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DTSTAMP:20230124T170806Z
LOCATION:Lower Lobby C
DTSTART;TZID=America/Chicago:20221117T083000
DTEND;TZID=America/Chicago:20221117T170000
UID:submissions.supercomputing.org_SC22_sess279_svs107@linklings.com
SUMMARY:Visualizing the Supernova Explosion of a 25-Solar-Mass Star and th
 e Simultaneous Birth of a Neutron-Star
DESCRIPTION:Posters, Scientific Visualization & Data Analytics Showcase\n\
 nVisualizing the Supernova Explosion of a 25-Solar-Mass Star and the Simul
 taneous Birth of a Neutron-Star\n\nInsley, Alvarez, Brynteson, Burrows, Mu
 rphy\n\nThis explanatory visualization shows the results of a state-of-the
 -art 3D simulation of supernova explosion and neutron-star birth. It is a 
 rare instance where the full stellar evolution of an object, including the
  physics of the convection and the radiation, has been simulated in three 
 dimensions. Among the highlights is the deep core that is shrinking after 
 explosion due to neutrino cooling and deleptonization on its way to becomi
 ng a cold, compact neutron star. There is also evidence of inner proto-neu
 tron star convection, perhaps the site of magnetic dynamo action that can 
 turn a pulsar into a magnetar. An exterior view shows the blast wave, whic
 h cocoons the newly-birthed neutron star, moving at ∼10,000 km/s. Addition
 ally, a reusable pipeline was developed, which leverages state-of-the-art 
 tools for scientific data analysis and visualization resulting in high-qua
 lity renderings.\n\nRegistration Category: Tech Program Reg Pass, Exhibits
  Reg Pass
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