High temperature reliability of power module substrates

The thermal cycling reliability of candidate copper and aluminium power substrates has been assessed for use at temperatures exceeding 300°C peak using a combination of thermal cycling, nanoindentation and finite element modelling to understand the relative stresses and evolution of the mechanical properties. The results include the relative cycling lifetimes up to 350°C, demonstrating almost an order of magnitude higher lifetime for active metal brazed Al / AlN substrates over Cu / Si3N4, but four times more severe roughening and cracking of the Ni-P plating's on the Al / AlN (DBA) substrates. The nonlinear finite element modelling illustrated that the yield strength of the metal and the thickness of the ceramic are the main stress controlling factors, but comparisons with the cycling lifetime results demonstrated that the fracture toughness (resistance) of the ceramic is the over-riding controlling factor for the overall passive thermal cycling lifetimes. In order to achieve the highest substrate lifetime for the highly stressed high temperature thermal cycled applications, the optimum solution appears to be annealed copper, brazed on to a thicker than normal or higher fracture toughness Si3N4 ceramic

Force-Free Gravitational Redshift: Proposed Gravitational Aharonov-Bohm experiment

We propose a feasible laboratory interferometry experiment with matter waves in a gravitational potential caused by a pair of artificial field-generating masses. It will demonstrate that the presence of these masses (and, for moving atoms, time dilation) induces a phase shift, even if it does not cause any classical force. The phase shift is identical to that produced by the gravitational redshift (or time dilation) of clocks ticking at the atom's Compton frequency. In analogy to the Aharonov-Bohm effect in electromagnetism, the quantum mechanical phase is a function of the gravitational potential and not the classical forces.Comment: Updated to published versio

Are methodological quality and completeness of reporting associated with citation-based measures of publication impact? A secondary analysis of a systematic review of dementia biomarker studies

Objective: To determine whether methodological and reporting quality are associated with surrogate measures of publication impact in the field of dementia biomarker studies. Methods: We assessed dementia biomarker studies included in a previous systematic review in terms of methodological and reporting quality using the Quality Assessment of Diagnostic Accuracy Studies (QUADAS) and Standards for Reporting of Diagnostic Accuracy (STARD), respectively. We extracted additional study and journal-related data from each publication to account for factors shown to be associated with impact in previous research. We explored associations between potential determinants and measures of publication impact in univariable and stepwise multivariable linear regression analyses. Outcome measures: We aimed to collect data on four measures of publication impact: two traditional measures—average number of citations per year and 5-year impact factor of the publishing journal and two alternative measures—the Altmetric Attention Score and counts of electronic downloads. Results: The systematic review included 142 studies. Due to limited data, Altmetric Attention Scores and electronic downloads were excluded from the analysis, leaving traditional metrics as the only analysed outcome measures. We found no relationship between QUADAS and traditional metrics. Citation rates were independently associated with 5-year journal impact factor (β=0.42; p<0.001), journal subject area (β=0.39; p<0.001), number of years since publication (β=-0.29; p<0.001) and STARD (β=0.13; p<0.05). Independent determinants of 5-year journal impact factor were citation rates (β=0.45; p<0.001), statement on conflict of interest (β=0.22; p<0.01) and baseline sample size (β=0.15; p<0.05). Conclusions: Citation rates and 5-year journal impact factor appear to measure different dimensions of impact. Citation rates were weakly associated with completeness of reporting, while neither traditional metric was related to methodological rigour. Our results suggest that high publication usage and journal outlet is not a guarantee of quality and readers should critically appraise all papers regardless of presumed impact

Determination of the Baryon Density from Large Scale Galaxy Redshift Surveys

We estimate the degree to which the baryon density, $\Omega_{b}$, can be determined from the galaxy power spectrum measured from large scale galaxy redshift surveys, and in particular, the Sloan Digital Sky Survey. A high baryon density will cause wiggles to appear in the power spectrum, which should be observable at the current epoch. We assume linear theory on scales $\geq 20h^{-1}Mpc$ and do not include the effects of redshift distortions, evolution, or biasing. With an optimum estimate of $P(k)$ to $k\sim 2\pi/(20 h^{-1} Mpc)$, the $1 \sigma$ uncertainties in $\Omega_{b}$ are roughly 0.07 and 0.016 in flat and open ($\Omega_{0}=0.3$) cosmological models, respectively. This result suggests that it should be possible to test for consistency with big bang nucleosynthesis estimates of $\Omega_{b}$ if we live in an open universe.Comment: 23 Pages, 10 Postscript figure

