Video URL http://pirsa.org/22060049
Abstract
Black hole echoes have been considered as new probes to standard gravitational waveforms. Here, I consider reflections of scalar waves around a black hole as a model of black hole echoes arising from scalar fields. This problem is difficult due to the need for a proper understanding of the characteristic fields that propagate in numerical relativity. Using the "Einstein-Christoffel" system, I model the characteristic fields and the boundary conditions in such a way as to properly reflect scalar waves at a boundary using the full power of Einstein’s equations.
Details
Talk Number
22060049
Speaker Profile
Conner Dailey
Collection
Young Researchers Conference
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Scientific Area
- Other Physics
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Talk Type
- Conference
Subject
Physics
Source Repository
PIRSA