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SUMMARY:Mode spectrum of the electromagnetic field in open universe models
DTSTART;VALUE=DATE-TIME:20120523T090000Z
DTEND;VALUE=DATE-TIME:20120523T100000Z
DTSTAMP;VALUE=DATE-TIME:20130522T152227Z
UID:indico-event-188899@cern.ch
DESCRIPTION:It has been claimed that in open FRW there exist magnetic fiel
 d\nmodes which decay slower than at the usual "adiabatic" rate of\nB ~ 1/a
 ²\, so-called "supercurvature" modes. If they are present\, it was\nargue
 d that the residual field strength in these modes could be of\ncosmologica
 l relevance even if our Universe is only marginally open\,\nwith (1 - Omeg
 a_0) \n\nhttp://indico.cern.ch/conferenceDisplay.py?confId=188899
LOCATION:CERN TH common room
URL:http://indico.cern.ch/conferenceDisplay.py?confId=188899
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