Statewide Policy Advocacy Intervention in California: The No Time for Complacency Initiative

California has made substantial progress since 1991 in reducing its teen birth rate, and its rate reduction now leads the nation. Yet more than 50,000 Californian teens continue to give birth each year, and many more became pregnant. And due to changing demographics and the recent reversal in the last decade’s poverty rate declines, California’s improvements are at risk. The No Time for Complacency (NTFC) initiative is a policy advocacy intervention designed to promote effective statewide teen pregnancy prevention policy and funding in California. This initiative employs legislative-district data analysis to provide a politically compelling organization of teen birth data, cost analyses to heighten the societal relevance of teen births, policy analysis to identify promising and effective state policies, and media advocacy to focus attention on these issues in all regions of the state. The process and results described show how it was possible to achieve impacts on state-level health policy and program funding

Intermediate Mass Black Hole Induced Quenching of Mass Segregation in Star Clusters

In many theoretical scenarios it is expected that intermediate-mass black holes (IMBHs, with masses M ~ 100-10000 solar masses) reside at the centers of some globular clusters. However, observational evidence for their existence is limited. Several previous numerical investigations have focused on the impact of an IMBH on the cluster dynamics or brightness profile. Here we instead present results from a large set of direct N-body simulations including single and binary stars. These show that there is a potentially more detectable IMBH signature, namely on the variation of the average stellar mass between the center and the half-light radius. We find that the existence of an IMBH quenches mass segregation and causes the average mass to exhibit only modest radial variation in collisionally relaxed star clusters. This differs from when there is no IMBH. To measure this observationally requires high resolution imaging at the level of that already available from the Hubble Space Telescope (HST) for the cores of a large sample of galactic globular clusters. With a modest additional investment of HST time to acquire fields around the half-light radius, it will be possible to identify the best candidate clusters to harbor an IMBH. This test can be applied only to globulars with a half-light relaxation time less than or equal to 1 Gyr, which is required to guarantee efficient energy equipartition due to two-body relaxation.Comment: 15 pages, 3 figures, ApJ, in pres

Planetary astronomy

The authors profile the field of astronomy, identify some of the key scientific questions that can be addressed during the decade of the 1990's, and recommend several facilities that are critically important for answering these questions. Scientific opportunities for the 1990' are discussed. Areas discussed include protoplanetary disks, an inventory of the solar system, primitive material in the solar system, the dynamics of planetary atmospheres, planetary rings and ring dynamics, the composition and structure of the atmospheres of giant planets, the volcanoes of IO, and the mineralogy of the Martian surface. Critical technology developments, proposed projects and facilities, and recommendations for research and facilities are discussed

Characterizing the Microeconomic Decision Factors of Energy Efficient Commercial Building Retrofits

Engineering analyses have claimed that the implementation of retrofits in existing buildings can significantly reduce their energy consumption and generate cost savings for owners – yet such investment in energy efficiency has been minimal by many standards. The primary goal of this thesis is to identify and quantify the factors affecting stakeholders' decisions to adopt (or not adopt) energy conservation measures during commercial building retrofits, and then to suggest ways in which these decision processes can be improved through policy instruments. Chapter I presents a literature review of previous research on the subject and explains the theoretical basis of the "energy-efficiency gap." Chapter II presents findings from a set of surveys in order to clarify the major determinants of the commercial energy-efficient building retrofit decision – and uses these data to make observations of differences in retrofit investment preferences between different types of organizations and leasing structures. Chapter III summarizes the implications of the first two chapters and suggests possible policy-based solutions to encourage increased attention to energy efficiency in the commercial building sector. Results from the surveys conducted for this study are shown to be generally in agreement with a third data source, the Johnson Controls Energy Efficiency 2011 Indicator survey. The relative importance of various financial metrics (such as simple payback period) in stakeholders' decision processes is quantified and the ability to alter the outcomes of these processes via the addition of new financial information is documented. It is found that stakeholders' behavior may be partially explained by their beliefs in the future cost of energy, which they expect will decrease in real terms over the next 20 years (though significant variation does exist in these perceptions). An approximate quantitative measure of "split incentives" is obtained and differences in its effect between different organization ownership structures are outlined. Together, the data presented in this thesis suggest that an "energy efficiency gap" does exist, though to a smaller degree than have been suggested by some. Specific policy solutions to increase investment in energy efficiency are recommended, including 1) targeting nonprofit and government organizations to act as "early adopters," 2) the creation of a thirdparty database with cost and performance information for ECMs, and 3) the widespread adoption of on-bill financing.M.S., Environmental Engineering -- Drexel University, 201