Reflecting scalar fields in numerical relativity
APA
Dailey, C. (2022). Reflecting scalar fields in numerical relativity. Perimeter Institute. https://pirsa.org/22060049
MLA
Dailey, Conner. Reflecting scalar fields in numerical relativity. Perimeter Institute, Jun. 21, 2022, https://pirsa.org/22060049
BibTex
@misc{ pirsa_PIRSA:22060049, doi = {10.48660/22060049}, url = {https://pirsa.org/22060049}, author = {Dailey, Conner}, keywords = {Other}, language = {en}, title = {Reflecting scalar fields in numerical relativity}, publisher = {Perimeter Institute}, year = {2022}, month = {jun}, note = {PIRSA:22060049 see, \url{https://pirsa.org}} }
Perimeter Institute for Theoretical Physics
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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.