The European Undergraduate Research-Oriented Participatory Education (EU-ROPE) At Copenhagen Business School

While the knowledge management literature has addressed the explicit and tacit skills needed for successful performance in the modern enterprise, little attention has been paid to date in this particular literature as to how these wide-ranging skills may be suitably acquired during the course of an undergraduate business school education. This paper presents case analysis of the research-oriented participatory education curriculum developed at Copenhagen Business School because it appears uniquely suited, by a curious mix of Danish education tradition and deliberate innovation, to offer an educational experience more empowering of essential tacit knowledge skills than that found in educational institutions in other national settings. We specify the program forms and procedures for consensus-based governance and group work (as benchmarks) that demonstrably instruct undergraduates in the tacit skill dimensions of knowledge thought to be essential for success following graduation

Undergraduate Synopsis-based Oral Examinations at a Scandinavian Business School

We report a local or regional undergraduate examination form – the synopsis-based oral examination (S-BOE), as it is deployed in both large and small international management education programs at a Scandinavian business school. The S-BOE format is designed to assess student cognitive achievement in light of specified learning objectives through a focused presentation and dialogue involving an examiner and qualified censor, the latter being formally present to ensure process fairness for both examiner and student. It affords the examiner and censor the opportunity to explore student cognitive skills over the known range: unistructural > multistructural > relational > extended abstract (Biggs, J. 1999). Individuals as well as student project groups may be assessed using this approach. Administrative costs do not significantly exceed that of other course assessment formats: written reports or in-class group examinations. There are also interesting learning efficiencies; practitioner experience, reflection, and dialogue with students suggest that all students experience this examination format as a learning experience in itself, over a range of course-related knowledge issues and interpersonal skilling. Exemplary students manifest “dramatic knowledge” in those instances when they creatively display a comprehensive, reflective, and reflexive understanding of course material in presentation and subsequent intersubjective dialogue. The authors discuss important features of this undergraduate examination format that remain largely overlooked and under-appreciated in terms that regionally and locally contextualize international accreditation standards and process. At a time when economic, efficiency, and standardization concerns increasingly pressure educational institutions to adopt testing methods that are psychologically “distant” in respect to the instructor-student relationship, the synopsis-based oral examination is an interesting alternative suitable for small as well as large academic programs

European Undergraduate - Research Oriented Participatory Education (EU-ROPE, 2) At a Danish Business School: Education Policy, Administrative Practice, and Survey Data on Project Advisor Qualifications and Preferences

This paper was composed in the fall of 2007. It was then presented on 17 November 2007 at the Matchpoints Conference at the University of Århus, a conference jointly sponsored by the Irish Embassy to Denmark and the University of Århus. We subsequently presented the paper to an internal IKL session of colleagues involved in educational research (dubbed, the "Educational Irregulars’) and then offered the paper to an internal seminar of the Asian Research Center. Throughout this process, Maribel Blasco has been particularly helpful as a colleague with knowledge and interest in the role, nature, and politics of tertiary education. We learned through this process that our Working Paper is at least four separate research journal pieces – in potential. Thus, we file this as a record of a work in progress and as a follow up to the previously filed Working Paper we now refer to as the "EU-ROPE 1” paper – our first venture into exploring the educational character and implications of the CBS SPRØK undergraduate educational model

CFD Analysis to Demonstrate in Vessel Retention Inducing a Bypass Flow

The goal of this work is to design a nozzle system around the Reactor Pressure Vessel (RPV) of a VVER-1000 nuclear reactor which would ensure successful melt retention during a severe accident. Simulations were performed with a multiphase model in ANSYS Fluent 19.1 to determine this. The results suggest that an efficient cooling can be achieved by inducing a flow rising parallel to the RPV walls in the flooded reactor cavity. In order to do this, it is proposed to use one central nozzle below the RPV and a ring of 32 nozzles 0.5 m above the RPV bottom. Assuming a 2 bar pressure, injection of 750 m3/h water at 80oC through the nozzles led to little steam production and a heat flux below the critical value

Periodic orbits in the restricted three-body problem and Arnold's J+J^+-invariant

