4,521 research outputs found

    Increasing the Size of a Piece of Popcorn

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    Popcorn is an extremely popular snack food in the world today. Thermodynamics can be used to analyze how popcorn is produced. By treating the popping mechanism of the corn as a thermodynamic expansion, a method of increasing the volume or size of a kernel of popcorn can be studied. By lowering the pressure surrounding the unpopped kernel, one can use a thermodynamic argument to show that the expanded volume of the kernel when it pops must increase. In this project, a variety of experiments are run to test the validity of this theory. The results show that there is a significant increase in the average kernel size when the pressure of the surroundings is reduced.Comment: Latex document, 14 pages, 4 figures, 1 page of table

    Human epicardial adipose tissue expresses a pathogenic profile of adipocytokines in patients with cardiovascular disease

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    Introduction: Inflammation contributes to cardiovascular disease and is exacerbated with increased adiposity, particularly omental adiposity; however, the role of epicardial fat is poorly understood. Methods: For these studies the expression of inflammatory markers was assessed in epicardial fat biopsies from coronary artery bypass grafting (CABG) patients using quantitative RT-PCR. Further, the effects of chronic medications, including statins, as well as peri-operative glucose, insulin and potassium infusion, on gene expression were also assessed. Circulating resistin, CRP, adiponectin and leptin levels were determined to assess inflammation. Results: The expression of adiponectin, resistin and other adipocytokine mRNAs were comparable to that in omental fat. Epicardial CD45 expression was significantly higher than control depots (p < 0.01) indicating significant infiltration of macrophages. Statin treated patients showed significantly lower epicardial expression of IL-6 mRNA, in comparison with the control abdominal depots (p < 0.001). The serum profile of CABG patients showed significantly higher levels of both CRP (control: 1.28 ± 1.57 μg/mL vs CABG: 9.11 ± 15.7 μg/mL; p < 0.001) and resistin (control: 10.53 ± 0.81 ng/mL vs CABG: 16.8 ± 1.69 ng/mL; p < 0.01) and significantly lower levels of adiponectin (control: 29.1 ± 14.8 μg/mL vs CABG: 11.9 ± 6.0 μg/mL; p < 0.05) when compared to BMI matched controls. Conclusion: Epicardial and omental fat exhibit a broadly comparable pathogenic mRNA profile, this may arise in part from macrophage infiltration into the epicardial fat. This study highlights that chronic inflammation occurs locally as well as systemically potentially contributing further to the pathogenesis of coronary artery disease

    The effect of distance on reaction time in aiming movements

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    Target distance affects movement duration in aiming tasks but its effect on reaction time (RT) is poorly documented. RT is a function of both preparation and initiation. Experiment 1 pre-cued movement (allowing advanced preparation) and found no influence of distance on RT. Thus, target distance does not affect initiation time. Experiment 2 removed pre-cue information and found that preparing a movement of increased distance lengthens RT. Experiment 3 explored movements to targets of cued size at non-cued distances and found size altered peak speed and movement duration but RT was influenced by distance alone. Thus, amplitude influences preparation time (for reasons other than altered duration) but not initiation time. We hypothesise that the RT distance effect might be due to the increased number of possible trajectories associated with further targets: a hypothesis that can be tested in future experiments

    Mechanisms Underlying the Delayed Activation of the Cap1 Transcription Factor in Candida albicans following Combinatorial Oxidative and Cationic Stress Important for Phagocytic Potency

