Understanding the orbits of spinning bodies in curved spacetime is important for modeling
binary black hole systems with small mass ratios. At zeroth order in mass ratio and ignoring …

Inspirals of stellar-mass compact objects into massive black holes, known as extreme mass
ratio inspirals (EMRIs), are one of the key targets for upcoming space-based gravitational …

Extreme mass-ratio inspirals (EMRIs) are one of the most sensitive probes of black hole
spacetimes with gravitational-wave measurements. In this work, we systematically analyze …

We introduce an action-angle formalism for bounded geodesic motion in Kerr black hole
spacetime using canonical perturbation theory. Namely, we employ a Lie series technique to …

Future space based gravitational wave detectors, such as the Laser Interferometer Space
Antenna (LISA) will allow for the detection of previously undetectable gravitational wave …

Extreme mass ratio inspirals (EMRIs), where a compact object orbits a massive black hole,
are a key source of gravitational waves for the future Laser Interferometer Space Antenna …

Large mass ratio binary black hole systems are essential for studying the two-body problem
in general relativity and are key sources of low-frequency gravitational waves. These …