Facets of Psychopathy in Relation to Trauma-Exposure and Posttraumatic Stress Symptomology in a Sample of Incarcerated Male Offenders

Purpose: The aim was to investigate the moderating role of psychopathy facets on the relationship between traumatic exposure and posttraumatic stress disorder (PTSD) symptomology. Design/methodology/approach: Participants were male prisoners incarcerated in the U.K. Findings: The analysis revealed differential associations between the two facets of psychopathy, with potentially traumatic events and symptoms of PTSD. Specifically, neither primary psychopathy nor trauma exposure were significantly related to PTSD, while secondary psychopathy was positively and significantly related with PTSD symptoms. Furthermore, the effect of trauma exposure on PTSD was found to depend on the level of secondary psychopathy. More specifically, trauma exposure was strongly and positively associated with PTSD symptoms for low levels of secondary psychopathy and negatively associated with PTSD symptomology for individuals with high levels of secondary psychopathy. Originality/value: The findings clarify linkages among psychopathy facets, trauma, and PTSD, and extend our understanding of the presentation of PTSD in male prisoners

The origin of Jupiter's outer radiation belt

The intense inner radiation belt at Jupiter (>50 MeV at 1.5 RJ) is generally accepted to be created by radial diffusion of electrons from further away from the planet. However, this requires a source with energies that exceed 1 MeV outside the orbit of the moon Io at 5.9 RJ, which has never been explained satisfactorily. Here we test the hypothesis that this source population could be formed from a very soft energy spectrum, by particle injection processes and resonant electron acceleration via whistler mode chorus waves. We use the British Antarctic Survey Radiation Belt Model to calculate the change in the electron flux between 6.5 and 15 RJ; these are the first simulations at Jupiter combining wave particle interactions and radial diffusion. The resulting electron flux at 100 keV and 1 MeV lies very close to the Galileo Interim Radiation Electron model spectrum after 1 and 10 days, respectively. The primary driver for the increase in the flux is cyclotron resonant acceleration by chorus waves. A peak in phase space density forms such that inside L≈9 radial diffusion transports electrons toward Jupiter, but outside L≈9 radial diffusion acts away from the planet. The results are insensitive to the softness of the initial energy spectrum but do depend on the value of the flux at the minimum energy boundary. We conclude by suggesting that the source population for the inner radiation belt at Jupiter could indeed be formed by wave-particle interactions

Theory of a Higher Order Phase Transition: Superconducting Transition in BKBO

We describe here the properties expected of a higher (with emphasis on the order fourth) order phase transition. The order is identified in the sense first noted by Ehrenfest, namely in terms of the temperature dependence of the ordered state free energy near the phase boundary. We have derived an equation for the phase boundary in terms of the discontinuities in thermodynamic observables, developed a Ginzburg-Landau free energy and studied the thermodynamic and magnetic properties. We also discuss the current status of experiments on $Ba_{0.6}K_{0.4}BiO_3$ and other $BiO_3$ based superconductors, the expectations for parameters and examine alternative explanations of the experimental results.Comment: 18 pages, no figure

Survey of Saturn Z-mode Emission

Because of the role of Z-mode emission in the diffusive scattering and resonant acceleration of electrons, we conduct a survey of intensity in the Saturn inner magnetosphere. Z-mode is primarily observed as “5 kHz” narrowband emission in the lower density regions where the ratio of cyclotron to plasma frequency, fc/fp > 1 to which we limit this study. This occurs at Saturn along the inner edge of the Enceladus torus near the equator and at higher latitudes. We present profiles and parametric fits of intensity as a function of frequency, radius, latitude, and local time. The magnetic field intensity levels are lower than chorus, but the electric field intensities are comparable. We conclude that Z-mode wave-particle interactions may make a significant contribution to electron acceleration in the inner magnetosphere of Saturn, supplementing acceleration produced by chorus emission

