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DTSTART:20070311T020000
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DTSTAMP:20260807T095615
DTSTART;TZID=America/Detroit:20261016T150000
DTEND;TZID=America/Detroit:20261016T160000
SUMMARY:Lecture / Discussion:HET Seminar | Cosmological Seed Magnetic Field from Inflation
DESCRIPTION:A cosmological magnetic field of nG strength on Mpc length scales could be the seed magnetic field needed to explain observed few microG large-scale galactic magnetic fields. I first briefly review the observational and theoretical motivations for such a seed field\, two galactic magnetic field amplification models\, and some non-inflationary seed field generation scenarios. I then discuss an inflation magnetic field generation model. I conclude by mentioning possible extensions of this model as well as potentially observable consequences.
UID:149986-21907766@events.umich.edu
URL:https://events.umich.edu/event/149986
CLASS:PUBLIC
STATUS:CONFIRMED
CATEGORIES:High Energy Theory Seminar,lecture,Natural Sciences,Physics,Science,Seminar
LOCATION:West Hall - 340
CONTACT:
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