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2022

Adiabatic equatorial inspirals of a spinning body into a Kerr black hole

Skoupý, Viktor, Lukes-Gerakopoulos, Georgios

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The detection of gravitational waves from Extreme mass Ratio Inspirals (EMRIs) by the future space-based gravitational-wave detectors demands the generation of accurate enough waveform templates.

Since the spin of the smaller secondary body cannot be neglected for the detection and parameter estimation of EMRIs, we study its influence on the phase of the gravitational waves from EMRIs with spinning secondary.
We focus on generic eccentric equatorial orbits around a Kerr black hole.
To model the spinning secondary object, we use the Mathisson-Papapetrou-Dixon equations in the pole-dipole approximation.

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