Academic Faculty

Name	Discipline/Position	Phone	Office	E-Mail	Home Page
Moshe Michael	Nonlinear	02 5494 819	Kaplun 102
Orgad Dror	Condensed Matter Physics	02 6586 980	Danciger B 214
Perel Reuven	Biophysics and Interdisciplinary Research	02 6586 881	Popick 106
Piran Tsvi	Astrophysics and Relativity	02 6584 233	Kaplun 108
Rapaport Ronen	Atomic, Molecular and Optical Physics	02 6586 270	Danciger B 122
Retzker Alex	Atomic, Molecular and Optical Physics	02 6586 329	Danciger B 203
Ringel Zohar	Condensed Matter Physics	02 6585 919	Danciger B 222
Ron Guy	Nuclear Hadronic and Few-Body Physics	02 6585 200	Kaplun 18
Saar Amir	Condensed Matter Physics	02 6585 701	Bergman 123
Sari Reem	Astrophysics and Relativity	02 6585 806	Kaplun 111

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Upcoming Events

Tomorrow

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.
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Tuesday, December 3rd

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
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