Light echos and coherent autocorrelations in a black hole spacetime
APA
Chesler, P. (2021). Light echos and coherent autocorrelations in a black hole spacetime. Perimeter Institute. https://pirsa.org/21020052
MLA
Chesler, Paul. Light echos and coherent autocorrelations in a black hole spacetime. Perimeter Institute, Feb. 25, 2021, https://pirsa.org/21020052
BibTex
@misc{ pirsa_PIRSA:21020052, doi = {10.48660/21020052}, url = {https://pirsa.org/21020052}, author = {Chesler, Paul}, keywords = {Strong Gravity}, language = {en}, title = {Light echos and coherent autocorrelations in a black hole spacetime}, publisher = {Perimeter Institute}, year = {2021}, month = {feb}, note = {PIRSA:21020052 see, \url{https://pirsa.org}} }
Light rays can orbit the photon shell of a black hole many times before escaping to infinity. This means that a distant observer can see a successive series of "echo" images, each separated in time by the photon shell orbital period, and each dimmer than the previous. I will present a study of light echos using coherent autocorrelation functions sourced by fluctuating matter in accretion flows. I will demonstrate that coherent autocorrelation functions are peaked at integer multiples of the photon shell orbital period. Furthermore, I will argue that the power in echos from supermassive black holes is too small to be observed on Earth.
Zoom Link: https://pitp.zoom.us/j/92751681169?pwd=V0hQeUMwaWtTQjQ3UzdxekJiT0lmQT09