Friday, December 18, 2020, 9:00 am — https://bluejeans.com/487211447
Abstract: The observed mass and radius relations of neutron stars can be explained remarkably well using a model of dense matter known as quarkyonic matter. I describe how the quarkyonic model can arise dynamically from an excluded volume model for nuclear interactions. I also discuss how thermal effects can be incorporated in such a model.
Hosted by: Semeon Valgushev
16033 | INT/EXT | Events Calendar
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