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January 01, 2013
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Date:19TuesdayMarch 2013Lecture
“Tales from the Cellular Underworld: mRNA Decay and Disease”
More information Time 14:00 - 15:00Location Gerhard M.J. Schmidt Lecture HallLecturer Prof. Lynne Maquat
University of Rochester Medical Center School of Medicine and Dentistry, USAOrganizer Department of Chemical and Structural BiologyContact -
Date:19TuesdayMarch 2013Cultural Events
Everyone Loves Carmen!
More information Time 17:30 - 17:30Title Nitza ShaulLocation Michael Sela AuditoriumContact -
Date:20WednesdayMarch 2013Lecture
THE PROGENITORS OF TYPE IA SUPERNOVA EXPLOSIONS ARE HEAD-ON COLLISIONS OF WHITE DWARFS IN TRIPLE SYSTEMS
More information Time 11:00 - 12:00Location Nella and Leon Benoziyo Physics BuildingLecturer Prof. Doron Kushnir Organizer Nella and Leon Benoziyo Center for AstrophysicsContact Abstract Show full text abstract about We argue that type Ia supernovae (SNe Ia) are the result of ...» We argue that type Ia supernovae (SNe Ia) are the result of head-on collisions of White Dwarfs (WDs) in
triple systems. The thermonuclear explosions resulting from the zero-impact-parameter collisions of WDs
are calculated from first principles by using 2D hydrodynamical simulations. Collisions of typical WDs with
masses 0.5-0.9 Msun result in explosions that synthesize 56Ni masses in the range of 0.15-0.8M Msun, spanning the wide distribution of yields observed for the majority of SNe Ia. The robustness of the shock ignition process is verified with a detailed study using a one-dimensional toy model and analytic tools. The late-time (& 50 days after peak) bolometric light curve is equal to the instantaneous energy deposition and is calculated exactly, by solving the transport of gmma-rays emitted by the decay of 56Ni using a Monte-Carlo code. All collisions are found to have the same late-time light curves, when normalized to the amount of synthesized 56Ni. This universal light curve is shown to agree with the majority of the supernovae in the compilation made by M. Stritzinger to an accuracy of better than 30% in the range 40 < t < 80 days after bolometric peak. The widths of the 56Ni mass- weighted-line-of-sight velocity distributions are correlated with the 56Ni yield and in agreement with the observed Mazzali relation. The continuous distribution of observed SN Ia features, is naturally reproduced with the distribution of WD masses involved in the collisions. -
Date:20WednesdayMarch 2013Lecture
Local Rankin-Selberg integrals for SO(2l) x GL(n)
More information Time 11:00 - 11:00Location Jacob Ziskind BuildingLecturer Eyal Kaplan
Organizer Faculty of Mathematics and Computer ScienceContact -
Date:20WednesdayMarch 2013Lecture
Half planar maps
More information Time 11:00 - 11:00Location The David Lopatie Hall of Graduate StudiesLecturer Omer Angel
University of British ColumbiaOrganizer Faculty of Mathematics and Computer ScienceContact -
Date:20WednesdayMarch 2013Lecture
A very smooth ride in rough sea
More information Time 16:00 - 16:00Location The David Lopatie Hall of Graduate StudiesLecturer Uriel Frisch
Observatoire de la Cote d'AzurOrganizer Faculty of Mathematics and Computer ScienceContact -
Date:20WednesdayMarch 2013Cultural Events
A Comedy of Errors
More information Time 20:30 - 20:30Title the Camari Theater, Subscription choiceLocation Michael Sela AuditoriumContact -
Date:21ThursdayMarch 2013Lecture
Magnetic Resonance Seminar
More information Time 09:30 - 09:30Title Quantitative MRI for studying brain development in preterm babiesLocation Gerhard M.J. Schmidt Lecture HallLecturer Dr. Revital Nossin-Manor
Hadassah-Hebrew University Medical CenterOrganizer Department of Chemical and Biological PhysicsContact -
Date:21ThursdayMarch 2013Lecture
Chaperones as polypeptide unfolding enzymes combating toxic misfolded conformers in protein conformational diseases
More information Time 11:00 - 11:00Location Arthur and Rochelle Belfer Building for Biomedical ResearchLecturer Prof. Pierre Goloubinoff Organizer Department of Molecular GeneticsContact -
Date:21ThursdayMarch 2013Colloquia
Atmospheric dynamics on giant planets
More information Time 11:15 - 12:30Location Edna and K.B. Weissman Building of Physical SciencesLecturer Prof. Yohai Kaspi
WIS – Faculty of ChemistryOrganizer Faculty of PhysicsContact Abstract Show full text abstract about The atmospheric circulation on Jupiter, Saturn, Uranus and N...» The atmospheric circulation on Jupiter, Saturn, Uranus and Neptune is dominated by strong east-west jet-streams. In this talk we will discuss the physical mechanisms controlling these jets, focusing on the depth to which they extend into the planets' fluid interiors. New information about the vertical structure of these winds is expected in 2016 when NASA's Juno and Cassini spacecraft will perform close flybys of Jupiter and Saturn, obtaining for the first time a high order gravity spectrum of these planets. We will show how the relations between the fluid velocity and the measured gravity perturbations due to dynamics can be used to constrain the depth of the circulation on these planets. We find that for the case of Uranus and Neptune, even the already known values of the fourth zonal gravity harmonic, J4, can constrain the observed zonal jets to a thin weather-layer containing no more than the uppermost 0.2% of the planetary mass. -