Studies of coagulation and fibrinolysis in normal and pregnant subjects

In this thesis, the development, refinement and standardisation of a wide range of coagulation and fibrinolytic assay techniques are described. Particular attention was directed towards the assay of Factor VIII, cryofibrinogen and fibrin/fibrinogen degradation products (F.D.P.). A new type of coagulation end point recorder was investigated and the use of the Atlas computer in the analysis of results is outlined. In addition, a study was made of various standard plasma preparations for the control of coagulation factor assays. Using these laboratory techniques, the effect of severe and moderate exercise, adrenalin infusions and beta- adrenergic receptor blockage on selected parameters of the coagulation and fibrinolytic systems, in normal volunteers, were studied. No correlations were observed between parameter changes in either system, and contrary to some reports, Factor XII was not increased post exercise. Some subjects exhibited a low fibrinolytic response to the exercise procedures, confirming previous work from this laboratory, but the coagulation response in these individuals did not appear to differ in any constant manner from the normal pattern. The adrenalin induced changes in Factor VIII were completely blocked by Propranolol, but this drug only partially lowered the response to adrenalin of plasminogen activator. The new beta -adrenergic blocker drug, ICI 50172, was fouhd to have only minimal effects on the two systems. These results are fully discussed in the light of presently available concepts of the haemostatic mechanism. In the studies on pregnant subjects, parameters of coagulation and fibrinolysis throughout the gestational period were measured. One new finding was that of a significant increase of serum F.D.P. in late pregnancy. It was also found, in another study, that the reactivity of the fibrinolytic system to an exercise stress in the third trimester was greatly impaired in some subjects. Further coagulation and fibrinolytic studies in pregnant and non -pregnant patients undergoing intra- abdominal surgical operations, demonstrated that significant changes occurred in euglobulin lysis activity, fibrinogen and F.D.P. levels. The application of specific coagulation and fibrinolytic tests to clinical haemostatic emergencies of pregnancy is described in the final section. All these studies have provided a basis for a fuller discussion in each section, of concepts such as the Shwartzman reaction, disseminated intravascular coagulation, and haemorrhage and thromboembolism. It is concluded that although some of the physio-pathologidal interrelationships of coagulation and fibrinolysis are now becoming clarified, many problems still remain, and these may only be resolved when improved methodology becomes available. The extension of work reported in this thesis may aid in the elucidation of important aspects of haemorrhage and thrombosis

‘We have to wait in a queue for our turn quite a bit’ Examining children’s physical activity during primary physical education lessons

The overall purpose of this study was to examine children’s physical activity (PA) during primary physical education (PE). This was achieved through the following two research objectives: (1) to measure children’s PA, lesson context and teacher promotion of PA during PE lessons; and (2) to explore teachers’ and children’s perspectives on PA levels during PE lessons. Evidence suggests that children’s PA during PE is below recommended levels and further research is required to understand the reasons why. Through a mixed method design, 138 children were observed using the System for Observing Fitness and Instruction Time, 80 children participated in group interviews, and 13 teachers were interviewed, across three primary schools in England. Findings indicated that the mean percentage of lesson time allocated to moderate to vigorous PA (MVPA) was 42.4% and the average lesson length was 35.3 minutes. Qualitative themes identified were: ‘knowledge and beliefs’; ‘teacher pedagogy’; and ‘teacher development’. The findings indicate that a change in perspective is needed, which includes a focus on PA during primary PE lessons. Intervention work is required that targets teachers’ knowledge and beliefs towards PE along with the development of effective teaching strategies. However, this needs to be grounded in an ecological approach which will allow researchers and schools to target the various levels of influence. It is strongly recommended that interventions are grounded in behaviour change theory, as this study indicates that sharing knowledge about pedagogical strategies to increase children’s MVPA does not necessarily produce changes in teachers’ behaviours

Young children’s impressionable use of teleology: the influence of question wording and questioned topic on teleological explanations for natural phenomena

