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  • Articles  (3,472)
  • Nature Publishing Group (NPG)  (3,472)
  • 2015-2019  (3,472)
  • Natural Sciences in General  (3,472)
  • Energy, Environment Protection, Nuclear Power Engineering
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  • Articles  (3,472)
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  • 1
    Publication Date: 2016-05-27
    Description: 〈br /〉〈span class="detail_caption"〉Notes: 〈/span〉Cappa, Chris -- England -- Nature. 2016 May 25;533(7604):478-9. doi: 10.1038/533478a.〈br /〉〈span class="detail_caption"〉Author address: 〈/span〉Department of Civil and Environmental Engineering, University of California, Davis, Davis, California 95616, USA.〈br /〉〈span class="detail_caption"〉Record origin:〈/span〉 〈a href="http://www.ncbi.nlm.nih.gov/pubmed/27225118" target="_blank"〉PubMed〈/a〉
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    Topics: Biology , Chemistry and Pharmacology , Medicine , Natural Sciences in General , Physics
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  • 2
    Publication Date: 2016-05-27
    Description: 〈br /〉〈span class="detail_caption"〉Notes: 〈/span〉Ott, Martin -- England -- Nature. 2016 May 11;533(7604):472-3. doi: 10.1038/nature18436.〈br /〉〈span class="detail_caption"〉Author address: 〈/span〉Center for Biomembrane Research, Department of Biochemistry and Biophysics, Stockholm University, SE-106 91 Stockholm, Sweden.〈br /〉〈span class="detail_caption"〉Record origin:〈/span〉 〈a href="http://www.ncbi.nlm.nih.gov/pubmed/27225113" target="_blank"〉PubMed〈/a〉
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  • 3
    Publication Date: 2016-05-27
    Description: In many animal societies where hierarchies govern access to reproduction, the social rank of individuals is related to their age and weight and slow-growing animals may lose their place in breeding queues to younger 'challengers' that grow faster. The threat of being displaced might be expected to favour the evolution of competitive growth strategies, where individuals increase their own rate of growth in response to increases in the growth of potential rivals. Although growth rates have been shown to vary in relation to changes in the social environment in several vertebrates including fish and mammals, it is not yet known whether individuals increase their growth rates in response to increases in the growth of particular reproductive rivals. Here we show that, in wild Kalahari meerkats (Suricata suricatta), subordinates of both sexes respond to experimentally induced increases in the growth of same-sex rivals by raising their own growth rate and food intake. In addition, when individuals acquire dominant status, they show a secondary period of accelerated growth whose magnitude increases if the difference between their own weight and that of the heaviest subordinate of the same sex in their group is small. Our results show that individuals adjust their growth to the size of their closest competitor and raise the possibility that similar plastic responses to the risk of competition may occur in other social mammals, including domestic animals and primates.〈br /〉〈span class="detail_caption"〉Notes: 〈/span〉Huchard, Elise -- English, Sinead -- Bell, Matt B V -- Thavarajah, Nathan -- Clutton-Brock, Tim -- England -- Nature. 2016 May 25;533(7604):532-4. doi: 10.1038/nature17986.〈br /〉〈span class="detail_caption"〉Author address: 〈/span〉Large Animal Research Group, Department of Zoology, University of Cambridge, Downing Street, Cambridge CB2 3EJ, UK. ; CEFE UMR 5175, CNRS - Universite de Montpellier, 1919 Route de Mende, 34293 Montpellier Cedex 5, France. ; Department of Zoology and Entomology, Mammal Research Institute, University of Pretoria, Pretoria, Gauteng 0002, South Africa.〈br /〉〈span class="detail_caption"〉Record origin:〈/span〉 〈a href="http://www.ncbi.nlm.nih.gov/pubmed/27225127" target="_blank"〉PubMed〈/a〉
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  • 4
