Numerical black holes in dynamical Chern-Simons gravity
APA
Okounkova, M. (2018). Numerical black holes in dynamical Chern-Simons gravity. Perimeter Institute. https://pirsa.org/18090050
MLA
Okounkova, Maria. Numerical black holes in dynamical Chern-Simons gravity. Perimeter Institute, Sep. 27, 2018, https://pirsa.org/18090050
BibTex
@misc{ pirsa_PIRSA:18090050, doi = {10.48660/18090050}, url = {https://pirsa.org/18090050}, author = {Okounkova, Maria}, keywords = {Strong Gravity}, language = {en}, title = {Numerical black holes in dynamical Chern-Simons gravity}, publisher = {Perimeter Institute}, year = {2018}, month = {sep}, note = {PIRSA:18090050 see, \url{https://pirsa.org}} }
This talk will explore the applications of the computing power of numerical relativity to gravitational theories beyond general relativity. Specifically, I will consider dynamical Chern-Simons gravity, which has roots in string theory and loop quantum gravity. I will discuss our formalism and efforts to simulate binary black holes in this theory to generate waveforms LIGO and LISA. Additionally, I will discuss the generation of numerical black hole solutions in this theory, and applications to probing black hole shadows with the Event Horizon Telescope.