Post-Docs

Name	Discipline/Position	Phone	Office	E-Mail	Home Page
Cornuault Nicolas	Astrophysics and Relativity
Benyamin David	Astrophysics and Relativity		Kaplun 100
Thaler Irina	Astrophysics and Relativity
Tang Xiaping	Astrophysics and Relativity
Fragione Giacomo	Astrophysics and Relativity
Sarkar Kartick Chandra	Astrophysics and Relativity		Ross Bldg. 216
Globus Noemie	Astrophysics and Relativity	02 6584 997	Kaplun 103
Ziskin Shlomi	Astrophysics and Relativity
Reetanjali Moharana	Astrophysics and Relativity	02 6585 492	Kaplun 103
Freundlich Jonathan	Astrophysics and Relativity	02 6584 675	Kaplun 201

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Upcoming Events

Tomorrow

Physics Colloquium : "Quantum gas in a box"
- Start time: 04:00pm
- End date: Monday, May 23rd
- End time: 05:30pm
- Lecturer: Prof. Zoran Hadzibabic, Cambridge UniversityAbstract:For nearly three decades, ultracold atomic gases have been used with great success tostudy fundamental many-body phenomena such as Bose-Einstein condensation andsuperfluidity. While traditionally they were produced in harmonic electromagnetictraps and thus had inhomogeneous densities, it is now also possible to createhomogeneous samples in the uniform potential of an optical box trap. Boxtrapping simplifies the interpretation of experimental results, provides more directconnections with theory and, in some cases, allows qualitatively new, hithertoimpossible experiments. I will give an overview of our recent experiments with box-trapped three- and two-dimensional Bose gases, focusing on a series of relatedexperiments on non-equilibrium phenomena, including phase-transition dynamics,turbulence, and equilibration of closed quantum systems.
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Tuesday, May 24th

Astrolunch: Andrea Possenti
- Start time: 12:30pm
- End date: Tuesday, May 24th
- End time: 01:30pm
- Title: Exploiting globular cluster pulsars in astrophysicsAbstract: Pulsars and millisecond pulsars are highly magnetised and rapidly spinning neutron stars. Thanks to the clock-like nature of their pulsed radio emission, some of them can be used as unique probes for performing a variety of high value experiments. The scientific reward is especially high for the pulsars included in a globular cluster. On one hand in these stellar systems one can find exotic pulsar binaries, impossible to form in the galactic field. That leads to explore previously uncharted physical effects or to see in act physical and/or astrophysical processes that are very hard to be checked elsewhere. On the other hand, when multiple pulsars are detected in a specific cluster, that opens the possibility to constrain properties of that cluster which are otherwise very elusive to other kinds of observation.
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Wednesday, May 25th

Nonlinear Physics Seminar: ""
- Start time: 12:00pm
- End date: Wednesday, May 25th
- End time: 01:30pm
- Lecturer: Ido Tishby, HUJIAbstract:
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