• Corpus ID: 231582913

# Gravitational wave templates from Extreme Mass Ratio Inspirals

@inproceedings{Skoupy2021GravitationalWT,
title={Gravitational wave templates from Extreme Mass Ratio Inspirals},
author={Viktor Skoup'y and Georgios Lukes-Gerakopoulos Institute of Theoretical Physics and Faculty of Mathematics and Physics and Charles University and Prague and Czech Republic and Astronomical Institute of the Slovak Academy of Sciences},
year={2021}
}
• Published 12 January 2021
• Physics
An extreme mass ratio inspiral takes place when a compact stellar object is inspiraling into a supermassive black hole due to gravitational radiation reaction. Gravitational waves (GWs) from this system can be calculated using the Teukolsky equation (TE). In our case, we compute the asymptotic GW fluxes of a spinning body orbiting a Kerr black hole by solving numerically the TE both in time and frequency domain. Our ultimate goal is to produce GW templates for space-based detectors such as LISA…
4 Citations

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