”, “pediatric”, “school-aged”, and “chronic”. Only relevant evidence data from the last five years are analyzed to ensure the validity of the study and uncover the best evidence-based practice to implement. Results: A total of ten articles were appraised for the study. The following themes were identified: prolonged hospitalizations led to social developmental delays, there is an increased risk of delay in developmental milestones, and peer group interventions are recommended for better outcomes. Depending on the age, severity of illness, and peer interactions, children’s development is affected. Conclusion: Prolonged hospitalizations affect children\u27s ability to reach developmental milestones. There are many different factors that play a role in reaching development milestones, and healthcare providers need to consider these factors in developing evidence-based interventions appropriate for this group

    The statistical morphology of Saturn’s equatorial ENA projections

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    Saturn is engulfed in a cloud of neutral gas that originates from ice fissures on the surface of Enceladus. Some particles collide and exchange charge, separating electrons and ions which are guided by Saturn’s magnetic field. In this way, Saturn’s rotating magnetosphere is loaded with mass, which eventually must be lost into space via ejections of plasma that stretch magnetic field lines to breaking point. Some charged particles in the outer magnetosphere do not escape, but are fired back towards Saturn with field lines as they snap back into place. These energetic ions collide with neutrals, creating energetic neutral atoms (ENA) that were detectable using the INCA camera onboard Cassini. Pictures of Saturn’s magnetosphere from INCA reveal dynamic regions of plasma flow, important for understanding the entire system. We present an analysis of the INCA image set obtained throughout Cassini’s mission. We’ve processed ~670,000 images to characterise Saturn’s average ENA morphology. Rings of ENAs are located at distances between 7-10 Rs, the point of peak interaction between the energetic ions and the neutral cloud. We also find ENA variation with Saturn’s rotation period, associated with current systems that modulate the thickness of the plasmasheet every ~10 hours

    The silicon supplement 'Monomethylsilanetriol' is safe and increases the body pool of silicon in healthy Pre-menopausal women.

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    BACKGROUND: Monomethylsilanetriol (MMST) has been used for decades as an oral silicon supplement for bone and connective tissue health, although there are no formal data on its in vivo utilisation or safety following sustained dosing. METHODS: To investigate whether MMST contributes to the body pool of silicon and, secondly, to establish its safety following 4 weeks' supplementation in humans, twenty-two healthy pre-menopausal women (22-38 years) were recruited and supplemented with MMST at the maximum daily recommended dose (10.5 mg Si/day) for 4 weeks in a double-blind, randomised, placebo-controlled, cross-over design (i.e. 8 weeks in total). Fasting serum and urine samples were collected at baseline and at the end of the 4-week supplementation/placebo periods for analysis of total silicon by inductively coupled plasma optical emission spectrometry, MMST by proton nuclear magnetic resonance spectroscopy and full serum biochemistry. Participants also reported on, by questionnaire, their health, well-being and quality of life at 0, 4 and 8 weeks. RESULTS: Overall, 4-weeks supplementation with MMST significantly increased total fasting Si concentrations in serum and urine (P ≤ 0.003; paired t-test). MMST was semi-quantifiable in serum and quantifiable in urine, but only accounted for ca. 50% and 10%, respectively, of the increased total-Si concentration. There were no reported adverse effects (i.e. changes to health and well-being) or serum biochemical changes with MMST versus placebo. CONCLUSIONS: Our data indicate that oral MMST is safe, is absorbed and undergoes sufficient metabolism in vivo to raise fasting serum silicon levels, consistent with other well absorbed forms of dietary silicon (e.g. orthosilicic acid). It thus appears to be a suitable silicon supplement

    Dietary Observations of Ultra-Endurance Runners in Preparation for and During a Continuous 24-h Event

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    Carbohydrate (CHO) intake recommendations for events lasting longer than 3h indicate that athletes should ingest up to 90g.h.−1 of multiple transportable carbohydrates (MTC). We examined the dietary intake of amateur (males: n=11, females: n=7) ultra-endurance runners (mean age and mass 41.5±5.1years and 75.8±11.7kg) prior to, and during a 24-h ultra-endurance event. Heart rate and interstitial glucose concentration (indwelling sensor) were also tracked throughout the event. Pre-race diet (each 24 over 48h) was recorded via weighed intake and included the pre-race meal (1–4h pre-race). In-race diet (24h event) was recorded continuously, in-field, by the research team. Analysis revealed that runners did not meet the majority of CHO intake recommendations. CHO intake over 24–48h pre-race was lower than recommended (4.0±1.4g·kg−1; 42±9% of total energy), although pre-race meal CHO intake was within recommended levels (1.5±0.7g·kg−1). In-race CHO intake was only in the 30–60g·h−1 range (mean intake 33±12g·h−1) with suboptimal amounts of multiple transportable CHO consumed. Exercise intensity was low to moderate (mean 68%HRmax 45%VO2max) meaning that there would still be an absolute requirement for CHO to perform optimally in this ultra-event. Indeed, strong to moderate positive correlations were observed between distance covered and both CHO and energy intake in each of the three diet periods studied. Independent t-tests showed significantly different distances achieved by runners consuming ≥5 vs

    The effect of field-aligned currents and centrifugal forces on ionospheric outflow at Saturn

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    Ionospheric outflow is driven by an ambipolar electric field induced due to the separation of electrons and ions in a gravitational field when equilibrium along a magnetic field line is lost. A model of ionospheric outflow at Saturn was developed using transport equations to estimate the number of charged particles that flow from the auroral regions into the magnetosphere. The model evaluates the outflow from 1,400 km in altitude above the 1 bar level, to 3 RS along the field line. The main ion constituents evaluated are R+ and R+3. We consider the centrifugal force exerted on the particles due to a fast rotation rate, along with the effects of field‐aligned currents present in the auroral regions. The total number flux from both auroral regions is found to be 5.5–13.0×1027 s−1, which relates to a total mass source of 5.5–17.7 kg s−1. These values are on average an order of magnitude higher than expected without the additional effects of centrifugal force and field‐aligned currents. We find the ionospheric outflow rate to be comparable to the lower estimates of the mass loading rate from Enceladus and are in agreement with recent Cassini observations. This additional mass flux into the magnetosphere can substantially affect the dynamics and composition of the inner and middle magnetosphere of Saturn
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