Gravitational waves from extreme-mass-ratio inspirals in equatorially eccentric orbits
From MaRDI portal
Publication:2876549
DOI10.1142/S0218271814500643zbMath1293.83013OpenAlexW2168464293MaRDI QIDQ2876549
Publication date: 19 August 2014
Published in: International Journal of Modern Physics D (Search for Journal in Brave)
Full work available at URL: https://doi.org/10.1142/s0218271814500643
Observational and experimental questions in relativity and gravitational theory (83B05) Gravitational waves (83C35)
Related Items (1)
Cites Work
- Analytic black hole perturbation approach to gravitational radiation
- Gravitational Radiation from a Kerr Black Hole. I. Formulation and a Method for Numerical Analysis
- Gravitational Field of a Particle Falling in a Schwarzschild Geometry Analyzed in Tensor Harmonics
- Stability of a Schwarzschild Singularity
- Gravitational self-force in extreme mass-ratio inspirals
- New Numerical Methods to Evaluate Homogeneous Solutions of the Teukolsky Equation
- Event rate estimates for LISA extreme mass ratio capture sources
- Binary black hole merger in the extreme-mass-ratio limit
- Intermediate and extreme mass-ratio inspirals—astrophysics, science applications and detection using LISA
- An Efficient Numerical Method for Computing Gravitational Waves Induced by a Particle Moving on Eccentric Inclined Orbits around a Kerr Black Hole
- New Numerical Methods to Evaluate Homogeneous Solutions of the Teukolsky Equation. II: -- Solutions of the Continued Fraction Equation --
- The motion of point particles in curved spacetime
This page was built for publication: Gravitational waves from extreme-mass-ratio inspirals in equatorially eccentric orbits
