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Multi-D Core-Collapse Supernova Models: where we are and where we are going?

  • 25 de març de 2015
Imatge conferència Key Kotake

Conferències al DAA. Xarrada a càrrec de l'investigador Key Kotake del Department of Applied Physics, de la Fukuoka University. Lloc: Seminari del Departament d'Astronomia i Astrofísica, 4a planta de l'Edifici d'Investigació, a Burjassot. Dia: dimecres 25 de març. Hora: 12:00.

Abstract:
After we summarize a recent status of core-collapse supernova models, we report our recent results based on two-(2D) and three-dimensional (3D) radiation-hydrodynamics simulations. We also talk about signals of neutrinos and gravitational waves expected from the self-consistent models, which would be important to extract the information of the central engine from the multi-messenger observations. We also report our code development where 3D general-relativistic hydrodynamics is now meeting with spectral neutrino transport.

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