Date:21ThursdayMarch 2013Lecture
Efficient incremental structure from motion and vision-based single- and multi-agent localization
More information Time 12:00 - 12:00Location Jacob Ziskind BuildingLecturer Vadim Indelman
Georgia TechOrganizer Faculty of Mathematics and Computer ScienceContact -
Date:21ThursdayMarch 2013Cultural Events
The Israel Brass Quintet
More information Time 12:30 - 12:30Title Music at NoonLocation Michael Sela AuditoriumContact -
Date:21ThursdayMarch 2013Lecture
Life Science Lecture Series
More information Time 15:00 - 16:30Title From Bench-top Photosynthesis to Bed-side Cancer TherapyLocation Dolfi and Lola Ebner AuditoriumLecturer Prof. Avigdor Scherz
Department of Plant SciencesContact -
Date:24SundayMarch 2013Lecture
Metabolic Syndrome Research Club
More information Time 15:00 - 15:00Title Neighborly relationship: cooperative regulation of metabolic homeostasis by the host and its microbiomeLocation Camelia Botnar BuildingLecturer Prof. Eran Elinav
Dept. of Immunology, Weizmann InstituteContact -
Date:02TuesdayApril 2013Lecture
Biomedical Magnetic Resonance in Israel: A pre-ISMRM Symposium
More information Time 09:00 - 17:00Location Gerhard M.J. Schmidt Lecture HallOrganizer Department of Chemical and Biological PhysicsContact -
Date:02TuesdayApril 2013Lecture
"The landscape of Adenosine-to-inosine RNA editing in human"
More information Time 10:00 - 10:00Location Wolfson Building for Biological ResearchLecturer Dr. Erez Levanon
Faculty of Life Sciences, Bar-Ilan UniversityOrganizer Department of Biomolecular SciencesContact -
Date:02TuesdayApril 2013Lecture
Mathematical models for cell polarization and motility
More information Time 11:00 - 11:00Location Jacob Ziskind BuildingLecturer Leah Edelstein-Keshet
University of British ColumbiaOrganizer Faculty of Mathematics and Computer ScienceContact -
Date:02TuesdayApril 2013Lecture
p53 and friends under glucose starvation
More information Time 12:00 - 12:00Location Wolfson Building for Biological ResearchLecturer Chagay Gonen Organizer Department of Molecular Cell BiologyContact -
Date:02TuesdayApril 2013Lecture
Empathic helping in rats and its modulation by social parameters
More information Time 12:30 - 12:30Location Arthur and Rochelle Belfer Building for Biomedical ResearchLecturer Dr. Inbal Ben-Ami Bartal
Dept of Neurobiology, University of ChicagoOrganizer Department of Brain SciencesContact Abstract Show full text abstract about Empathy, the recognition and sharing of affective states bet...» Empathy, the recognition and sharing of affective states between individuals, is an adaptive response with ancient evolutionary roots. The experience of empathy rises from activation of subcortical neural circuits in the brain stem, thalamus and paralimbic areas that are highly conserved across mammalian species. Primarily, it is crucial for the survival of altricial mammals to be able to respond to the needs of offspring appropriately. More broadly, communication of emotions promotes group survival, by alerting against potential threats and, depending on context, inducing pro-social actions. Behavioral homologues of empathy have been observed in different non-human animals. For instance, it has been clearly established that rodents display emotional contagion of others’ distress, and are motivated to alleviate another rat’s distress. We found that rats intentionally released a cagemate trapped in a restrainer, even when social contact was prevented. When a second restrainer containing a highly palatable food (chocolate chips) was present, rats opened both restrainers and typically shared the chocolate. Since only cagemates were tested, it is unclear if these behaviors generalize to strangers. Helping others is costly and resource depleting, and should thus be discriminately extended. In humans, the expression of empathically motivated pro-social behavior is dependent on social context, where people are more motivated to help in-group members than out-group members. Correspondingly, emotional contagion is modulated by familiarity in rodents. Mice have been found to display heightened pain sensitivity when witnessing a cagemate in pain, but not a stranger in pain. To investigate these questions, we are currently exploring the effect of social parameters such as familiarity and relatedness on the expression of empathic helping in rats. -
Date:02TuesdayApril 2013Lecture
"The heartbeat of transcription - dynamics of the transcription machinery studied by single-molecule FRET"
More information Time 14:00 - 15:00Location Helen and Milton A. Kimmelman BuildingLecturer Dr. Dina Grohmann
Physikalische und Theoretische Chemie -NanoBioSciences, TU Braunschweig, GermanyOrganizer Department of Chemical and Structural BiologyContact
