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December 01, 2013
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Date:03TuesdayJanuary 2017Lecture
Joint Chemical Physics and Materials and Interfaces Seminar
More information Time 10:00 - 10:00Title Carbon Monoxide Adsorption and Oxidation on Copper Surfaces: From Atoms to ComplexityLocation Perlman Chemical Sciences BuildingLecturer Dr. Baran Eren
Materials Sciences Division, LBNLOrganizer Department of Chemical and Biological PhysicsContact Abstract Show full text abstract about An extensive array of surface-sensitive characterization tec...» An extensive array of surface-sensitive characterization techniques that provide microscopic and spectroscopic information have revealed the structure of many crystal surfaces in their pristine clean state. Most of these studies are carried out in ultrahigh vacuum (UHV), which makes it possible to control sample composition and cleanliness to better than 0.1% of a monolayer. Starting from those by Irving Langmuir, such surface science studies constituted the core of our present understanding of solid surfaces. Under realistic ambient conditions, however, our knowledge is far less extensive. Of particular interest is the structure and chemical state of surfaces in dynamic equilibrium with gases and liquids at ambient conditions. Ambient pressure x-ray photoelectron spectroscopy (APXPS) and high pressure scanning tunneling microscopy (HPSTM) were developed for this purpose, i.e., understanding the atomic, electronic, and chemical structure of surfaces in the presence of reactant gases and liquids.
My talk will have three parts. The first part will be about ‘following surface structures’. I will show that the most compact and stable surfaces of Cu undergo massive reconstructions in the presence of CO at room temperature at pressures in the Torr range, and they decompose into two-dimensional nanoclusters, which is a double effect of low cohesive energy of Cu and the high gain in adsorption energy at the newly formed under-coordinated sites. Finally, it will be shown that the surfaces which are broken up into clusters are more active for water dissociation, a key step in the water gas shift reaction. Such a behavior opens a new paradigm, especially for other soft metals like gold, silver, zinc, etc., and it is clear that we need more of such studies. I will also briefly comment on the predictive power of my results and whether we can extrapolate it to other metals and reactants other than CO.
The second part will centered on ‘following surface reactions’ with APXPS. This technique is so powerful that it allows us to monitor the changes in the chemical state of the adsorbent, as well as coverage of adsorbates. As an example, I chose the CO oxidation reaction on Cu surfaces. It will be shown that if Cu remains metallic, the activation energy of the reactions scales with the oxygen binding energy, which is the manifestation of the Sabatier effect. In the presence of both CO and O2, however, the surface gets covered with 1-3 nm of Cu2O layer, which is more active than metallic Cu, but no CuO forms under the pressure and temperature range chosen in my study.
The final part will be about the possible future directions which I find important in the field for the next 5-10 years. Especially I will mention new approaches I plan to take for technique development which can offer measurements at higher pressures, as well as extend the outreach of the available techniques to other fields where solid-gas and solid-liquid interactions play an essential role.
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Date:03TuesdayJanuary 2017Lecture
Caught in between: Transmembrane Derived Peptides for Targeting TLR Signaling in Diseases
More information Time 10:30 - 11:00Location Wolfson Building for Biological ResearchLecturer Liraz Shmuel Galia
Member - Dept. of Biomolecular Sciences-WISOrganizer Department of Biomolecular SciencesContact -
Date:03TuesdayJanuary 2017Lecture
Developing Chemical Tools to Specifically Target Protein-Protein Interactions
More information Time 11:00 - 12:00Location Helen and Milton A. Kimmelman BuildingLecturer Dr. Nir Qvit
Department of Chemical and Systems Biology Stanford UniversityOrganizer Department of Molecular Chemistry and Materials ScienceContact -
Date:03TuesdayJanuary 2017Lecture
Active Remote Sensing of the atmosphere
More information Time 11:00 - 11:00Location Sussman Family Building for Environmental SciencesLecturer Prof. Albert Ansmann
Leibniz Institute for Tropospheric Research (TROPOS), GermanyOrganizer Department of Earth and Planetary SciencesContact -
Date:03TuesdayJanuary 2017Lecture
Bacterial decision making on plant leaf surfaces
More information Time 11:15 - 11:15Location Ullmann Building of Life SciencesLecturer Dr. Nadav Kashtan
Department of Plant Pathology and Microbiology, Robert H. Smith Faculty of Agriculture, Food and Environment, The Hebrew University of Jerusalem, RehovotOrganizer Department of Plant and Environmental SciencesContact -
Date:03TuesdayJanuary 2017Lecture
MCB - Students seminar
More information Time 12:15 - 12:15Title TBALocation Wolfson Building for Biological ResearchOrganizer Department of Molecular Cell BiologyContact -
Date:03TuesdayJanuary 2017Lecture
Coding with Correlated Neurons
More information Time 12:30 - 12:30Location Gerhard M.J. Schmidt Lecture HallLecturer Dr. Rava da Silveira
École Normale Supérieure, Paris, FranceOrganizer Department of Brain SciencesContact Abstract Show full text abstract about Arguably, quantitative neuroscience was born when scientists...» Arguably, quantitative neuroscience was born when scientists started to correlate the activity of a neuron with sensory stimuli. But complex stimuli, such as natural ones, are encoded in the activity of
entire populations of neurons. What is the grammar of this code? Specifically, how are the correlations among neurons and their physiological diversity involved in this code? In this talk, I will discuss analyses of the output of populations of identified and simultaneously recorded visual neurons. In these populations, and against the textbook picture of neural population coding, correlations in the spiking variability enhance the coding performance. This unexpected phenomenon relies upon a particular structure of the correlations observed in data and, surprisingly, yields a strong effect even in very small populations of neurons. I will, further, explain how the favorable structure of correlations can emerge from simple circuit features. Finally, if time allows, I will present more general theoretical extensions in which, with the use of simple models, one can illustrate the massive influence that correlations and physiological diversity can have on the precision and capacity of the neural code.