There is a significant body of research on children's preconceptions concerning scientific concepts and the impact this has upon their science education. One active issue concerns the extent to which young children's explanations for the existence of natural kinds rely on a teleological rationale: for example, rain is for watering the grass, or tigers’ stripes are for camouflage. It has been argued that this teleological tendency hampers children's ability to learn about causality in the natural world. This paper investigates two factors (question wording and topic) which it is argued have led to a misestimation of children's teleological tendencies within the area natural phenomena: i.e., those that are time-constrained, natural events or process such as snow, clouds or night. Sixty-six (5- to 8-years-old) children took part in a repeated-measures experiment, answering both open- and leading-questions across 10 topics of natural phenomena. The findings indicate that children's teleological reasoning may have been overestimated as open question forms significantly reduced their tendency to answer teleologically. Moreover, the concept of teleology is more nuanced than often suggested. Consequently, young children may be more able to learn about causal explanations for the existence of natural phenomena than the literature implies

Electron Correlation and Jahn-Teller Interaction in Manganese Oxides

The interplay between the electron repulsion $U$ and the Jahn-Teller electron-phonon interation $E_{LR}$ is studied with a large $d$ model for the ferromagnetic state of the manganese oxides. These two interactions collaborate to induce the local isospin (orbital) moments and reduce the bandwidth $B$. Especially the retardation effect of the Jahn-Teller phonon with the frequency $\Omega$ is effective to reduce $B$, but the strong $\Omega$-dependence occurs even when the Coulombic interaction is dominating ($U >> E_{LR}$) as long as $E_{LR} > \Omega$. The phonon spectrum consists of two components, i.e., the temperature independent sharp peak at $\omega = {\tilde \Omega} = \Omega [(U +4 E_{LR})/U]^{1/2}$ and that corresponding to the Kondo peak. These results compared with the experiments suggest that $\Omega <E_{LR} <U$ in the metallic manganese oxides.Comment: REVTE

Electron acceleration at Jupiter: input from cyclotron-resonant interaction with whistler-mode chorus waves

Jupiter has the most intense radiation belts of all the outer planets. It is not yet known how electrons can be accelerated to energies of 10 MeV or more. It has been suggested that cyclotron-resonant wave-particle interactions by chorus waves could accelerate electrons to a few MeV near the orbit of Io. Here we use the chorus wave intensities observed by the Galileo spacecraft to calculate the changes in electron flux as a result of pitch angle and energy diffusion. We show that, when the bandwidth of the waves and its variation with L are taken into account, pitch angle and energy diffusion due to chorus waves is a factor of 8 larger at L-shells greater than 10 than previously shown. We have used the latitudinal wave intensity profile from Galileo data to model the time evolution of the electron flux using the British Antarctic Survey Radiation Belt (BAS) model. This profile confines intense chorus waves near the magnetic equator with a peak intensity at ∼5° latitude. Electron fluxes in the BAS model increase by an order of magnitude for energies around 3 MeV. Extending our results to L = 14 shows that cyclotron-resonant interactions with chorus waves are equally important for electron acceleration beyond L = 10. These results suggest that there is significant electron acceleration by cyclotron-resonant interactions at Jupiter contributing to the creation of Jupiter's radiation belts and also increasing the range of L-shells over which this mechanism should be considered

Strain effect on electronic transport and ferromagnetic transition temperature in La0.9_{0.9}Sr0.1_{0.1}MnO3_{3} thin films

We report on a systematic study of strain effects on the transport properties and the ferromagnetic transition temperature $T_{c}$ of high-quality La$_{0.9}$Sr$_{0.1}$MnO$_{3}$ thin films epitaxially grown on (100) SrTiO$_{3}$ substrates. Both the magnetization and the resistivity are critically dependent on the film thickness. $T_{c}$ is enhanced with decreasing the film thickness due to the compressive stain produced by lattice mismatch. The resistivity above 165 K of the films with various thicknesses is consistent with small polaronic hopping conductivity. The polaronic formation energy $E_{P}$ is reduced with the decrease of film thickness. We found that the strain dependence of $T_{c}$ mainly results from the strain-induced electron-phonon coupling. The strain effect on $E_{P}$ is in good agreement with the theoretical predictions.Comment: 6 pages and 5 figures, accepted for publication in Phys. Rev.