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February 01, 2010

  • Date:19TuesdayNovember 2013

    The principle of detailed balance, opto-electronic reciprocity, and the thermodynamics of light trapping in solar cells

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    Time
    14:00 - 14:00
    Location
    Perlman Chemical Sciences Building
    LecturerProf. Uwe Rau
    Forschungszentrum Julich,Julich, Germany
    Organizer
    Department of Molecular Chemistry and Materials Science
    Contact
    Lecture
  • Date:19TuesdayNovember 2013

    The role of IFITM genes in the pathogenesis of the gastro-intestinal tract

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    Time
    14:00 - 14:30
    Title
    Student Seminar
    Location
    Wolfson Building for Biological Research
    LecturerZoya Alteber
    Organizer
    Department of Systems Immunology
    Contact
    Lecture
  • Date:19TuesdayNovember 2013

    Pulsed Laser Assisted Generation of Novel Materials and Related Applications

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    Time
    15:30 - 15:30
    LecturerProf. Emmanuel Stratakis
    1. Institute of Electronic Structure and Laser, Foundation for Research & Technology Hellas, (IESL-FORTH), P.O. Box 1527, Heraklion 711 10, Greece. 2. University of Crete, Heraklion 714 09, Greece.
    Organizer
    Department of Molecular Chemistry and Materials Science
    Contact
    Lecture
  • Date:20WednesdayNovember 2013

    Neural stem cells and regeneration in zebrafish

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    Time
    10:00 - 10:00
    Location
    Arthur and Rochelle Belfer Building for Biomedical Research
    LecturerProf. Jan Kaslin
    Australian Regenerative Medicine Institute, Monash University, Melbourne, Australia
    Contact
    Lecture
  • Date:20WednesdayNovember 2013

    Vertex algebras and integrable systems (II)

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    Time
    11:00 - 11:00
    Location
    Jacob Ziskind Building
    LecturerDaniel Fleisher
    Organizer
    Faculty of Mathematics and Computer Science
    Contact
    Lecture
  • Date:20WednesdayNovember 2013

    The dark side of molecular clouds

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    Time
    11:15 - 12:00
    Location
    Nella and Leon Benoziyo Physics Building
    LecturerRaanan Nordon
    Organizer
    Nella and Leon Benoziyo Center for Astrophysics
    Contact
    AbstractShow full text abstract about In the last 4 years many measurements of the gas content in ...»
    In the last 4 years many measurements of the gas content in galaxies at increasing redshifts have been published. This wave has been driven by new and upgraded instruments in the far-infrared and sub-millimeter that are able to perform such measurements in "normal" z>0.5 galaxies. CO observations receive special attention these days as ALMA enters routine operation phase. But does CO emission trace all the molecular gas? I will discuss the structure of molecular clouds and the so called 'dark gas' that we may be missing.
    Lecture
  • Date:20WednesdayNovember 2013

    The unique value of immensely concentrated sunlight in photovoltaics, antenna harvesting, and the synthesis of singular nanomaterials

