Candida albicans Is Resistant to Polyglutamine Aggregation and Toxicity

Acknowledgments We thank the Donnelly Sequencing Centre for sequencing, and Jonathan Krieger at the SikKids Proteomics, Analytics, Robotics & Chemical Biology Centre at The Hospital for Sick Children for mass spectrometry analysis. M.D.L. is supported by a Sir Henry Wellcome Postdoctoral Fellowship (Wellcome Trust grant 096072), T.K. is supported by a Queen Elizabeth II Graduate Scholarship in Science and Technology (University of Toronto), M.L.D. is supported by a Canadian Institutes of Health Research (CIHR) Operating grant 325538, L.E.C. is supported by a Canada Research Chair in Microbial Genomics and Infectious Disease, by CIHR grants MOP-119520 and MOP-86452, and by the Natural Sciences and Engineering Research Council (NSERC) of Canada (grants 06261 and 462167).Peer reviewedPublisher PD

Quantum Tunneling in Nuclear Fusion

Recent theoretical advances in the study of heavy ion fusion reactions below the Coulomb barrier are reviewed. Particular emphasis is given to new ways of analyzing data, such as studying barrier distributions; new approaches to channel coupling, such as the path integral and Green function formalisms; and alternative methods to describe nuclear structure effects, such as those using the Interacting Boson Model. The roles of nucleon transfer, asymmetry effects, higher-order couplings, and shape-phase transitions are elucidated. The current status of the fusion of unstable nuclei and very massive systems are briefly discussed.Comment: To appear in the January 1998 issue of Reviews of Modern Physics. 13 Figures (postscript file for Figure 6 is not available; a hard copy can be requested from the authors). Full text and figures are also available at http://nucth.physics.wisc.edu/preprints

Gallium Solar Neutrino Experiments: Absorption Cross sections, Neutrino spectra, and Predicted Event Rates

Neutrino absorption cross sections for 71Ga are calculated for all solar neutrino sources with standard energy spectra, and for laboratory sources of 51Cr and 37Ar; the calculations include, where appropriate, the thermal energy of fusing solar ions and use improved nuclear and atomic data. The ratio, R, of measured (in GALLEX and SAGE) to calculated 51Cr capture rate is R = 0.95 +/- 0.07 (exp)} + ^{+0.04}_{-0.03} (theory). Cross sections are also calculated for specific neutrino energies chosen so that a spline fit determines accurately the event rates in a gallium detector even if new physics changes the energy spectrum of solar neutrinos. Theoretical uncertainties are estimated for cross sections at specific energies and for standard neutrino energy spectra. Standard energy spectra are presented for pp and CNO neutrino sources in the appendices. Neutrino fluxes predicted by standard solar models, corrected for diffusion, have been in the range 120 SNU to 141 SNU since 1968.Comment: 57 pages, ReVTeX file. Accepted for publication in Phys. Rev. C. Viewgraphs and numerical tables of neutrino spectra and cross sections at http://www.sns.ias.edu/~jn

A Glial Variant of the Vesicular Monoamine Transporter Is Required To Store Histamine in the Drosophila Visual System

Unlike other monoamine neurotransmitters, the mechanism by which the brain's histamine content is regulated remains unclear. In mammals, vesicular monoamine transporters (VMATs) are expressed exclusively in neurons and mediate the storage of histamine and other monoamines. We have studied the visual system of Drosophila melanogaster in which histamine is the primary neurotransmitter released from photoreceptor cells. We report here that a novel mRNA splice variant of Drosophila VMAT (DVMAT-B) is expressed not in neurons but rather in a small subset of glia in the lamina of the fly's optic lobe. Histamine contents are reduced by mutation of dVMAT, but can be partially restored by specifically expressing DVMAT-B in glia. Our results suggest a novel role for a monoamine transporter in glia that may be relevant to histamine homeostasis in other systems

Modelling human choices: MADeM and decision‑making

Research supported by FAPESP 2015/50122-0 and DFG-GRTK 1740/2. RP and AR are also part of the Research, Innovation and Dissemination Center for Neuromathematics FAPESP grant (2013/07699-0). RP is supported by a FAPESP scholarship (2013/25667-8). ACR is partially supported by a CNPq fellowship (grant 306251/2014-0)

Can anodal stimulation contribute to cardiac resynchronization?

In order to increase intraventricular synchronization, dual-site activation of the left ventricle (LV) could be achieved by a bipolar lead capable of both cathodal and anodal capture. However, anodal pulses might imply a higher arrhythmic risk than cathodal pulses, due to a lower threshold in the vulnerable period. In the aim of increasing LV stimulation safety, we studied end-diastolic anodal activation in the rat heart. Epicardial isopotential and isochrone maps revealed two mechanisms of anodal excitation: i) at threshold, at the pacing site, after 5-12 ms from the pulse onset (anode break); ii) at higher current intensities after 3-5 ms (anode make), in two symmetric regions 1 mm from pacing site along fibres, corresponding to the virtual cathodes of the bidomain model. Whole cell patch clamp demonstrated that break excitation is mainly sustained by a depolarizing current activated in hyperpolarization (ih), which slowly deactivates after the pulse offset. Break excitation is likely to explain the reduced anodal threshold in the vulnerable period. Stimulation modalities that could prevent the anode break response, while still allowing “make” activation in the virtual cathodes, are under investigation