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VERSION:2.0
PRODID:icalendar-ruby
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METHOD:PUBLISH
BEGIN:VEVENT
DTSTAMP:20260818T233919Z
UID:https://www.mpsd.mpg.de/events/5146/17178
DTSTART:20160415T120000Z
DTEND:20160415T130000Z
CLASS:PUBLIC
CREATED:20160329T110245Z
DESCRIPTION:Our Universe displays a vast panoply of exotic objects like the
  Earth\, black holes\, or neutron stars. With a mass of twice the Sun mass
  and a radius of ~10 km\, a neutron star is a very dense object. At a temp
 erature of 10^8 K\, the spin 1/2 neutrons are believed to be in a superflu
 id state. We will show how dilute gases prepared by laser techniques at th
 e other extreme of the temperature scale\, in the Nano kelvin range\, can 
 help us to understand the superfluid state of neutron stars.\nSpeaker: Chr
 istophe Salomon
LAST-MODIFIED:20160415T111704Z
LOCATION:CFEL (Bldg. 99)\, Room: Seminar Room I-III\, EG.076-080
ORGANIZER;CN="CFEL, CUI, DESY, European XFEL, HZG, MPSD, SFB 925, UHH":mail
 to:
SUMMARY:Hamburg Photon Science Colloquium: Simulating Neutron Stars in the 
 Laboratory
URL;VALUE=URI:https://www.mpsd.mpg.de/events/5146/17178
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