Donor behavior in indium-alloyed silicon

The anomalous doping behavior of Si regrown from In solution was studied by (1) Schottky barrier evaluation of conductivity type, (2) electron microprobe analysis for phosphorus, and (3) channeling effect measurements for interstitial In. The latter showed In present at ~ 10^19 cm^–3, but not occupying a regular substitutional or interstitial position. A correlation was found in the first two measurements between phosphorus contamination and n-type conductivity. When the In was contacted only by quartz freshly etched in HF, the n-type behavior and phosphorus contamination disappeared. The anomalous doping behavior is most likely due to phosphorus inpurity picked up by the In

Corporate Governance in the Cause of Peace: An Environmental Perspective

This Article examines the role of multinational corporations in creating global peace. Part I discusses the role of multinational corporations in the global economy, emphasizing the relationship between multinational corporations, governments, and the environment. Part II explores whether corporations have a moral duty to oppose ill-conceived laws and policy proposals and to support well-conceived laws that encourage efficiency and sustainability, but may hinder short-term profitability. Part III expands and further explores the argument set forth in Part II by examining the continuing dependency of the United States and other industrialized democracies on oil from the Middle East. Part IV concludes the Article by noting that multinational corporations have both the power and responsibility to create products and services that materially enhance human well-being by preserving the natural environment

The stability of the O(N) invariant fixed point in three dimensions

We study the stability of the O(N) fixed point in three dimensions under perturbations of the cubic type. We address this problem in the three cases $N=2,3,4$ by using finite size scaling techniques and high precision Monte Carlo simulations. It is well know that there is a critical value $2<N_c<4$ below which the O(N) fixed point is stable and above which the cubic fixed point becomes the stable one. While we cannot exclude that $N_c<3$, as recently claimed by Kleinert and collaborators, our analysis strongly suggests that $N_c$ coincides with 3.Comment: latex file of 18 pages plus three ps figure

Eight fields of MATCEMIB help students to generate more ideas

This paper presents the results of the idea generation experiment that repeats the study originally conducted at RMIT. In order to establish the influence that the experimental treatments make on the number and the breadth of solution ideas proposed by problem solvers with different knowledge levels, students from different years of study were recruited. Ninety students from the Offenburg University of Applied Sciences, Germany were divided into three groups. All students were asked to generate ideas on cleaning lime deposits from the inside of a water pipe and were given 16 minutes to record their individual ideas. Students of two experimental groups were shown some words for two minuted each. The Su-Field group was exposed to the eight fields of MATCEMIB. The Random Word group was shown eight random words every two minutes. The Su-Field group outperformed both the Control group and the Random Word group in the number of ideas generated. It was also found that the students from the Su-Field group proposed significantly broader solutions than the students from the Control and Random Word groups. The overall results of the experiment support the conclusions made by the RMIT researchers that simple ideation techniques can significantly improve idea generation and that the systematised Substance-Field Analysis is a suitable heuristic for engineering students

Educating a creative engineer: learning from engineering professionals

The rapid growth of engineering knowledge has resulted in continuous expansion of novel technologies and materials that can be used in designing new products and processed. Computer- and web-based technologies allowed engineers to significantly shorten the development of novel artefacts. These advances intensified the competition between engineering companies and shortened the lifespans of the majority of engineering products. As a result, practicing engineers are now expected to deliver creative designs to markets much more swiftly than ever before. This paper presents the results of a survey that intended to establish the ways and the means of enhancing engineering creativity that suit the engineering industry of the 21st Century. This study engaged 46 engineering experts from the major international corporations who utilised numerous creativity techniques including TRIZ in their day-to-day engineering work. It had been found that the surveyed engineering experts think that in the current Information age (i) knowledge beyond engineering profession is more important for creativity than the discipline knowledge; (ii) learning creativity methods and problem solving heuristics is more important than acquiring additional discipline knowledge; (iii) the problem solving stage of identifying and understanding a problem is the key to a creative solution

Forming Disk Galaxies in Lambda CDM Simulations

We used fully cosmological, high resolution N-body + SPH simulations to follow the formation of disk galaxies with rotational velocities between 135 and 270 km/sec in a Lambda CDM universe. The simulations include gas cooling, star formation, the effects of a uniform UV background and a physically motivated description of feedback from supernovae. The host dark matter halos have a spin and last major merger redshift typical of galaxy sized halos as measured in recent large scale N--Body simulations. The simulated galaxies form rotationally supported disks with realistic exponential scale lengths and fall on both the I-band and baryonic Tully Fisher relations. An extended stellar disk forms inside the Milky Way sized halo immediately after the last major merger. The combination of UV background and SN feedback drastically reduces the number of visible satellites orbiting inside a Milky Way sized halo, bringing it in fair agreement with observations. Our simulations predict that the average age of a primary galaxy's stellar population decreases with mass, because feedback delays star formation in less massive galaxies. Galaxies have stellar masses and current star formation rates as a function of total mass that are in good agreement with observational data. We discuss how both high mass and force resolution and a realistic description of star formation and feedback are important ingredients to match the observed properties of galaxies.Comment: Revised version after the referee's comments. Conclusions unchanged. 2 new plots. MNRAS in press. 20 plots. 21 page