Learning from Kaupapa Māori: Issues and techniques for engagement

This article argues for recognition of the value and relevance of Indigenous knowledges about principles and practices of engagement to theory-building and praxis in public relations. Specifically, in this article, the Kaupapa Māori body of knowledge and practice that has developed around Indigenous/non-Indigenous engagement in Aotearoa is identified as a valid source of insight for the analogous situation of organisation-public engagement where power imbalance is inherent

The Formation of Star Clusters II: 3D Simulations of Magnetohydrodynamic Turbulence in Molecular Clouds

(Abridged) We present a series of decaying turbulence simulations that represent a cluster-forming clump within a molecular cloud, investigating the role of magnetic fields on the formation of potential star-forming cores. We present an exhaustive analysis of numerical data from these simulations that includes a compilation of all of the distributions of physical properties that characterize bound cores - including their masses, radii, mean densities, angular momenta, spins, magnetizations, and mass-to-flux ratios. We also present line maps of our models that can be compared with observations. Our simulations range between 5-30 Jeans masses of gas, and are representative of molecular cloud clumps with masses between 100-1000 solar masses. The cores have mass-to-flux ratios that are generally less than that of the original cloud, and so a cloud that is initially highly supercritical can produce cores that are slightly supercritical, similar to that seen by Zeeman measurements of molecular cloud cores. Clouds that are initially only slightly supercritical will instead collapse along the field lines into sheets, and the cores that form as these sheets fragment have a different mass spectrum than what is observed. The spin rates of these cores suggests that subsequent fragmentation into multiple systems is likely. The sizes of the bound cores that are produced are typically 0.02-0.2 pc and have densities in the range 10^4-10^5 cm^{-3} in agreement with observational surveys. Finally, our numerical data allow us to test theoretical models of the mass spectrum of cores, such as the turbulent fragmentation picture of Padoan-Nordlund. We find that while this model gets the shape of the core mass spectrum reasonably well, it fails to predict the peak mass in the core mass spectrum.Comment: Accepted by MNRAS. 28 pages, 16 figures. Substantial revision since last versio

Alien Registration- Tilley, Loretta E. (Houlton, Aroostook County)

https://digitalmaine.com/alien_docs/34892/thumbnail.jp

Innovations in the design of an architectural engineering curriculum

This paper introduces a new curriculum, launched in October 2021, in Architectural Engineering, designed out of London, UK for implementation in Giza, Egypt. The developers of this newly formed higher education institution, Newgiza University, sought to introduce more contemporary approaches as well as cutting-edge curricular innovations to the education landscape in Egypt. To achieve this, they enlisted curriculum developers in architecture and engineering from University College London who have expertise in education research, curricular innovation, and the delivery of engineering and architecture modules and degree programs. The team worked in collaboration with experts and educators from Egypt to create a bespoke curriculum, drawing from a range of innovative approaches and educational theories, combining these with many well-established approaches. This paper, which represents the “scholarship of integration”, highlights distinctive aspects of the curriculum, and illustrates how prior research was integrated into the curriculum design, with a focus on the first year. The paper is geared toward design educators as well as curriculum developers

Local contribution of a quantum condensate to the vacuum energy density

We evaluate the local contribution g_[mu nu]L of coherent matter with lagrangian density L to the vacuum energy density. Focusing on the case of superconductors obeying the Ginzburg-Landau equation, we express the relativistic invariant density L in terms of low-energy quantities containing the pairs density. We discuss under which physical conditions the sign of the local contribution of the collective wave function to the vacuum energy density is positive or negative. Effects of this kind can play an important role in bringing about local changes in the amplitude of gravitational vacuum fluctuations - a phenomenon reminiscent of the Casimir effect in QED.Comment: LaTeX, 8 pages. Final journal versio

Gravitational waves in preheating

We study the evolution of gravitational waves through the preheating era that follows inflation. The oscillating inflaton drives parametric resonant growth of scalar field fluctuations, and although super-Hubble tensor modes are not strongly amplified, they do carry an imprint of preheating. This is clearly seen in the Weyl tensor, which provides a covariant description of gravitational waves.Comment: 8 pages, 8 figures, Revte