Cultures of denial: managing the past, justifying the present

In this paper, I propose that if dominant white understandings of colonisation rely upon a relatively linear interpretation of history, then the unsettling of this linearity may allow for the voicing of a critical reading of racism in Australia. In order to do this, I suggest that psychoanalysis may provide a means for understanding the everyday talk of white people in ways that may challenge the now/then accounts of history that are used to deny ongoing acts of white violence and, thus, to refuse the fact of Indigenous sovereignty. Through a brief analysis of focus group data with white Australians, I suggest that we may see repression at work when those of us who are descendants of white colonisers attempt to manage our relationship to the past. However, I also suggest that such acts of repression are never successful; they reveal the contingency of the present upon the past, and forever unsettle the location of white people in Australia.Damien W. Rigg

Enhanced Fermi surface nesting in superconducting BaFe2_2(As1−x_{1-x}Px_x)2_2 revealed by de Haas-van Alphen effect

The three-dimensional Fermi surface morphology of superconducting BaFe_2(As_0.37}P_0.63)_2 with T_c=9K, is determined using the de Haas-van Alphen effect (dHvA). The inner electron pocket has a similar area and k_z interplane warping to the observed hole pocket, revealing that the Fermi surfaces are geometrically well nested in the (\pi,\pi) direction. These results are in stark contrast to the Fermiology of the non-superconducting phosphides (x=1), and therefore suggests an important role for nesting in pnictide superconductivity.Comment: 5 pages, 4 figure

Interiors : works by Gregor Bell, Geoff Kleem, Ted Riggs, Derek Smith, Alex Wanders, Geoff Weary

Interiors : works by Gregor Bell, Geoff Kleem, Ted Riggs, Derek Smith, Alex Wanders, Geoff Wear

Quantum oscillations in the parent pnictide BaFe2_2As2_2 : itinerant electrons in the reconstructed state

We report quantum oscillation measurements that enable the direct observation of the Fermi surface of the low temperature ground state of \ba122. From these measurements we characterize the low energy excitations, revealing that the Fermi surface is reconstructed in the antiferromagnetic state, but leaving itinerant electrons in its wake. The present measurements are consistent with a conventional band folding picture of the antiferromagnetic ground state, placing important limits on the topology and size of the Fermi surface.Comment: 5 pages, 3 figure

COMPUTABLE GENERAL EQUILIBRIUM MODELING OF RANGELAND FIRES IN NORTHERN NEVADA

Resource /Energy Economics and Policy,

RANGELAND FIRES IN NORTHERN NEVADA: AN APPLICATION OF COMPUTABLE GENERAL EQUILIBRIUM MODELING

Resource /Energy Economics and Policy,

Operating and maintaining underground outlet terrace systems (1993)

The proper operation of underground outlet terrace systems depends on good farming practices, frequent inspections and prompt correction of problems. Inspect your systems soon after each significant rainfall. This is the best time to see existing or potential problems. Plainly marked inlets and outlets make this chore easy. Timely repairs or replacements normally lower maintenance costs, increase the life of the system and prevent serious problems

The Overlooked Potential of Generalized Linear Models in Astronomy-III: Bayesian Negative Binomial Regression and Globular Cluster Populations

In this paper, the third in a series illustrating the power of generalized linear models (GLMs) for the astronomical community, we elucidate the potential of the class of GLMs which handles count data. The size of a galaxy's globular cluster population $N_{\rm GC}$ is a prolonged puzzle in the astronomical literature. It falls in the category of count data analysis, yet it is usually modelled as if it were a continuous response variable. We have developed a Bayesian negative binomial regression model to study the connection between $N_{\rm GC}$ and the following galaxy properties: central black hole mass, dynamical bulge mass, bulge velocity dispersion, and absolute visual magnitude. The methodology introduced herein naturally accounts for heteroscedasticity, intrinsic scatter, errors in measurements in both axes (either discrete or continuous), and allows modelling the population of globular clusters on their natural scale as a non-negative integer variable. Prediction intervals of 99% around the trend for expected $N_{\rm GC}$comfortably envelope the data, notably including the Milky Way, which has hitherto been considered a problematic outlier. Finally, we demonstrate how random intercept models can incorporate information of each particular galaxy morphological type. Bayesian variable selection methodology allows for automatically identifying galaxy types with different productions of GCs, suggesting that on average S0 galaxies have a GC population 35% smaller than other types with similar brightness.Comment: 14 pages, 12 figures. Accepted for publication in MNRA