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DTSTART;TZID=Europe/Rome:20200114T114500
DTEND;TZID=Europe/Rome:20200114T124500
DTSTAMP:20260407T081556
CREATED:20191008T060530Z
LAST-MODIFIED:20200107T140305Z
UID:6889-1579002300-1579005900@www.oa-roma.inaf.it
SUMMARY:The two-families scenario: what does it predict?
DESCRIPTION:I will revisit the two-families scenario in which neutron stars coexist with strange quark stars\, i.e. with compact objects made almost\nentirely of deconfined quarks. I will outline the differences between this scenario and other schemes in which quark matter appears only at the center of compact stars and I will discuss how it compares with GW170817\, GRB170817A\, AT2017gfo and with the existing limits on masses and radii of compact stars.
URL:https://www.oa-roma.inaf.it/event/colloquium-alessandro-drago/
LOCATION:Aula Gratton
CATEGORIES:Seminari
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