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SUMMARY:321D modelling of the evolution\, nucleosynthesis and fate of mass
 ive stars
DTSTART:20250423T113000Z
DTEND:20250423T123000Z
DTSTAMP:20260417T055800Z
UID:indico-event-22176@indico.gsi.de
CONTACT:t.neff@gsi.de
DESCRIPTION:Speakers: Raphael Hirschi (Keele University\, UK)\n\nMassive s
 tars play a key role in the Universe through the light they shine\, the ch
 emical elements they produce and the supernova explosions that mark their 
 death. They leave remnants (neutron stars or black holes) that can later m
 erge and emit gravitational waves (GW)\, which we can now detect with dete
 ctors such as LIGO and Virgo. In this talk\, I will review the properties 
 and evolution of massive stars and present theoretical predictions for the
 ir fate and the remnant they produce across cosmic times. I will also disc
 uss the prospect of detecting rare supernova types and the key uncertainti
 es affecting theoretical predictions. Finally\, I will review the expected
  and unexpected nucleosynthesis taking place in the late phases of their e
 volution.\n\nhttps://indico.gsi.de/event/22176/\n\nZoom: https://gsi-fair.
 zoom.us/j/92473872583
LOCATION:KBW 2.27 (GSI)
URL:https://indico.gsi.de/event/22176/
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