Magnetic effects on the generation of gravitational waves in a black hole-neutron star binary system

DOI10.1088/1361-6382/AB7D80zbMath1479.83046OpenAlexW3010288938MaRDI QIDQ5161976

Mattia Villani

Publication date: 1 November 2021

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

Full work available at URL: https://doi.org/10.1088/1361-6382/ab7d80

zbMATH Keywords

neutron starsclassical black holesgravitational waves: generation and sources

Mathematics Subject Classification ID

Black holes (83C57) Two-body problems (70F05) Galactic and stellar structure (85A15) Gravitational waves (83C35) Motion of the gyroscope (70E05) Mono-, di- and multipole moments (EM and other), gyromagnetic relations (81V60)

Related Items (1)

Stability of the Hayward black hole under electromagnetic perturbations

Cites Work

• Unnamed Item
• Unnamed Item
• Unnamed Item
• Unnamed Item
• Center of Mass, Spin Supplementary Conditions, and the Momentum of Spinning Particles
• The third and a half-post-Newtonian gravitational wave quadrupole mode for quasi-circular inspiralling compact binaries
• Quadratic-in-spin effects in the orbital dynamics and gravitational-wave energy flux of compact binaries at the 3PN order
• Radiative gravitational fields in general relativity I. General structure of the field outside the source
• Gravitational radiation reaction in the equations of motion of compact binaries to 3.5 post-Newtonian order
• A Relativist's Toolkit
• Next-to-next-to-leading order spin–orbit effects in the equations of motion of compact binary systems
• Next-to-next-to-leading order spin–orbit effects in the near-zone metric and precession equations of compact binaries
• Cubic-order spin effects in the dynamics and gravitational wave energy flux of compact object binaries
• Gravitational radiation from post-Newtonian sources and inspiralling compact binaries

This page was built for publication: Magnetic effects on the generation of gravitational waves in a black hole-neutron star binary system