Academic

Name	Primary Category	Discipline/Position	Phone	Office	E-Mail	Home Page
Sfaradi Itai	Graduate Students	Astrophysics and Relativity
Shacham Tomer	Visiting Scientists	Astrophysics and Relativity	02 6584 173	Kaplun 214
Shaltiel David	Emeriti	Condensed Matter Physics	02 6584 497	Danciger B 119
Sharon Eran	Faculty	Nonlinear	02 6585 674	Levin 16b
Shaviv Nir	Faculty	Astrophysics and Relativity	02 6585 807	Kaplun 102
Sherman Eilon	Faculty	Biophysics and Interdisciplinary Research	02 6586 878	Danciger B 102
Shir Ruth	Post-Docs	High Energy Physics	02 6584 173	Kaplun 214
Shubho Roy	Post-Docs	High Energy Physics	02 6584 354	Kaplun 202
Shvartsman Leonid	Senior Scientists	Condensed Matter Physics	02 6586 356	Danciger B 100
Silverwater Tal	Graduate Students	Astrophysics and Relativity

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Upcoming Events

Yesterday

Physics Colloquium : "Are `analog computers' back in fashion?"
- Start time: 12:00pm
- End date: Monday, December 2nd
- End time: 01:30pm
- Lecturer: Prof. Oren Raz, Weizmann InstituteAbstract:In the last decade there have been several efforts to use physical systems as 'physical computers': D-Wave is using super-conducting qubits as an adiabatic computer, the Israeli company Light-Solver uses lasers to find optimal solutions to optimization algorithm, HP is developing `memristor computation', and companies like Toshiba and Fujitsu are commercializing products like `Bifurcation machines' and `Digital annealers'... In the talk I will review this topic, show some results, what we do and don't understand, and try to provide some intuition on what physical mechanisms are expected to give real benefits.
- View this event in Google Calendar

Today

Astrolunch: Cecilia Chirenti
- Start time: 04:00pm
- End date: Tuesday, December 3rd
- End time: 05:00pm
- Speaker: Prof. Cecilia Chirenti (Federal University of ABC, Santo Andre, Brazil; Department of Astronomy, University of Maryland, USA)Title: Quasi-periodic oscillations in short gamma-ray bursts and implications for neutron starsAbstract:Short gamma ray bursts (GRBs) have already been associated with binary neutron star mergers, which are also sources of gravitational waves. Numerical relativity simulations indicate that the merger can form a short-lived hypermassive neutron star (which could produce a millisecond magnetar), lasting for tens to hundreds of milliseconds before gravitational collapse forms a black hole. This neutron star remnant is expected to emit gravitational waves (GWs) with kHz frequencies that will be detectable by third generation ground-based GW detectors in the 2030s. Recently, kHz quasiperiodic oscillations were discovered in GRBs 910711 and 931101B, providing evidence for a hypermassive neutron star stage in these events. When analyzed together with new quasi-universal relations obtained from numerical relativity simulations, these detections provide a novel method to constrain the equation of state of the dense matter in neutron star cores.Zoom link:https://huji.zoom.us/j/83438422733?pwd=bO4fe7y4WgZ5OWdFjaUxulnbjurow1.1Meeting ID: 834 3842 2733Passcode: 294941 Contact: Dima Ofengeim
- View this event in Google Calendar