    Publication Date: 2016-05-27
    Description: Circulating antibodies can access most tissues to mediate surveillance and elimination of invading pathogens. Immunoprivileged tissues such as the brain and the peripheral nervous system are shielded from plasma proteins by the blood-brain barrier and blood-nerve barrier, respectively. Yet, circulating antibodies must somehow gain access to these tissues to mediate their antimicrobial functions. Here we examine the mechanism by which antibodies gain access to neuronal tissues to control infection. Using a mouse model of genital herpes infection, we demonstrate that both antibodies and CD4 T cells are required to protect the host after immunization at a distal site. We show that memory CD4 T cells migrate to the dorsal root ganglia and spinal cord in response to infection with herpes simplex virus type 2. Once inside these neuronal tissues, CD4 T cells secrete interferon-gamma and mediate local increase in vascular permeability, enabling antibody access for viral control. A similar requirement for CD4 T cells for antibody access to the brain is observed after intranasal challenge with vesicular stomatitis virus. Our results reveal a previously unappreciated role of CD4 T cells in mobilizing antibodies to the peripheral sites of infection where they help to limit viral spread.〈br /〉〈span class="detail_caption"〉Notes: 〈/span〉Iijima, Norifumi -- Iwasaki, Akiko -- AI054359/AI/NIAID NIH HHS/ -- AI062428/AI/NIAID NIH HHS/ -- AI064705/AI/NIAID NIH HHS/ -- Howard Hughes Medical Institute/ -- England -- Nature. 2016 May 18;533(7604):552-6. doi: 10.1038/nature17979.〈br /〉〈span class="detail_caption"〉Author address: 〈/span〉Howard Hughes Medical Institute, Department of Immunobiology, Yale School of Medicine, New Haven, Connecticut 06520, USA.〈br /〉〈span class="detail_caption"〉Record origin:〈/span〉 〈a href="http://www.ncbi.nlm.nih.gov/pubmed/27225131" target="_blank"〉PubMed〈/a〉
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  • 5
    Publication Date: 2016-05-27
    Description: Topological insulators are insulating materials that display conducting surface states protected by time-reversal symmetry, wherein electron spins are locked to their momentum. This unique property opens up new opportunities for creating next-generation electronic, spintronic and quantum computation devices. Introducing ferromagnetic order into a topological insulator system without compromising its distinctive quantum coherent features could lead to the realization of several predicted physical phenomena. In particular, achieving robust long-range magnetic order at the surface of the topological insulator at specific locations without introducing spin-scattering centres could open up new possibilities for devices. Here we use spin-polarized neutron reflectivity experiments to demonstrate topologically enhanced interface magnetism by coupling a ferromagnetic insulator (EuS) to a topological insulator (Bi2Se3) in a bilayer system. This interfacial ferromagnetism persists up to room temperature, even though the ferromagnetic insulator is known to order ferromagnetically only at low temperatures (〈17 K). The magnetism induced at the interface resulting from the large spin-orbit interaction and the spin-momentum locking of the topological insulator surface greatly enhances the magnetic ordering (Curie) temperature of this bilayer system. The ferromagnetism extends ~2 nm into the Bi2Se3 from the interface. Owing to the short-range nature of the ferromagnetic exchange interaction, the time-reversal symmetry is broken only near the surface of a topological insulator, while leaving its bulk states unaffected. The topological magneto-electric response originating in such an engineered topological insulator could allow efficient manipulation of the magnetization dynamics by an electric field, providing an energy-efficient topological control mechanism for future spin-based technologies.