497 research outputs found

    Query Theory Applications: Choice Experiments under Oath, Attendance to Attributes, and Genetically Modified Food Labeling Policy

    Get PDF
    In recent years, there has been an intensifying campaign by some stakeholders regarding concern over genetically modified (GM) foods in the U.S. As a result, the issue of labeling has entered into the federal agenda. This research uses Query Theory to provide a deeper understanding of the demand for GM foods and the preferences for GM policy. Query theory is first applied to the formation of hypothetical bias in the estimation of consumers’ willingness-to-pay. To address this, the honesty oath is used as an ex-ante technique to reduce hypothetical bias. Paper one using Query Theory in a discrete-choice experiment (DCE) setting to examine the mechanism behind the effectiveness of the honesty oath in reducing hypothetical bias in discrete choice experiments. Our results show that the honesty oath can change the content and order of queries, thereby reducing hypothetical bias in discrete choice experiments. In the second paper, Query Theory is used to examine the thought processes of individuals in a DCE in order to deduce attendance to individual attributes. Respondents may attend some attributes of the good in question and ignore others during each choice task. As a result, respondents may not make the trade-offs between all the attributes as assumed. The results show that the query approach to modeling attendance to attributes outperforms two other common approaches: the stated and inferred approaches. Finally, in paper three, Query Theory is applied to the study of the influence of cultural worldview on the demand for GM foods policy in the U.S. Our results demonstrate that an individual’s cultural worldview influences their preferences for GM policy and consumer valuations. The results also support our Query Theory prediction that cultural worldview influences individual’s affective reactions to choice options leading to significantly different valuations. Though important differences do exist between individuals with different CWVs, there is common ground as well. Support for mandatory labeling is high with 82 percent of respondents indicating support for mandatory labeling which ranged from 71 percent to 88 percent, depending on CWV

    Documenting Teaching Effectiveness

    Get PDF
    In this presentation, three veteran faculty members discuss how faculty can document their teaching effectiveness for purposes of annual reviews, awards, and promotion

    Molecular identification and targeting of colorectal cancer stem cells

    Get PDF
    Tumor initiating or cancer stem cells (CSCs) are suggested to be responsible for tumor initiation and growth. Moreover, therapy resistance and minimal residual disease are thought to result from selective resistance of CSCs. Isolation of CSCs from colon carcinomas can be accomplished by selection of a subpopulation of tumor cells based on expression of one or multiple cell surface markers associated with cancer stemness, like CD133, CD44, CD24, CD29, CD166 and Lgr5. Identification of colon CSCs will lead to a better rational for new therapies that aim to target this fraction specifically. In this review, we analyze known markers used for selection of colon CSCs and their potential function in CSC biology. Moreover, we discuss potential targeting strategies for eradicating CSCs specifically in order to develop more effective therapeutic strategies as well as to address more fundamental questions like the actual role of CSCs in tumor growth

    Analysis of Experimental Nucleation Data for Silver and SiO Using Scaled Nucleation Theory

    Get PDF
    The experimental vapor phase nucleation data of Nuth et al., for silver [J. A. Nuth, K. A. Donnelly, B. Donn, and L. U. Lilleleht, J. Chem. Phys. 77, 2639 (1982)] and SiO [J. A. Nuth and B. Donn, J. Chem. Phys. 85, 1116 (1986)] are reanalyzed using a scaled model for homogeneous nucleation [B. N. Hale, Phys. Rev. A 33, 4156 (1986)]. The approximation is made that the vapor pressure at the nucleation site is not diminished significantly from that at the source (crucible). It is found that the data for ln S have a temperature dependence consistent with the scaled theory ln S≈ΓΩ3/2 [Tc /T-1]3/2, and predict critical temperatures 3800 ± 200 K for silver and 3700 ± 200 K for SiO. One can also extract an effective excess surface entropy per atom Ω = 2.1 ± 0.1 and an effective surface tension σ ≈ 1500 - 0.45 T ergs/cm2 for the small silver clusters (assuming a range of nucleation rates from 105 to 1011 cm-3 s-1). The corresponding values for SiO are Ω ≈ 1.7 ± 0.1 and σ ≈ 820 - 0.22 T ergs/cm2 (assuming a range of nucleation rates from 109 to 1012 cm-3 s-1)

    The Chemistry of Extragalactic Carbon Stars

    Get PDF
    Prompted by the ongoing interest in Spitzer Infrared Spectrometer spectra of carbon stars in the Large Magellanic Cloud, we have investigated the circumstellar chemistry of carbon stars in low-metallicity environments. Consistent with observations, our models show that acetylene is particularly abundant in the inner regions of low metallicity carbon-rich asymptotic giant branch stars - more abundant than carbon monoxide. As a consequence, larger hydrocarbons have higher abundances at the metallicities of the Magellanic Clouds than in stars with solar metallicity. We also find that the oxygen and nitrogen chemistry is suppressed at lower metallicity, as expected. Finally, we calculate molecular line emission from carbon stars in the Large and Small Magellanic Cloud and find that several molecules should be readily detectable with the Atacama Large Millimeter Array at Full Science operations

    On the metallicity dependence of crystalline silicates in oxygen-rich asymptotic giant branch stars and red supergiants

    Full text link
    We investigate the occurrence of crystalline silicates in oxygen-rich evolved stars across a range of metallicities and mass-loss rates. It has been suggested that the crystalline silicate feature strength increases with increasing mass-loss rate, implying a correlation between lattice structure and wind density. To test this, we analyse Spitzer IRS and Infrared Space Observatory SWS spectra of 217 oxygen-rich asymptotic giant branch stars and 98 red supergiants in the Milky Way, the Large and Small Magellanic Clouds and Galactic globular clusters. These encompass a range of spectral morphologies from the spectrally-rich which exhibit a wealth of crystalline and amorphous silicate features to 'naked' (dust-free) stars. We combine spectroscopic and photometric observations with the GRAMS grid of radiative transfer models to derive (dust) mass-loss rates and temperature. We then measure the strength of the crystalline silicate bands at 23, 28 and 33 microns. We detect crystalline silicates in stars with dust mass-loss rates which span over 3 dex, down to rates of ~10^-9 solar masses/year. Detections of crystalline silicates are more prevalent in higher mass-loss rate objects, though the highest mass-loss rate objects do not show the 23-micron feature, possibly due to the low temperature of the forsterite grains or it may indicate that the 23-micron band is going into absorption due to high column density. Furthermore, we detect a change in the crystalline silicate mineralogy with metallicity, with enstatite seen increasingly at low metallicity.Comment: Accepted for publication in MNRAS, 24 pages, 16 figure
    • …
    corecore