Neutron stars in the effective fly-by framework: f-mode re-summation

DOI10.1088/1361-6382/AC1083zbMath1482.85001arXiv2101.10963OpenAlexW3187070777MaRDI QIDQ5162929

J. Nijaid Arredondo, Nicholas Loutrel

Publication date: 8 November 2021

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

Full work available at URL: https://arxiv.org/abs/2101.10963

zbMATH Keywords

gravitational wavesneutron starspost-Newtonian approximationeccentric binariesf-modes

Mathematics Subject Classification ID

Two-body problems (70F05) Fourier series and coefficients in several variables (42B05) Galactic and stellar dynamics (85A05) Orbital mechanics (70M20) Gravitational waves (83C35) Approximation procedures, weak fields in general relativity and gravitational theory (83C25)

Related Items (1)

Eccentric catastrophes & what to do with them

Cites Work

• Analytic properties of Hansen coefficients
• Hereditary effects in eccentric compact binary inspirals to third post-Newtonian order
• A xylophone configuration for a third-generation gravitational wave detector
• Gravity
• Eccentric gravitational wave bursts in the post-Newtonian formalism
• Quasi-normal modes of stars and black holes
• Unnamed Item

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