BEGIN:VCALENDAR
VERSION:2.0
PRODID:-//CERN//INDICO//EN
BEGIN:VEVENT
SUMMARY:Recent Progress in Numerical Modeling of Core-Collapse Supernovae 
 and Binary Neutron Star Mergers [CANCELLED]
DTSTART:20260521T084500Z
DTEND:20260521T091500Z
DTSTAMP:20260520T205800Z
UID:indico-event-25078@indico.gsi.de
CONTACT:g.martinez@gsi.de
DESCRIPTION:Speakers: Hiroki Nagakura (National Astronomical Observatory o
 f Japan)\n\nCore-collapse supernovae (CCSNe) and binary neutron star merge
 rs (BNSMs) are among the most energetic phenomena in the universe\, playin
 g central roles in the formation of compact objects (such as neutron stars
  and black holes) and the production of heavy elements. Understanding thes
 e events requires detailed numerical modeling that captures the interplay 
 between macrophysics (e.g.\, hydrodynamics and gravity) and microphysics (
 e.g.\, weak interactions\, the equation of state\, and nucleosynthesis). I
 n this talk\, I will present recent progress in theoretical studies of CCS
 Ne and BNSMs\, highlighting how numerical simulations have advanced our un
 derstanding of explosion mechanisms in CCSNe\, BNSM dynamics\, and their o
 bservable signatures. I will then discuss key open issues in the theory\, 
 focusing on neutrino quantum kinetics\, which governs neutrino transport\,
  matter interactions\, and flavor conversions. In particular\, I will pres
 ent our recent studies\, including large-scale global simulations of neutr
 ino quantum kinetics associated with collective neutrino oscillations. Fin
 ally\, I will outline future directions toward more realistic simulations 
 and their connection to multi-messenger observations.\n\nhttps://indico.gs
 i.de/event/25078/
LOCATION:SB3 3.170a (GSI)
URL:https://indico.gsi.de/event/25078/
END:VEVENT
END:VCALENDAR