〈br /〉〈span class="detail_caption"〉Notes: 〈/span〉Katmis, Ferhat -- Lauter, Valeria -- Nogueira, Flavio S -- Assaf, Badih A -- Jamer, Michelle E -- Wei, Peng -- Satpati, Biswarup -- Freeland, John W -- Eremin, Ilya -- Heiman, Don -- Jarillo-Herrero, Pablo -- Moodera, Jagadeesh S -- England -- Nature. 2016 May 9;533(7604):513-6. doi: 10.1038/nature17635.〈br /〉〈span class="detail_caption"〉Author address: 〈/span〉Department of Physics, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA. ; Francis Bitter Magnet Laboratory, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA. ; Plasma Science and Fusion Center, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA. ; Quantum Condensed Matter Division, Neutron Sciences Directorate, Oak Ridge National Laboratory, Oak Ridge, Tennessee 37831, USA. ; Institut fuer Theoretische Physik III, Ruhr-Universitaet Bochum, D-44801 Bochum, Germany. ; Institute for Theoretical Solid State Physics, Institut fuer Festkoerper- und Werkstoffforschung, Dresden, D-01069 Dresden, Germany. ; Department of Physics, Northeastern University, Boston, Massachusetts 02115, USA. ; Departement de Physique, Ecole Normale Superieure, Centre National de la Recherche Scientifique, Paris Sciences et Lettres Research University, Paris 75005, France. ; Saha Institute of Nuclear Physics, 1/AF Bidhannagar, Kolkata 64, India. ; Advanced Photon Source, Argonne National Laboratory, Argonne, Illinois 60439, USA.〈br /〉〈span class="detail_caption"〉Record origin:〈/span〉 〈a href="http://www.ncbi.nlm.nih.gov/pubmed/27225124" target="_blank"〉PubMed〈/a〉
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  • 6
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    Nature Publishing Group (NPG)
    Publication Date: 2016-05-27
    Description: 〈br /〉〈span class="detail_caption"〉Notes: 〈/span〉Yao, Yijun -- England -- Nature. 2016 May 25;533(7604):469. doi: 10.1038/533469a.〈br /〉〈span class="detail_caption"〉Record origin:〈/span〉 〈a href="http://www.ncbi.nlm.nih.gov/pubmed/27225107" target="_blank"〉PubMed〈/a〉
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  • 7
    Publication Date: 2016-05-27
    Description: 〈br /〉〈span class="detail_caption"〉Notes: 〈/span〉Tollefson, Jeff -- England -- Nature. 2016 May 25;533(7604):446-7. doi: 10.1038/533446a.〈br /〉〈span class="detail_caption"〉Record origin:〈/span〉 〈a href="http://www.ncbi.nlm.nih.gov/pubmed/27225094" target="_blank"〉PubMed〈/a〉
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  • 8
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    Nature Publishing Group (NPG)
    Publication Date: 2016-05-27
    Description: 〈br /〉〈span class="detail_caption"〉Notes: 〈/span〉Mehrabi, Zia -- England -- Nature. 2016 May 25;533(7604):469. doi: 10.1038/533469c.〈br /〉〈span class="detail_caption"〉Author address: 〈/span〉University of British Columbia, Canada.〈br /〉〈span class="detail_caption"〉Record origin:〈/span〉 〈a href="http://www.ncbi.nlm.nih.gov/pubmed/27225111" target="_blank"〉PubMed〈/a〉
    Keywords: Conservation of Natural Resources/*methods ; *Ecosystem ; *Wilderness
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  • 9
    Publication Date: 2016-05-27
    Description: Surveys have revealed many multi-planet systems containing super-Earths and Neptunes in orbits of a few days to a few months. There is debate whether in situ assembly or inward migration is the dominant mechanism of the formation of such planetary systems. Simulations suggest that migration creates tightly packed systems with planets whose orbital periods may be expressed as ratios of small integers (resonances), often in a many-planet series (chain). In the hundreds of multi-planet systems of sub-Neptunes, more planet pairs are observed near resonances than would generally be expected, but no individual system has hitherto been identified that must have been formed by migration. Proximity to resonance enables the detection of planets perturbing each other. Here we report transit timing variations of the four planets in the Kepler-223 system, model these variations as resonant-angle librations, and