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February 01, 2010
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Date:19TuesdayNovember 2013Lecture
The principle of detailed balance, opto-electronic reciprocity, and the thermodynamics of light trapping in solar cells
More information Time 14:00 - 14:00Location Perlman Chemical Sciences BuildingLecturer Prof. Uwe Rau
Forschungszentrum Julich,Julich, GermanyOrganizer Department of Molecular Chemistry and Materials ScienceContact -
Date:19TuesdayNovember 2013Lecture
The role of IFITM genes in the pathogenesis of the gastro-intestinal tract
More information Time 14:00 - 14:30Title Student SeminarLocation Wolfson Building for Biological ResearchLecturer Zoya Alteber Organizer Department of Systems ImmunologyContact -
Date:19TuesdayNovember 2013Lecture
Pulsed Laser Assisted Generation of Novel Materials and Related Applications
More information Time 15:30 - 15:30Lecturer Prof. 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 ScienceContact -
Date:20WednesdayNovember 2013Lecture
Neural stem cells and regeneration in zebrafish
More information Time 10:00 - 10:00Location Arthur and Rochelle Belfer Building for Biomedical ResearchLecturer Prof. Jan Kaslin
Australian Regenerative Medicine Institute, Monash University, Melbourne, AustraliaContact -
Date:20WednesdayNovember 2013Lecture
Vertex algebras and integrable systems (II)
More information Time 11:00 - 11:00Location Jacob Ziskind BuildingLecturer Daniel Fleisher
Organizer Faculty of Mathematics and Computer ScienceContact -
Date:20WednesdayNovember 2013Lecture
The dark side of molecular clouds
More information Time 11:15 - 12:00Location Nella and Leon Benoziyo Physics BuildingLecturer Raanan Nordon Organizer Nella and Leon Benoziyo Center for AstrophysicsContact Abstract Show 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.
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Date:20WednesdayNovember 2013Lecture
The unique value of immensely concentrated sunlight in photovoltaics, antenna harvesting, and the synthesis of singular nanomaterials
More information Time 13:00 - 13:00Location Gerhard M.J. Schmidt Lecture HallLecturer Prof. Jeffrey M. Gordon
Department of Solar Energy & Environmental Physics, Blaustein Institutes for Desert Research, Ben-Gurion University of the Negev, Sede Boqer CampusOrganizer Weizmann School of ScienceContact Abstract Show 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.
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Date:20WednesdayNovember 2013Cultural Events
Chapell concert
More information Time 20:30 - 20:30Location Dolfi and Lola Ebner AuditoriumContact -
Date:21ThursdayNovember 2013Conference
IAWR Conference
More information Time All dayLocation The David Lopatie Conference CentreChairperson Dan Yakir -
Date:21ThursdayNovember 2013Lecture
Life Sciences Colloquium
More information Time 11:00 - 11:00Title A model stem cell niche and its control of germline self-renewal and differentiationLocation Dolfi and Lola Ebner AuditoriumLecturer Prof. Judith Kimble Contact -
Date:21ThursdayNovember 2013Lecture
Invariant random subgroup rigidity in product groups
More information Time 11:00 - 11:00Location Jacob Ziskind BuildingLecturer Dr. Yair Hartman
Organizer Faculty of Mathematics and Computer ScienceContact -
Date:21ThursdayNovember 2013Colloquia
The thirteen billion year history of the most
More information Time 11:15 - 12:30Location Edna and K.B. Weissman Building of Physical SciencesLecturer HAGAI NETZER
School of Physics and Astronomy, TAUOrganizer Faculty of PhysicsContact Abstract Show 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.
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Date:21ThursdayNovember 2013Lecture
Robust Subspace Modeling
More information Time 12:00 - 12:00Location Jacob Ziskind BuildingLecturer Gilad Lerman
University of MinnesotaOrganizer Faculty of Mathematics and Computer ScienceContact -
Date:24SundayNovember 201325MondayNovember 2013Conference
ACCIS
More information Time All dayLocation Edna and K.B. Weissman Building of Physical SciencesChairperson Hadar AlperContact -
Date:24SundayNovember 2013Lecture
How hot can it be? Clumped isotopes perspective on Eocene high latitude temperatures.
More information Time 11:00 - 11:00Location Gerhard M.J. Schmidt Lecture HallLecturer Hagit P Affek
Geology and Geophysics Yale UniversityOrganizer Department of Earth and Planetary SciencesContact Abstract Show 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. -
Date:24SundayNovember 2013Lecture
A Population of Fast Radio Bursts at Cosmological Distances
More information Time 13:00 - 14:00Location Nella and Leon Benoziyo Physics BuildingLecturer Assaf Horesh Organizer Nella and Leon Benoziyo Center for AstrophysicsContact Abstract Show full text abstract about http://arxiv.org/abs/1307.1628 ...» http://arxiv.org/abs/1307.1628 -
Date:24SundayNovember 2013Lecture
Optimizing and Coordinating Networks and Markets of Selfish Players
More information Time 14:30 - 14:30Location Jacob Ziskind BuildingLecturer Retsef Levi
MITOrganizer Faculty of Mathematics and Computer ScienceContact -
Date:24SundayNovember 2013Lecture
The Annual Chaim Weizmann Lecture in the Humanities
More information Time 19:30 - 22:00Location Michael Sela AuditoriumLecturer The Annual Chaim Weizmann Lecture in the Humanities Organizer Yad Chaim WeizmannContact -
Date:25MondayNovember 2013Lecture
Insights on the role of cells and matrices and their combination in cell based therapies
More information Time 11:00 - 12:30Title Special Guest SeminarLocation Wolfson Building for Biological ResearchLecturer Prof. Raphael Gorodetsky
Hadassah - Hebrew University Medical CenterOrganizer Department of Systems ImmunologyContact -
Date:25MondayNovember 2013Lecture
Towards a complete dissection of genetic risk for neurological disease
More information Time 14:00 - 14:00Location Dolfi and Lola Ebner AuditoriumLecturer John Hardy
Professor UCL, LondonOrganizer Nella and Leon Benoziyo Center for Neurological DiseasesContact
