Exploring waveforms with non-GR deviations for extreme mass-ratio inspirals
From MaRDI portal
Publication:6636411
DOI10.1088/1475-7516/2024/10/047zbMATH Open1548.83034MaRDI QIDQ6636411
Arpan Bhattacharyya, Rishabh Kumar Singh, Shailesh Kumar, Abhishek Chowdhuri
Publication date: 12 November 2024
Published in: Journal of Cosmology and Astroparticle Physics (Search for Journal in Brave)
equations of motionmodified gravitygravitational waves/theorygravitational waves in GR and beyond: theoryand 2-body problem in GR and beyond
Cites Work
- The effective field theorist's approach to gravitational dynamics
- Probes and tests of strong-field gravity with observations in the electromagnetic spectrum
- The Scalar-Tensor Theory of Gravitation
- Intermediate and extreme mass-ratio inspirals—astrophysics, science applications and detection using LISA
- Mapping spacetimes with LISA: inspiral of a test body in a ‘quasi-Kerr’ field
- Gravitational Radiation from Point Masses in a Keplerian Orbit
- Gravitational wave from extreme mass-ratio inspirals as a probe of extra dimensions
- Gravitational radiation from post-Newtonian sources and inspiralling compact binaries
- Extreme mass-ratio inspiral as a probe of extra dimensions: the case of spinning massive object
- Observables from classical black hole scattering in scalar-tensor theory of gravity from worldline quantum field theory
- Testing disformal non-circular deformation of Kerr black holes with LISA
- Prospects of detecting deviations to Kerr geometry with radiation reaction effects in EMRIs
- Unnamed Item
- Unnamed Item
This page was built for publication: Exploring waveforms with non-GR deviations for extreme mass-ratio inspirals
