Publication at Faculty of Mathematics and Physics |
2020
Abstract
We are using a time domain code to calculate the gravitational wave fluxes from extreme mass ratio inspirals. To test this code, we have to calculate the results with different method.
We have calculated the energy fluxes from spinning particles on circular equatorial orbits around a Kerr black hole in frequency domain to compare it with the time domain results. We used Black Hole Perturbation Toolkit to find the radial and angular function.