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    Time
    13:00 - 13:00
    Location
    Gerhard M.J. Schmidt Lecture Hall
    LecturerProf. Jeffrey M. Gordon
    Department of Solar Energy & Environmental Physics, Blaustein Institutes for Desert Research, Ben-Gurion University of the Negev, Sede Boqer Campus
    Organizer
    Weizmann School of Science
    Contact
    AbstractShow full text abstract about Basic thermodynamics informs us that concentrating solar rad...»
    Basic thermodynamics informs us that concentrating solar radiation creates the potential for both higher solar power conversion efficiency, and achieving the ultra-high threshold temperatures and flux densities that are crucial for some novel solar utilization strategies. Three examples constituting distinct solar conversion paradigms will be explored in this presentation.
    The first paradigm is ultra-efficient solar electricity generation stemming from the confluence of progress in multi-junction photovoltaic technologies and advanced solar concentrator design. The evolution from the initial optical and solid-state inventions to megawatt-scale commercial concentrator photovoltaic power plants will be reviewed. Several generations of new optics that approach the thermodynamic limit to concentration and optical tolerance, and have been tailored to the exigencies of the latest generations of concentrator solar cells, will be presented.
    The second paradigm is the tantalizing prospect of using solar rectifying antennas for solar power conversion. Although direct sunlight is commonly viewed as incoherent – therefore ostensibly not suitable for antenna collection – all radiation exhibits spatial coherence on a sufficiently small scale. The theory and experimental confirmation of basic performance bounds based on the partial coherence of broadband solar radiation will be reviewed. The ramifications for using optical concentrators that can effectively replace orders of magnitude of antenna and rectifier elements will be discussed. In addition, a basic upper bound on the ability to rectify (AC to DC) the inordinately high-frequency broadband signals from solar antennae will be evaluated.
    The third distinct solar paradigm is creating valued materials at the service of human technology, rather than using solar to generate heat, electricity or fuels (in collaboration with Reshef Tenne and his group at the WIS). It requires novel optical concentrators, and understanding the unique nature of solar reactor conditions (ultra-high temperatures with strong flux gradients and expansive ultra-hot annealing regions). Successful case studies subsume: cage-like nanostructures of Cs2O; high-yield syntheses for fullerene-like and nanotube MoS2, MoSe2, WS2, WSe2; nanowires and nanospheres of SiO2 generated for the first time from pure quartz; nanorods of pure Si; and SiC nanowires. Some of the MoS2 nanostructures achieve fundamentally minimum sizes predicted by molecular structural theory, as well as unique hybrid nanostructures.
    Lecture
  • Date:20WednesdayNovember 2013

    Chapell concert

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    Time
    20:30 - 20:30
    Location
    Dolfi and Lola Ebner Auditorium
    Contact
    Cultural Events
  • Date:21ThursdayNovember 2013

    IAWR Conference

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    Time
    All day
    Location
    The David Lopatie Conference Centre
    Chairperson
    Dan Yakir
    Conference
  • Date:21ThursdayNovember 2013

    Life Sciences Colloquium

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    Time
    11:00 - 11:00
    Title
    A model stem cell niche and its control of germline self-renewal and differentiation
    Location
    Dolfi and Lola Ebner Auditorium
    LecturerProf. Judith Kimble
    Contact
    Lecture
  • Date:21ThursdayNovember 2013

    Invariant random subgroup rigidity in product groups

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    Time
    11:00 - 11:00
    Location
    Jacob Ziskind Building
    LecturerDr. Yair Hartman
    Organizer
    Faculty of Mathematics and Computer Science
    Contact
    Lecture
  • Date:21ThursdayNovember 2013

    The thirteen billion year history of the most

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    Time
    11:15 - 12:30
    Location
    Edna and K.B. Weissman Building of Physical Sciences
    LecturerHAGAI NETZER
    School of Physics and Astronomy, TAU
    Organizer
    Faculty of Physics
    Contact
    AbstractShow full text abstract about Super-massive black holes that are found in the centers of m...»
    Super-massive black holes that are found in the centers of most galaxies started their
    growth when the universe was about 300 million years old. Some of these "seed black holes" were probably the remnants of the earliest stars. The largest black holes, that are some 10^10 times more massive than the sun, accumulated most of their mass during the first 3 billion years after the big bang. The less massive ones are still growing today.
    I will describe a large ground-based and space-borne project that follows BH evolution with special emphasis on the epoch when the universe was 1.2 Gyr old. This is probably the fastest growth episode of such objects and the fastest star formation in their host galaxies. The new observations provide important clues about the parallel evolution of massive BHs and their host galaxies throughout the history of the universe.
    Colloquia
  • Date:21ThursdayNovember 2013

    Robust Subspace Modeling

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    Time
    12:00 - 12:00
    Location
    Jacob Ziskind Building
    LecturerGilad Lerman
    University of Minnesota
    Organizer
    Faculty of Mathematics and Computer Science
    Contact
    Lecture
  • Date:24SundayNovember 201325MondayNovember 2013

    ACCIS

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    Time
    All day
    Location
    Edna and K.B. Weissman Building of Physical Sciences
    Chairperson
    Hadar Alper
    Contact
    Conference
  • Date:24SundayNovember 2013

    How hot can it be? Clumped isotopes perspective on Eocene high latitude temperatures.