We apply Arnold's theory of generic smooth plane curves to Stark-Zeeman systems. This is a class of Hamiltonian dynamical systems that describes the dynamics of an electron in an external electric and magnetic field, and includes many systems from celestial mechanics. Based on Arnold's $J^+$-invariant, we introduce invariants of periodic orbits in planar Stark-Zeeman systems and study their behaviour.Comment: 36 Pages, 16 Figure

The Helium content and age of the Hyades: Constraints from five binary systems and Hipparcos parallaxes

We compare the accurate empirical mass-luminosity (M-L) relation based on five Hyades binary systems to predictions of stellar models calculated with various input parameters (helium, metallicity, age) or physics (mixing-length ratio, model atmosphere, equation of state, microscopic diffusion). Models based on a helium content Ysim0.28 inferred from the dydz enrichment law are more than 3sigma beyond the observations, suggesting that the initial helium abundance is lower than expected from its supersolar metallicity. With the photometric metallicity (FeH=0.144pm0.013 dex, Grenon (2000) we derive Y=0.255\pm0.009. Because of the (Y,FeH) degeneracy in the M-L plane, the uncertainty grows to Delta Y=0.013 if the metallicity from spectroscopy is adopted (FeH=0.14pm0.05 dex, Cayrel de Strobel et al 1997). We use these results to discuss the Hertzsprung-Russell (HR) diagram of the Hyades, in the (Mv,B-V) plane, based on the very precise Hipparcos dynamical parallaxes. Present models fit the tight observed sequence very well except at low temperatures. In the low mass region of the HR diagram sensitive to the mixing-length parameter (aMLT), the slope of the main sequence (MS) suggests that aMLT could decrease from a solar (or even supersolar) value at higher mass to subsolar values at low mass, which is also supported by the modeling of the vB22 M-L relation. We find that the discrepancy at low temperatures (B-V\gtrsim 1.2) remains, even if an improved equation of state or better model atmospheres are used. Finally, we discuss the positions of the stars at turn-off in the light of their observed rotation rates and we deduce that the maximum age of the Hyades predicted by the present models is sim650 Myr.Comment: 14 pages, 13 figures, accepted for publication in A&

Obscuration of Supersoft X-ray Sources by Circumbinary Material - A Way to Hide Type Ia Supernova Progenitors?

The progenitors of supernovae (SNe) type Ia are usually assumed to be either a single white dwarf (WD) accreting from a non-degenerate companion (the SD channel) or the result of two merging WDs (DD channel). However, no consensus currently exists as to which progenitor scenario is the correct one, or whether the observed SN Ia rate is produced by a combination of both channels. Unlike a DD progenitor a SD progenitor is expected to emit supersoft X-rays for a prolonged period of time (~1 Myr) as a result of the burning of accreted matter on the surface of the WD. An argument against the SD channel as a significant producer of SNe type Ia has been the lack of observed supersoft X-ray sources (SSS) and the lower-than-expected integrated soft X-ray flux from elliptical galaxies. We wish to determine if it is possible to obscure the supersoft X-ray emission from a nuclear burning white dwarf in an accreting single degenerate binary system. In case of obscured systems we wish to determine their general observational characteristics. We examine the emergent X-ray emission from a canonical SSS system surrounded by a spherically symmetric configuration of material, assuming a black body spectrum with T_BB=50 eV and L=10^38 erg/s. The circumbinary material is assumed to be of solar chemical abundances, and we leave the mechanism behind the mass loss into the circumbinary region unspecified. If steadily accreting, nuclear burning WDs are canonical SSS our analysis suggests that they can be obscured by relatively modest circumbinary mass loss rates. This may explain the discrepancy of SSS compared to the SN Ia rate inferred from observations if the SD progenitor scenario contributes significantly to the SN Ia rate. Recycled emissions from obscured systems may be visible in other wavebands than X-rays. It may also explain the lack of observed SSS in symbiotic binary systems.Comment: 10 pages, 4 figures, accepted A&

Detailed statistical analysis plan for the Danish Palliative care trial (DanPaCT)

