Monte Carlo cluster simulations to determine the rate of compact star inspiralling to a central galactic black hole
From MaRDI portal
Publication:2771217
DOI10.1088/0264-9381/18/19/309zbMath0992.83052arXivastro-ph/0107193OpenAlexW2084401962MaRDI QIDQ2771217
Publication date: 11 April 2002
Published in: Classical and Quantum Gravity (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/astro-ph/0107193
Black holes (83C57) Observational and experimental questions in relativity and gravitational theory (83B05) Computational methods for problems pertaining to relativity and gravitational theory (83-08)
Related Items (2)
Sources and technology for an atomic gravitational wave interferometric sensor ⋮ Monte-Carlo Models of Collisional Stellar Systems
This page was built for publication: Monte Carlo cluster simulations to determine the rate of compact star inspiralling to a central galactic black hole