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    ACKNOWLEDGMENTS We are grateful to Brian Morgan and Elizabeth Veal for insightful discussions, Mélanie Ikeh for experimental assistance, and Scott Moye-Rowley (University of Iowa) for the gift of the anti-Cap1 antibody. This work was funded by the NIHR Newcastle Biomedical Research Centre (I.K.), a BBSRC DTG studentship (M.J.P.), the Wellcome Trust (grants 089930 and 097377 to J.Q. and 080088 and 097377 to A.J.P.B.), the BBSRC (grants BB/K016393/1 to J.Q. and BB/F00513X/1 and BB/K017365/1 to A.J.P.B.), the European Research Council (STRIFE Advanced grant ERC-2009-AdG-249793 to A.J.P.B.), the ANR (grant CANDIHUB, ANR-14-CE14-0018-01, to C.D.), and the French Government’s Investissement d’Avenir program (grant IBEID, ANR-10-LABX-62-IBEID, to C.D.). FUNDING INFORMATION This work, including the efforts of Alistair J.P. Brown, was funded by Wellcome Trust (097377 and 080088). This work, including the efforts of Janet Quinn, was funded by Wellcome Trust (097377 and 089930). This work, including the efforts of Alistair J.P. Brown, was funded by EC European Research Council (ERC) (ERC-2009-AdG-249793). This work, including the efforts of Alistair J.P. Brown, was funded by Biotechnology and Biological Sciences Research Council (BBSRC) (BB/F00513X/1 and BB/K017365/1). This work, including the efforts of Janet Quinn, was funded by Biotechnology and Biological Sciences Research Council (BBSRC) (BB/K016393/1). This work, including the efforts of Christophe d’Enfert, was funded by Agence Nationale de la Recherche (ANR) (ANR-14-CE14-0018-01 and ANR-10-LABX-62-IBEID).Peer reviewedPublisher PD

    HIV Prevention in Care and Treatment Settings: Baseline Risk Behaviors among HIV Patients in Kenya, Namibia, and Tanzania.

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    HIV care and treatment settings provide an opportunity to reach people living with HIV/AIDS (PLHIV) with prevention messages and services. Population-based surveys in sub-Saharan Africa have identified HIV risk behaviors among PLHIV, yet data are limited regarding HIV risk behaviors of PLHIV in clinical care. This paper describes the baseline sociodemographic, HIV transmission risk behaviors, and clinical data of a study evaluating an HIV prevention intervention package for HIV care and treatment clinics in Africa. The study was a longitudinal group-randomized trial in 9 intervention clinics and 9 comparison clinics in Kenya, Namibia, and Tanzania (N = 3538). Baseline participants were mostly female, married, had less than a primary education, and were relatively recently diagnosed with HIV. Fifty-two percent of participants had a partner of negative or unknown status, 24% were not using condoms consistently, and 11% reported STI symptoms in the last 6 months. There were differences in demographic and HIV transmission risk variables by country, indicating the need to consider local context in designing studies and using caution when generalizing findings across African countries. Baseline data from this study indicate that participants were often engaging in HIV transmission risk behaviors, which supports the need for prevention with PLHIV (PwP). TRIAL REGISTRATION: ClinicalTrials.gov NCT01256463

    Feedback and the Formation of Dwarf Galaxy Stellar Halos

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    Stellar population studies show that low mass galaxies in all environments exhibit stellar halos that are older and more spherically distributed than the main body of the galaxy. In some cases, there is a significant intermediate age component that extends beyond the young disk. We examine a suite of Smoothed Particle Hydrodynamic (SPH) simulations and find that elevated early star formation activity combined with supernova feedback can produce an extended stellar distribution that resembles these halos for model galaxies ranging from v200v_{200} = 15 km s1^{-1} to 35 km s1^{-1}, without the need for accretion of subhalos.Comment: 15 pages, 15 figures, accepted MNRA

    Statistical characteristics of formation and evolution of structure in the universe

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    An approximate statistical description of the formation and evolution of structure of the universe based on the Zel'dovich theory of gravitational instability is proposed. It is found that the evolution of DM structure shows features of self-similarity and the main structure characteristics can be expressed through the parameters of initial power spectrum and cosmological model. For the CDM-like power spectrum and suitable parameters of the cosmological model the effective matter compression reaches the observed scales RwallR_{wall}\sim 20 -- 25h1h^{-1}Mpc with the typical mean separation of wall-like elements DSLSSD_{SLSS}\sim 50 -- 70h1h^{-1}Mpc. This description can be directly applied to the deep pencil beam galactic surveys and absorption spectra of quasars. For larger 3D catalogs and simulations it can be applied to results obtained with the core-sampling analysis. It is shown that the interaction of large and small scale perturbations modulates the creation rate of early Zel'dovich pancakes and generates bias on the SLSS scale. For suitable parameters of the cosmological model and reheating process this bias can essentially improve the characteristics of simulated structure of the universe. The models with 0.3Ωm0.50.3\leq \Omega_m \leq 0.5 give the best description of the observed structure parameters. The influence of low mass "warm" dark matter particles, such as a massive neutrino, will extend the acceptable range of Ωm\Omega_m and hh.Comment: 20pages, 7 figures, MNRAS in pres
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