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VERSION:2.0
CALSCALE:GREGORIAN
PRODID:UW-Madison-Physics-Events
BEGIN:VEVENT
SEQUENCE:1
UID:UW-Physics-Event-4990
DTSTART:20181219T160000Z
DTEND:20181219T170000Z
DTSTAMP:20260419T101439Z
LAST-MODIFIED:20181215T203609Z
LOCATION:5310 Chamberlin
SUMMARY:Update on the GNOME Experiment\, Atomic Physics Seminar\, Ibra
 him Sulai (for the GNOME collaboration)\, Bucknell University
DESCRIPTION:The Global Network of Optical Magnetometers for Exotic phy
 sics (GNOME) comprises an array of atomic<br>
\nmagnetometers used for
  searching for beyond the standard model spin interactions. It present
 ly<br>
\nconsists of 12 active magnetometer stations spread around the
  globe with gps-time stamped data being<br>
\ncontinuously streamed to
  a central server for analysis. Of special interest is the search for 
 dark matter in<br>
\nthe form of interactions with axion - like partic
 les (ALPs) which may form ALP domain walls and ALP<br>
\nstars. Such i
 nteractions will have the signature of temporally coincident transient
 s occurring in multiple<br>
\nsensors in the network. I will in this t
 alk describe the experimental details of the network and review some<b
 r>
\ndata analysis ideas.
URL:https://www.physics.wisc.edu/events/?id=4990
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