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Date:03TuesdayJanuary 2017Lecture
“Computer Controlled Molecular Motor Made of DNA”
More information Time 14:00 - 14:00Location Helen and Milton A. Kimmelman BuildingLecturer Dr. Eyal Nir
Department of Chemistry BGUOrganizer Department of Chemical and Structural BiologyContact -
Date:03TuesdayJanuary 2017Cultural Events
Morroccan theater - Tlata del schab
More information Time 20:30 - 22:00Location Michael Sela AuditoriumContact -
Date:04WednesdayJanuary 2017Lecture
Dry Intrusions and Warm Conveyor Belts: Feature-based Climatologies for Understanding Extratropical Weather Dynamics
More information Time 10:00 - 10:00Location Sussman Family Building for Environmental SciencesLecturer Dr. Shira Raveh
Department of Environmental Systems Science ETH ZurichOrganizer Department of Earth and Planetary SciencesContact -
Date:04WednesdayJanuary 2017Lecture
Tunable colors in zebrafish iridophores
More information Time 10:00 - 10:00Location Arthur and Rochelle Belfer Building for Biomedical ResearchLecturer Dr. Dvir Gur
Labs of Gil Levkowitz & Dan Oron, Depts. of Molecular Cell Biology & Physics of Complex Systems, WISContact -
Date:04WednesdayJanuary 2017Lecture
Special Guest Seminar
More information Time 11:00 - 12:00Title “Fueling immunity: mitochondrial rewiring drives anabolic metabolism for T cell activation”Location Wolfson Building for Biological ResearchLecturer Noga Ron-Harel
Department of Cell Biology, Harvard Medical SchoolOrganizer Department of Systems ImmunologyContact -
Date:04WednesdayJanuary 2017Lecture
"Cosmology in Mirror Twin Higgs and Neutrino Masses"
More information Time 11:00 - 11:00Location TechnionLecturer Roni Harnik
FermilabOrganizer Department of Particle Physics and AstrophysicsContact -
Date:04WednesdayJanuary 2017Lecture
"A Collective Quartic for the Composite Higgs from 6d"
More information Time 13:00 - 13:00Location TechnionLecturer Michael Geller
MarylandOrganizer Department of Particle Physics and AstrophysicsContact Abstract Show full text abstract about a Pseudo-Nambu-Goldstone boson (PNGB) and the resulting Higg...» a Pseudo-Nambu-Goldstone boson (PNGB) and the resulting Higgs properties deviate from those predicted by the SM. The current Higgs and EW data favor a SM-like Higgs, requiring a hierarchy between the PNGB Higgs decay constant f and its vacuum expectation value v. The v/f hierarchy is responsible for a significant part of the fine-tuning in these models. We show that adding an independent, adjustable quartic to the Higgs potential can eliminate the v/f tuning, such that the only remaining tuning arises from radiative corrections to the Higgs mass. We demonstrate how this quartic can be obtained from extra-dimensions, revisiting the 6d origin of the little-Higgs models, this time in a warped AdS5xS1 background. We construct a 6D Composite Higgs model and also consider its deconstruction into a two-site Randall-Sundrum model. The PNGB Higgs in this model corresponds to the extra-dimensional components of a gauge field, and the quartic arises from the non-abelian gauge action in 6d. We show that this quartic is collective just like in little Higgs models, and so it is stable against quantum corrections. Our quartic scales like (R6/R), where R6 is the size of the flat circle, and R is the curvature radius of AdS. We show that a general hierarchy of (R6/R) can be naturally stabilized, and any desired quartic can be obtained. -
Date:04WednesdayJanuary 2017Lecture
Chemical Physics Department Special Guest Seminar
More information Time 14:00 - 14:00Title Rice-quakes in crunchy soft matterLocation Perlman Chemical Sciences BuildingLecturer Prof Itai Einav
University of SydneyOrganizer Department of Chemical and Biological PhysicsContact Abstract Show full text abstract about Most of us have tried this at home: smash cereal with a spoo...» Most of us have tried this at home: smash cereal with a spoon. Yet, the science of snap, crackle and pop extends way beyond a cereal ad. Indeed, using such a simple experiment we reveal surprisingly rich compaction patterns due to competing processes of internal collapse and recovery. Using a simple spring-lattice model that captures these two processes, we successfully explain previously observed patterns in cereal, snow and sandstones. Subsequently, we use the model to guide us in the discovery of novel patterns, which we confirm experimentally in cereal. A further set of experiments with cereal partially soaked by fluid (milk/water) under constant pressure reveals coherent rice-quakes that could be explained by coupled fluid diffusion and the chemical degradation of the solid matrix; similar conditions often prevail in rockfill dams, which frequently fail unexpectedly. Our work reveals bifurcation in solids reminiscent of critical phenomena near phase transitions, and thus will be of relevance for people interested in soft matter physics, complex systems, and non-equilibrium thermodynamics.
