Submission Type
Poster
Start Date
4-26-2021
Abstract
Our ultimate goal is to compute the gravitational waves in an extreme mass-ratio binary system. Since gravitational perturbations are difficult to calculate, we model the compact object as a point carrying a scalar charge q and moving around a spinning black holes.
In this project, we take advantage of symmetry under rotation around the spin axis in order to separate φ variables and leverage the periodicity of the source to separate t variable with a Fourier series. The remaining differential equations will be solved numerically with an appropriate discretization considering a grid of points in r-θ plane
Recommended Citation
Nishimura, Nami, "029— Calculating Gravitational Waves in a Black Hole Binary System" (2021). GREAT Day Posters. 47.
https://knightscholar.geneseo.edu/great-day-symposium/great-day-2021/posters-2021/47
029— Calculating Gravitational Waves in a Black Hole Binary System
Our ultimate goal is to compute the gravitational waves in an extreme mass-ratio binary system. Since gravitational perturbations are difficult to calculate, we model the compact object as a point carrying a scalar charge q and moving around a spinning black holes.
In this project, we take advantage of symmetry under rotation around the spin axis in order to separate φ variables and leverage the periodicity of the source to separate t variable with a Fourier series. The remaining differential equations will be solved numerically with an appropriate discretization considering a grid of points in r-θ plane
Comments
Sponsored by Thomas Osburn