Brownian motion from stellar encounters in globular clusters imprints Doppler and aberrational phase shifts on IMRI gravitational waves that should be detectable for most sources loud enough for TianQin, LISA, or AION to see.
Monte Carlo Simulations of Star Clusters
1 Pith paper cite this work. Polarity classification is still indexing.
1
Pith paper citing it
abstract
A revision of Stod\'o{\l}kiewicz's Monte Carlo code is used to simulate evolution of large star clusters. The survey on the evolution of multi-mass N-body systems influenced by the tidal field of a parent galaxy and by stellar evolution is discussed. For the first time, the simulation on the "star-by-star" bases of evolution of 1,000,000 body star cluster is presented. \
fields
astro-ph.HE 1years
2025 1verdicts
CONDITIONAL 1representative citing papers
citing papers explorer
-
Detection of Intermediate-Mass Ratio Inspirals in Globular Clusters: Revealing the Brownian Motion with Gravitational Waves
Brownian motion from stellar encounters in globular clusters imprints Doppler and aberrational phase shifts on IMRI gravitational waves that should be detectable for most sources loud enough for TianQin, LISA, or AION to see.