compute the long-term stability of the resonant chain. The architecture of Kepler-223 is too finely tuned to have been formed by scattering, and our numerical simulations demonstrate that its properties are natural outcomes of the migration hypothesis. Similar systems could be destabilized by any of several mechanisms, contributing to the observed orbital-period distribution, where many planets are not in resonances. Planetesimal interactions in particular are thought to be responsible for establishing the current orbits of the four giant planets in the Solar System by disrupting a theoretical initial resonant chain similar to that observed in Kepler-223.〈br /〉〈span class="detail_caption"〉Notes: 〈/span〉Mills, Sean M -- Fabrycky, Daniel C -- Migaszewski, Cezary -- Ford, Eric B -- Petigura, Erik -- Isaacson, Howard -- England -- Nature. 2016 May 11;533(7604):509-12. doi: 10.1038/nature17445.〈br /〉〈span class="detail_caption"〉Author address: 〈/span〉Department of Astronomy and Astrophysics, The University of Chicago, 5640 South Ellis Avenue, Chicago, Illinois 60637, USA. ; Institute of Physics and CASA*, University of Szczecin, Wielkopolska 15, 70-451 Szczecin, Poland. ; Torun Centre for Astronomy, Nicolaus Copernicus University, Gagarina 11, 87-100 Torun, Poland. ; Center for Exoplanets and Habitable Worlds, The Pennsylvania State University, University Park, Pennsylvania 16802, USA. ; Department of Astronomy and Astrophysics, The Pennsylvania State University, University Park, Pennsylvania 16802, USA. ; Center for Astrostatistics, The Pennsylvania State University, University Park, Pennsylvania 16802, USA. ; University of California at Berkeley, Berkeley, California 94720, USA. ; California Institute of Technology, Pasadena, California 91125, USA.〈br /〉〈span class="detail_caption"〉Record origin:〈/span〉 〈a href="http://www.ncbi.nlm.nih.gov/pubmed/27225123" target="_blank"〉PubMed〈/a〉
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  • 10
    Publication Date: 2016-05-27
    Description: About half of present-day cloud condensation nuclei originate from atmospheric nucleation, frequently appearing as a burst of new particles near midday. Atmospheric observations show that the growth rate of new particles often accelerates when the diameter of the particles is between one and ten nanometres. In this critical size range, new particles are most likely to be lost by coagulation with pre-existing particles, thereby failing to form new cloud condensation nuclei that are typically 50 to 100 nanometres across. Sulfuric acid vapour is often involved in nucleation but is too scarce to explain most subsequent growth, leaving organic vapours as the most plausible alternative, at least in the planetary boundary layer. Although recent studies predict that low-volatility organic vapours contribute during initial growth, direct evidence has been lacking. The accelerating growth may result from increased photolytic production of condensable organic species in the afternoon, and the presence of a possible Kelvin (curvature) effect, which inhibits organic vapour condensation on the smallest particles (the nano-Kohler theory), has so far remained ambiguous. Here we present experiments performed in a large chamber under atmospheric conditions that investigate the role of organic vapours in the initial growth of nucleated organic particles in the absence of inorganic acids and bases such as sulfuric acid or ammonia and amines, respectively. Using data from the same set of experiments, it has been shown that organic vapours alone can drive nucleation. We focus on the growth of nucleated particles and find that the organic vapours that drive initial growth have extremely low volatilities (saturation concentration less than 10(-4.5) micrograms per cubic metre). As the particles increase in size and the Kelvin barrier falls, subsequent growth is primarily due to more abundant organic vapours of slightly higher volatility (saturation concentrations of 10(-4.5) to 10(-0.5) micrograms per cubic metre). We present a particle growth model that quantitatively reproduces our measurements. Furthermore, we implement a parameterization of the first steps of growth in a global aerosol model and find that concentrations of atmospheric cloud concentration nuclei can change substantially in response, that is, by up to 50 per cent in comparison with previously assumed growth rate parameterizations.