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VERSION:2.0
CALSCALE:GREGORIAN
PRODID:UW-Madison-Physics-Events
BEGIN:VEVENT
SEQUENCE:2
UID:UW-Physics-Event-6349
DTSTART:20211109T200000Z
DTEND:20211109T210000Z
DTSTAMP:20260414T193124Z
LAST-MODIFIED:20211105T002748Z
LOCATION:https://berkeley.zoom.us/j/99464252867
SUMMARY:Quarkyonic model for neutron stars\, Network in Neutrinos\, Nu
 clear Astrophysics\, and Symmetries (N3AS) Seminar\, Srimoyee Sen \, I
 owa State University
DESCRIPTION:The observed mass and radius relations of neutron stars ca
 n be explained remarkably well using a model of dense matter known as 
 quarkyonic matter. I describe how the quarkyonic matter can arise dyna
 mically from an excluded volume model for nuclear interactions and how
  thermal effects can be incorporated in such a model. I also discuss h
 ow one can improve the excluded volume model to correctly reproduce lo
 w energy nuclear interactions and recover mass radius relations of neu
 tron stars.  
URL:https://www.physics.wisc.edu/events/?id=6349
END:VEVENT
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