A semi-relativistic model for tidal interactions in BH–NS coalescing binaries
From MaRDI portal
Publication:5324013
DOI10.1088/0264-9381/26/12/125004zbMath1170.83412arXiv0801.2911OpenAlexW3101353550WikidataQ59910850 ScholiaQ59910850MaRDI QIDQ5324013
Francesco Pannarale, Leonardo Gualtieri, Valeria Ferrari
Publication date: 3 August 2009
Published in: Classical and Quantum Gravity (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/0801.2911
Black holes (83C57) Galactic and stellar dynamics (85A05) Equations of motion in general relativity and gravitational theory (83C10)
Related Items (4)
Forecasting Gamma‐Ray Bursts Using Gravitational Waves ⋮ Gravitational waves from neutron stars: Promises and challenges ⋮ Stellar oscillations induced by the passage of a fast stellar object ⋮ BLACK HOLE–NEUTRON STAR COALESCING BINARIES
This page was built for publication: A semi-relativistic model for tidal interactions in BH–NS coalescing binaries