〈br /〉〈span class="detail_caption"〉Notes: 〈/span〉Trostl, Jasmin -- Chuang, Wayne K -- Gordon, Hamish -- Heinritzi, Martin -- Yan, Chao -- Molteni, Ugo -- Ahlm, Lars -- Frege, Carla -- Bianchi, Federico -- Wagner, Robert -- Simon, Mario -- Lehtipalo, Katrianne -- Williamson, Christina -- Craven, Jill S -- Duplissy, Jonathan -- Adamov, Alexey -- Almeida, Joao -- Bernhammer, Anne-Kathrin -- Breitenlechner, Martin -- Brilke, Sophia -- Dias, Antonio -- Ehrhart, Sebastian -- Flagan, Richard C -- Franchin, Alessandro -- Fuchs, Claudia -- Guida, Roberto -- Gysel, Martin -- Hansel, Armin -- Hoyle, Christopher R -- Jokinen, Tuija -- Junninen, Heikki -- Kangasluoma, Juha -- Keskinen, Helmi -- Kim, Jaeseok -- Krapf, Manuel -- Kurten, Andreas -- Laaksonen, Ari -- Lawler, Michael -- Leiminger, Markus -- Mathot, Serge -- Mohler, Ottmar -- Nieminen, Tuomo -- Onnela, Antti -- Petaja, Tuukka -- Piel, Felix M -- Miettinen, Pasi -- Rissanen, Matti P -- Rondo, Linda -- Sarnela, Nina -- Schobesberger, Siegfried -- Sengupta, Kamalika -- Sipila, Mikko -- Smith, James N -- Steiner, Gerhard -- Tome, Antonio -- Virtanen, Annele -- Wagner, Andrea C -- Weingartner, Ernest -- Wimmer, Daniela -- Winkler, Paul M -- Ye, Penglin -- Carslaw, Kenneth S -- Curtius, Joachim -- Dommen, Josef -- Kirkby, Jasper -- Kulmala, Markku -- Riipinen, Ilona -- Worsnop, Douglas R -- Donahue, Neil M -- Baltensperger, Urs -- England -- Nature. 2016 May 25;533(7604):527-31. doi: 10.1038/nature18271.〈br /〉〈span class="detail_caption"〉Author address: 〈/span〉Paul Scherrer Institute, Laboratory of Atmospheric Chemistry, CH-5232 Villigen, Switzerland. ; Carnegie Mellon University, Center for Atmospheric Particle Studies, Pittsburgh, Pennsylvania 15213, USA. ; CERN, CH-1211 Geneva, Switzerland. ; Goethe University Frankfurt, Institute for Atmospheric and Environmental Sciences, 60438 Frankfurt am Main, Germany. ; Department of Physics, University of Helsinki, PO Box 64, FI-00014 Helsinki, Finland. ; Department of Applied Environmental Science, University of Stockholm, SE-10961 Stockholm, Sweden. ; Institute for Atmospheric and Climate Science, ETH Zurich, 8092 Zurich, Switzerland. ; Chemical Sciences Division, Earth System Research Laboratory, NOAA, Boulder, Colorado, USA. ; Division of Chemistry and Chemical Engineering, California Institute of Technology, Pasadena, California 91125, USA. ; Helsinki Institute of Physics, University of Helsinki, PO Box 64, FI-00014 Helsinki, Finland. ; Institute for Ion and Applied Physics, University of Innsbruck, 6020 Innsbruck, Austria. ; Ionicon Analytik GmbH, 6020 Innsbruck, Austria. ; WSL Institute for Snow and Avalanche Research SLF, 7260 Davos, Switzerland. ; University of Eastern Finland, 70211 Kuopio, Finland. ; Finnish Meteorological Institute, 00101 Helsinki, Finland. ; National Center for Atmospheric Research, Atmospheric Chemistry Observations and Modeling Laboratory, Boulder, Colorado 80301, USA. ; Institute of Meteorology and Climate Research, Karlsruhe Institute of Technology, Karlsruhe, Germany. ; School of Earth and Environment, University of Leeds, LS2 9JT Leeds, UK. ; Department of Chemistry, University of California, Irvine, California 92697, USA. ; Faculty of Physics, University of Vienna, 1090 Vienna, Austria. ; SIM, University of Lisbon and University of Beira Interior, 1849-016 Lisbon, Portugal. ; Aerodyne Research, Inc., Billerica, Massachusetts 01821, USA.〈br /〉〈span class="detail_caption"〉Record origin:〈/span〉 〈a href="http://www.ncbi.nlm.nih.gov/pubmed/27225126" target="_blank"〉PubMed〈/a〉
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