Speaker
Haakon Andresen
(Stockholm University)
Description
I will present recent results from 60 axisymmetric core-collapse simulations performed with FLASH. I will describe how the power gap, a narrow band of reduced emission observed in predicted gravitational wave signals, correlates with the properties of the numerical simulations. I will give an overview of proposed explanations and how well these explanations work for our set of simulations.
Author
Haakon Andresen
(Stockholm University)