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SUMMARY:Extreme States of Nuclear Matter
DESCRIPTION:After a pedagogical introduction to the basics of the strong interaction, we discuss neutron stars: the most compact stellar objects.
Various  phases of matter can be realized in their interior, in particular we focus on some phases that are superfluid and rigid at the same time. 
We conclude with a brief analysis of some astrophysical observables linked to the internal structure of neutron stars.
LOCATION:Erwin Schrödinger Saal
DTSTART:20230222T090000
DTEND:20230222T103000
TZID: Europe/Vienna
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