Eccentric self-forced inspirals into a rotating black hole
DOI10.1088/1361-6382/AC7507zbMath1498.83029arXiv2112.05651OpenAlexW4281730249MaRDI QIDQ5090128
Philip Lynch, Niels Warburton, Maarten van de Meent
Publication date: 15 July 2022
Published in: Classical and Quantum Gravity (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/2112.05651
eccentricityrelativistic celestial mechanicsextreme mass ratio inspiralsgravitational waveform modelinggravitational self force
Black holes (83C57) Relativistic dynamics for problems in Hamiltonian and Lagrangian mechanics (70H40) Geodesics in global differential geometry (53C22) Yang-Mills and other gauge theories in mechanics of particles and systems (70S15) Celestial mechanics (70F15) Orbital mechanics (70M20) Gravitational waves (83C35) Motion of the gyroscope (70E05)
Cites Work
- Analytical solutions of bound timelike geodesic orbits in Kerr spacetime
- Gravitational self-force in extreme mass-ratio inspirals
- Perturbation Techniques for Oscillatory Systems with Slowly Varying Coefficients
- Transition of EMRIs through resonance: Corrections to higher order in the on-resonance flux modification
- New Numerical Methods to Evaluate Homogeneous Solutions of the Teukolsky Equation
- Analytic solutions for parallel transport along generic bound geodesics in Kerr spacetime
- The mass and angular momentum of reconstructed metric perturbations
- Hamiltonian formulation of the conservative self-force dynamics in the Kerr geometry
- An Efficient Numerical Method for Computing Gravitational Waves Induced by a Particle Moving on Eccentric Inclined Orbits around a Kerr Black Hole
- Global Structure of the Kerr Family of Gravitational Fields
- The motion of point particles in curved spacetime
This page was built for publication: Eccentric self-forced inspirals into a rotating black hole