Acknowledgements We wish to thank the students who sent out the questionnaires, who entered and compared all data, help with data management, made material blind to the investigators, and were/will be outcome assessors of interventions given. They were: Nicla Rohde Christensen, Ellen Lundorff, Marc Klee Olsen, Charlotte Lund Rasmussen, and Nete Skjødt. This work was funded by the Tryg Foundation [journal number 7-10-0838A] and the Danish Cancer Society [journal number R16-A695]. Other than funding the trial, the funding body had no role in the design, conduct, analysis, or reporting of the present trial.Peer reviewedPublisher PD

The Rest-frame Optical Colors of 99,000 SDSS Galaxies

We synthesize the rest-frame Stroemgren colors using SDSS spectra for 99,088 galaxies selected from Data Release 1. This narrow-band ~200 AA photometric system (uz, vz, bz, yz), first designed for the determination of effective temperature, metallicity and gravity of stars, measures the continuum spectral slope of galaxies in the rest-frame 3200-5800 AA wavelength range. Galaxies form a remarkably narrow locus (~0.03 mag) in the resulting color-color diagram. The Bruzual & Charlot population synthesis models suggest that the position of a galaxy along this locus is controlled by a degenerate combination of metallicity and age of the dominant stellar population. Galaxy distribution along the locus is bimodal, with the local minimum corresponding to an ~1 Gyr old single stellar population. The position perpendicular to the locus is independent of metallicity and age, and reflects the galaxy's dust content, as implied by both the models and the statistics of IRAS detections. A comparison of this locus with the galaxy locus in the H_delta-D_n(4000) diagram, utilized by Kauffmann et al. (2003) to estimate stellar masses, reveals a tight correlation, although the two analyzed spectral ranges barely overlap. Overall, the galaxy spectral energy distribution in the entire UV to near-IR range can be described as a single-parameter family with an accuracy of 0.1 mag, or better. This nearly one-dimensional distribution of galaxies in the multi-dimensional space of measured parameters strongly supports the conclusion of Yip et al. (2004), based on a principal component analysis, that SDSS galaxy spectra can be described by a small number of eigenspectra. Apparently, the contributions of stellar populations that dominate the optical emission from galaxies are combined in a simple and well-defined way.Comment: Accepted for publication in MNRAS; 19 pages, 28 color figure

Tracing the evolution of NGC6397 through the chemical composition of its stellar populations

With the aim to constrain multiple populations in the metal-poor globular cluster NGC6397, we analyse and discuss the chemical compositions of a large number of elements in 21 red giant branch stars. High-resolution spectra were obtained with the FLAMES/UVES spectrograph on VLT. We have determined non-LTE abundances of Na and LTE abundances for the remaining 21 elements, including O, Mg, Al, alpha, iron-peak, and neutron-capture elements, many of which have not previously been analysed for this cluster. We have also considered the influence of possible He enrichment in the analysis of stellar spectra. We find that the Na abundances of evolved, as well as unevolved, stars show a distinct bimodality, which suggests the presence of two stellar populations; one primordial stellar generation with composition similar to field stars, and a second generation that is enriched in material processed through hydrogen-burning (enriched in Na and Al and depleted in O and Mg). The cluster is dominated (75%) by the second generation. The red giant branch show a similar bimodal distribution in the Stroemgren colour index c_y=c_1-(b-y), implying a large difference also in N abundance. The two populations have the same composition of all analysed elements heavier than Al, within the measurement uncertainty of the analysis, with the possible exception of [Y/Fe]. Using two stars with close to identical stellar parameters, one from each generation, we estimate the difference in He content, Delta Y=0.01+-0.06, given the assumption that the mass fraction of iron is the same for the stars. Finally, we show that winds from fast rotating massive stars of the first generation can be held responsible for the abundance patterns observed in NGC6397 second generation long-lived stars and estimate that the initial mass of the cluster were at least ten times higher than its present-day value.Comment: 13 pages + appendix with two tables. Accepted for publication in A&A. v2: minor language corrections and Table A.2. correcte