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Date:05ThursdayJanuary 2017Colloquia
Gamma-ray astronomy - observing the extreme places in the Universe
More information Time 11:15 - 12:30Location Edna and K.B. Weissman Building of Physical SciencesLecturer Christian Stegmann
DESYOrganizer Faculty of PhysicsContact Abstract Show full text abstract about Astronomy with gamma rays at energies above some 10 GeV has ...» Astronomy with gamma rays at energies above some 10 GeV has opened in the last decade a new window to the cosmos. Gamma rays allows us to take a look at the extreme places in our Universe. They are produced in Supernova remains, Black holes and active galaxies - cosmic particle accelerators, in which atomic nuclei and electrons are accelerated to vast energies.
Contrary to expectations high-energy phenomena are no exception in the cosmos, but occur in many galactic and extragalactic objects during their life cycle. There are currently over 2000 sources of GeV radiation and over 150 sources of TeV radiation. Thus the results of gamma astronomy are an important building block to the understanding of the development of the Milky Way and our Universe.
So far, gamma-ray astronomy in the TeV range, however, is performed with experiments that are only accessible to a limited circle of users.
With the Cherenkov Telescope Array CTA an international consortium of more than 1000 scientists and engineers aims for an open observatory.
Starting from the current findings of gamma-ray astronomy I will in the presentation date to look into the future to what we will be able to learn with CTA.
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Date:05ThursdayJanuary 2017Lecture
Immunology Departmental Student Seminar
More information Time 14:00 - 15:00Location Wolfson Building for Biological ResearchLecturer Adi Sharbi Yunger & Masha Kolesnikov Organizer Department of Systems ImmunologyContact -
Date:05ThursdayJanuary 2017Lecture
Shirat Hamada
More information Time 19:30 - 21:30Location Michael Sela AuditoriumContact -
Date:08SundayJanuary 2017Lecture
New CRISPR-Cas systems from uncultivated microbes
More information Time 09:00 - 09:00Location Arthur and Rochelle Belfer Building for Biomedical ResearchLecturer Dr. David Burstein
Department of Earth and Planetary Sciences, University of California, BerkeleyOrganizer Department of Molecular GeneticsContact -
Date:08SundayJanuary 2017Lecture
The Snowball Bifurcation on Exoplanets
More information Time 11:00 - 11:00Location Sussman Family Building for Environmental SciencesLecturer Dr. Dorian Abbot
Department of the Geophysical Sciences The University of ChicagoOrganizer Department of Earth and Planetary SciencesContact Abstract Show full text abstract about The Snowball Earth episodes may have affected the developmen...» The Snowball Earth episodes may have affected the development of life on Earth through increasing atmospheric oxygen and spurring evolution. Considering the habitability and increase in complexity of life on other planets therefore requires thought about Snowball climate states. Using an energy balance model and global climate model, I will show that it is unlikely a tidally locked planet could experience a Snowball Earth bifurcation. Instead the planet would smoothly transition to global ice coverage. This is due to the difference in the shape of the insolation, which increases strongly toward the substellar point on a tidally locked planet. I will then change focus slightly and explain how climate oscillations between a warm state and a Snowball state can occur on a planet within the habitable zone that has a small CO2 outgassing rate. I will develop analytical relations to understand these cycles and outline scalings in variables such as the cycle period as a function of important climatic and weathering parameters. Work of this type should help us understand the context of planetary habitability and focus on appropriate targets as we seek to find the first inhabited exoplanet.
