INTERMEDIATE-MASS BLACK HOLES

DOI10.1142/S0218271804004426zbMath1079.83500arXivastro-ph/0308402MaRDI QIDQ5700022

M. Coleman Miller, E. J. M. Colbert

Publication date: 27 October 2005

Published in: International Journal of Modern Physics D (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/astro-ph/0308402

zbMATH Keywords

gravitational wavesstellar dynamicsBlack hole physicsX-rays: binaries(galaxy) globular clusters: general

Mathematics Subject Classification ID

Black holes (83C57) Research exposition (monographs, survey articles) pertaining to relativity and gravitational theory (83-02) Galactic and stellar dynamics (85A05) Gravitational waves (83C35) Research exposition (monographs, survey articles) pertaining to astronomy and astrophysics (85-02)

Related Items (8)

Black-hole binaries, gravitational waves, and numerical relativity ⋮ Astrophysical Black Holes: A Compact Pedagogical Review ⋮ Spin and quadrupole couplings for high spin equatorial intermediate mass-ratio coalescences ⋮ Monte-Carlo Models of Collisional Stellar Systems ⋮ Relativistic binaries in globular clusters ⋮ Improvements to the construction of binary black hole initial data ⋮ Relativistic binaries in globular clusters ⋮ BLACK HOLES AS DARK MATTER ANNIHILATION BOOSTERS

Cites Work

• A time-transformed leapfrog scheme. Integration of few-body systems with large mass ratios
• LISA sources in globular clusters
• Gravitational waves from extreme mass ratio inspirals: challenges in mapping the spacetime of massive, compact objects
• The influence of gravitational wave momentum losses on the centre of mass motion of a Newtonian binary system
• Classical Radiation Recoil
• The dynamical decay of unstable 4-body systems
• Non-restricted double-averaged three body problem in Hill's case
• Gravitational waves from inspiralling binary black holes
• Gravitational radiation from black hole binaries in globular clusters
• Relativistic binaries in globular clusters

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