Post-Newtonian-accurate pulsar timing array signals induced by inspiralling eccentric binaries: accuracy, computational cost, and single-pulsar search

DOI10.1088/1361-6382/ACE234zbMath1527.83030arXiv2210.11454OpenAlexW4382197534MaRDI QIDQ6170206

Unnamed Author

Publication date: 12 July 2023

Published in: Classical and Quantum Gravity (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/2210.11454

zbMATH Keywords

gravitational wavesbinariespulsars

Mathematics Subject Classification ID

Signal detection and filtering (aspects of stochastic processes) (60G35) Two-body problems (70F05) Galactic and stellar structure (85A15) Orbital mechanics (70M20) Gravitational waves (83C35) Uniqueness of trigonometric expansions, uniqueness of Fourier expansions, Riemann theory, localization (42A63)

Cites Work

• Unnamed Item
• A cubic approximation for Kepler's equation
• Gravitational Radiation from Point Masses in a Keplerian Orbit
• Gravitational radiation from post-Newtonian sources and inspiralling compact binaries

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