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    Time
    11:00 - 11:00
    Location
    Gerhard M.J. Schmidt Lecture Hall
    LecturerHagit P Affek
    Geology and Geophysics Yale University
    Organizer
    Department of Earth and Planetary Sciences
    Contact
    AbstractShow full text abstract about The Eocene (56-34My ago) is one of the best analogs for a gr...»
    The Eocene (56-34My ago) is one of the best analogs for a greenhouse climate, with high CO2 concentrations, generally high temperatures, and no polar ice caps. A major feature of the Eocene geochemical records suggests a reduced latitudinal gradient, in which most of the warming occurs in polar regions (possibly exceeding 30°C in the Antarctic margin), but less in the tropics. These results could have profound implications for understanding polar amplification of greenhouse warming, but they are not captured in climate models, pointing to important gaps in climate models and to major uncertainties in the geochemical data. We combine two temperature proxies - carbonate clumped isotopes in fossil bivalve shells and archaeal lipid TEX86 in the sediment associated with the bivalves - to constrain Eocene temperatures in Southern high latitudes. Clumped isotope paleothermometry is a thermodynamically controlled temperature proxy that is not dependent on the isotopic composition of seawater, and presents a novel opportunity to reduce uncertainties in Eocene sea surface temperature estimates. We use it to constrain the calibration of TEX86 in order to compare paleotemperatures in the Antarctic Peninsula (Seymour Island) to those in the South Pacific (Eastern Tasman Plateau), both at ~65°S paleo-latitude. The data indicates middle to late Eocene paleotemperatures of 10-17C in Seymour Island and ~7°C higher in the Eastern Tasman Plateau, suggesting a pronounced zonal heterogeneity in southern high latitude sea surface temperatures.
    Lecture
  • Date:24SundayNovember 2013

    A Population of Fast Radio Bursts at Cosmological Distances

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    Time
    13:00 - 14:00
    Location
    Nella and Leon Benoziyo Physics Building
    LecturerAssaf Horesh
    Organizer
    Nella and Leon Benoziyo Center for Astrophysics
    Contact
    AbstractShow full text abstract about http://arxiv.org/abs/1307.1628 ...»
    http://arxiv.org/abs/1307.1628
    Lecture
  • Date:24SundayNovember 2013

    Optimizing and Coordinating Networks and Markets of Selfish Players

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    Time
    14:30 - 14:30
    Location
    Jacob Ziskind Building
    LecturerRetsef Levi
    MIT
    Organizer
    Faculty of Mathematics and Computer Science
    Contact
    Lecture
  • Date:24SundayNovember 2013

    The Annual Chaim Weizmann Lecture in the Humanities

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    Time
    19:30 - 22:00
    Location
    Michael Sela Auditorium
    LecturerThe Annual Chaim Weizmann Lecture in the Humanities
    Organizer
    Yad Chaim Weizmann
    Contact
    Lecture
  • Date:25MondayNovember 2013

    Insights on the role of cells and matrices and their combination in cell based therapies

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    Time
    11:00 - 12:30
    Title
    Special Guest Seminar
    Location
    Wolfson Building for Biological Research
    LecturerProf. Raphael Gorodetsky
    Hadassah - Hebrew University Medical Center
    Organizer
    Department of Systems Immunology
    Contact
    Lecture
  • Date:25MondayNovember 2013

    Towards a complete dissection of genetic risk for neurological disease

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    Time
    14:00 - 14:00
    Location
    Dolfi and Lola Ebner Auditorium
    LecturerJohn Hardy
    Professor UCL, London
    Organizer
    Nella and Leon Benoziyo Center for Neurological Diseases
    Contact
    Lecture

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