Reflecting scalar fields in numerical relativity


Dailey, C. (2022). Reflecting scalar fields in numerical relativity. Perimeter Institute. https://pirsa.org/22060049


Dailey, Conner. Reflecting scalar fields in numerical relativity. Perimeter Institute, Jun. 21, 2022, https://pirsa.org/22060049


          @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}}

Conner Dailey Perimeter Institute for Theoretical Physics

Talk Type Conference


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.