Epistemic and social scripts in computer-supported collaborative learning

Collaborative learning in computer-supported learning environments typically means that learners work on tasks together, discussing their individual perspectives via text-based media or videoconferencing, and consequently acquire knowledge. Collaborative learning, however, is often sub-optimal with respect to how learners work on the concepts that are supposed to be learned and how learners interact with each other. One possibility to improve collaborative learning environments is to conceptualize epistemic scripts, which specify how learners work on a given task, and social scripts, which structure how learners interact with each other. In this contribution, two studies will be reported that investigated the effects of epistemic and social scripts in a text-based computer-supported learning environment and in a videoconferencing learning environment in order to foster the individual acquisition of knowledge. In each study the factors ‘epistemic script’ and ‘social script’ have been independently varied in a 2×2-factorial design. 182 university students of Educational Science participated in these two studies. Results of both studies show that social scripts can be substantially beneficial with respect to the individual acquisition of knowledge, whereas epistemic scripts apparently do not to lead to the expected effects

A Survey of Perceived Job satisfaction Among School Nurses

Many studies have examined job satisfaction of nurses in various clinical settings, but few have focused on school nurses. This project was a follow-up to the study by Foley, Wilson, Lee, Young Cureton, & Canham (2004), who used a written questionnaire and convenience sample rather than the electronic means and random sampling employed here. Both studies, based on Stamp\u27s Index of Work Satisfaction, analyzed six parameters to determine the degree of job satisfaction among members of a state school nurses organization. The results of this study substantially agreed with the prior study. School nurses were not satisfied with their jobs. Autonomy in their job was the most significant parameter, followed by interaction, professional status, pay, task requirements, and organizational policies. Demographic information pointed to a potential problem with 53% of the school nurses surveyed intending to retire within 1 0 years

The phase diagram of neutral quark matter: Self-consistent treatment of quark masses

We study the phase diagram of dense, locally neutral three-flavor quark matter within the framework of the Nambu--Jona-Lasinio model. In the analysis, dynamically generated quark masses are taken into account self-consistently. The phase diagram in the plane of temperature and quark chemical potential is presented. The results for two qualitatively different regimes, intermediate and strong diquark coupling strength, are presented. It is shown that the role of gapless phases diminishes with increasing diquark coupling strength.Comment: 10 pages, 7 figures. Two new figures added as in the published versio

Condition for gapless color-antitriplet excitations in NJL models

We present an exact condition for the existence of gapless quasiparticle excitations in NJL models of color superconducting quark matter with a quark-quark interaction in the scalar color-antitriplet channel. The condition can be represented by a rotated ellipse in the plane of mass and chemical potential differences for the paired quark fields.Comment: Accepted for publication in PRC. 5 pages, 4 figures; Corrected typos and added one more term to the series expansion in (19

Campus Update: December 1989 v. 1, no. 3

Monthly newsletter of the BU Medical Campu

Tkachenko waves, glitches and precession in neutron star

Here I discuss possible relations between free precession of neutron stars, Tkachenko waves inside them and glitches. I note that the proposed precession period of the isolated neutron star RX J0720.4-3125 (Haberl et al. 2006) is consistent with the period of Tkachenko waves for the spin period 8.4s. Based on a possible observation of a glitch in RX J0720.4-3125 (van Kerkwijk et al. 2007), I propose a simple model, in which long period precession is powered by Tkachenko waves generated by a glitch. The period of free precession, determined by a NS oblateness, should be equal to the standing Tkachenko wave period for effective energy transfer from the standing wave to the precession motion. A similar scenario can be applicable also in the case of the PSR B1828-11.Comment: 6 pages, no figures, accepted to Ap&S

1. The Absolute Dynastic State

One of the most significant developments of the early modern period was the evolution of the national state from its beginnings in the feudal monarchy of the High and Late Middle Ages. The ghost of a universal state coincident with a universal church, which had lingered to the end of the Middle Ages, was finally laid to rest with the successful disruption of Christendom and recognition of the sovereignty of the national state. In its place there was a frank acceptance of the political fragmentation of Europe along the geographical lines which were already clearly discernible, at least in western Europe, by 1500. [excerpt

Diquark condensation effects on hot quark star configurations

The equation of state for quark matter is derived for a nonlocal, chiral quark model within the mean field approximation.We investigate the effects of a variation of the formfactors of the interaction on the phase diagram of quark matter. Special emphasis is on the occurrence of a diquark condensate which signals a phase transition to color superconductivity and its effects on the equation of state under the condition of beta- equilibrium and charge neutrality. We calculate the quark star configurations by solving the Tolman- Oppenheimer- Volkoff equations and obtain for the transition from a hot, normal quark matter core of a protoneutron star to a cool diquark condensed one a release of binding energy of the order of Delta M c^2 ~ 10^{53} erg. We find that this energy could not serve as an engine for explosive phenomena since the phase transition is not first order. Contrary to naive expectations the mass defect increases when for a given temperature we neglect the possibility of diquark condensation.Comment: 24 pages, 2 tables, 8 figures, references added, figures and text improve