Post-Keplerian waveform model for binary compact object as sources of space-based gravitational wave detector and its implications

DOI10.1007/S10714-023-03123-6zbMath1528.83014arXiv2306.10445OpenAlexW4380885434MaRDI QIDQ6174897

Zhoujian Cao, Li-Fang Li

Publication date: 15 July 2023

Published in: General Relativity and Gravitation (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/2306.10445

zbMATH Keywords

mass transfergravitational wavetidal interactionbinary compact objectpost-Keplerian waveform model

Mathematics Subject Classification ID

Black holes (83C57) Fluid-solid interactions (including aero- and hydro-elasticity, porosity, etc.) (74F10) Signal detection and filtering (aspects of stochastic processes) (60G35) Orbital mechanics (70M20) Gravitational waves (83C35) Adiabatic invariants for problems in Hamiltonian and Lagrangian mechanics (70H11) Sets with a single binary operation (groupoids) (20N02) Diffusive and convective heat and mass transfer, heat flow (80A19)

Cites Work

• The LISA verification binaries
• The two-body problem in the (truncated) PPN ? Theory
• Tensor-multi-scalar theories of gravitation

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