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X-WR-CALDESC:Events for LBNL Physics Division Research Progress Meetings
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DTSTART;TZID=America/Los_Angeles:20170316T160000
DTEND;TZID=America/Los_Angeles:20170316T170000
DTSTAMP:20260422T224403
CREATED:20170117T120837Z
LAST-MODIFIED:20170117T120837Z
UID:439-1489680000-1489683600@rpm.physics.lbl.gov
SUMMARY:Prof. Stacy McGaugh (Case Western) "The Radial Acceleration Relation in Rotationally Supported Galaxies"
DESCRIPTION:ABSTRACT:\nWe report a correlation between the radial acceleration traced by rotation curves and that predicted by the observed distribution of baryons. The same relation is followed by 2693 points in 153 galaxies with very different morphologies\, masses\, sizes\, and gas fractions. The correlation persists even when dark matter dominates. Consequently\, the dark matter contribution is fully specified by that of the baryons. The observed scatter is small and largely dominated by observational uncertainties. This radial acceleration relation is tantamount to a natural law for rotating galaxies.
URL:https://rpm.physics.lbl.gov/event/stacy-mcgaugh-case-western-tba/
LOCATION:Zoom Talk\, 50A-5132\, Berkeley\, ca\, 94720
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