Highlights
As the TEAMS collaboration pursues its mission to understand the astrophysical origin of the elements through simulations of astrophysical objects and events using the highest-performing computational resources available, we will periodically publish publicly accessible highlights of our results, in addition to our scholarly papers and presentations.
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Core-Collapse Supernova Explosion Theory (2021)
contact: Adam Burrows (Princeton) -
Supernova neutrino signals based on long-term axisymmetric simulations (2021)
contact: Adam Burrows (Princeton) - Equation
of State from Multi-Messenger Observations
contact: Andrew W. Steiner (UTK/ORNL) -
Three-Dimensional CCSN Explosion Models using Fornax (2019)
contact: Adam Burrows (Princeton) -
Neutron-Star Merger Simulations (2018)
contact: David Radice (Princeton/IAS) -
Gravitational Waves from 3D CCSN models
contact: David Radice (Princeton/IAS) -
Fornax (CCSN simulation capability) code paper
contact: Adam Burrows (Princeton) -
MAESTROeX Low Mach Number Solver
contact: Andy Nonaka (LBL) -
Microphysics Dependence of CCSN Explosions
contact: Adam Burrows (Princeton) -
Explosions of Low-Mass Massive Stars
contact: David Radice (Princeton) -
Gravitational Waves from Core-Collapse Supernovae
contact: Vikotoriya Morozova (Princeton) -
Exploding 3D CCSN Model
contact: Adam Burrows (Princeton) -
3D Fornax Supernova Simulation
contact: Adam Burrows (Princeton) -
3D Kilonova Model
contact: Jonah Miller (LANL) -
3D CCSN Correlations
contact: David Vartanyan (Berkeley) -
Resolution Dependence of CCSN 3D Simulations
contact: Hiroki Nagakura (Princeton) -
The Overarching Framework of Core-Collapse Supernova Explosions as Revealed by 3D Fornax simulations
contact: Adam Burrows (Princeton) - Equation
of State Distribution for Simulations
contact: Andrew W. Steiner (UTK/ORNL) -
A systematic study of proto-neutron star convection in three-dimensional core-collapse supernova simulations
contact: Adam Burrows (Princeton)