|General Relativistic Simulations of Rotational Supernova Core Collapse in Axisymmetry with Microphysics (Extended Model Set)|
|MPA Homepage > Scientific Research > Research Groups > Relativistic Hydrodynamics > Axisymmetric Core Collapse with Microphysics (Extended Model Set) > EPS Figures|
C.D. Ott (Department of Astronomy and Steward Observatory, University of Arizona, U.S.A.)
Figures of the waveforms in EPS format:
These figures contain the time evolution of the maximum density and the signal amplitude for all 136 simulated models.
The vertical dotted lines mark the time of peak maximum density (time of bounce).