Monte-Carlo Models of Collisional Stellar Systems

DOI10.1007/978-1-4020-8431-7_5zbMath1305.85014OpenAlexW1539576453MaRDI QIDQ5171868

Marc Freitag

Publication date: 12 February 2015

Published in: The Cambridge N-Body Lectures (Search for Journal in Brave)

Full work available at URL: https://doi.org/10.1007/978-1-4020-8431-7_5

Mathematics Subject Classification ID

Galactic and stellar dynamics (85A05) Computational methods for problems pertaining to astronomy and astrophysics (85-08)

Cites Work

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• Massive black hole binary evolution
• A time-transformed leapfrog scheme. Integration of few-body systems with large mass ratios
• Monte Carlo cluster simulations to determine the rate of compact star inspiralling to a central galactic black hole
• The Gravitational Million–Body Problem
• A new Monte Carlo code for star cluster simulations
• Intermediate and extreme mass-ratio inspirals—astrophysics, science applications and detection using LISA
• INTERMEDIATE-MASS BLACK HOLES
• Gravitational N-Body Simulations
• Gravitational Radiation from Point Masses in a Keplerian Orbit
• Relativistic binaries in globular clusters

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