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DTSTAMP:20260718T000702Z
UID:https://www.ipp.mpg.de/events/13284/4597191
DTSTART:20180504T083000Z
DTEND:20180504T100000Z
CLASS:PUBLIC
CREATED:20180313T132857Z
DESCRIPTION:Neutron stars are born as the endpoint of stellar evolution in 
 core-collapse supernovae. The densities in a neutron star are extremely hi
 gh\, so high that nuclei are squeezed into their constituents\, neutrons a
 nd protons. Exotic matter can appear in the core\, either in the form of h
 yperons or as a new phase in the form of strange quark matter. The propert
 ies of neutron stars are determined by the nuclear equation of state of de
 nse matter\, so that the observation of neutron stars and neutron star mer
 ger can give a telltale signature of the properties of dense matter under 
 extreme conditions. The present astrophysical data on neutron stars and pu
 lsars\, rotation-powered neutron stars\, is reviewed. The equation of stat
 e of dense matter will be discussed and possible implications for future o
 bservations of core-collapse supernovae and neutron star mergers will be o
 utlined.\nVortragende(r): Prof. Dr. Jürgen Schaffner-Bielich
LAST-MODIFIED:20180611T104317Z
LOCATION:Garching und Greifswald\, Raum: Hörsaal D2 (Übertragung nach HGW
  S1)
SUMMARY:Institutskolloquium: Dense matter in neutron stars
URL;VALUE=URI:https://www.ipp.mpg.de/events/13284/4597191
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