n -body simulations (Makino Inc)
90
Structured Review
Makino Inc
n -body simulations
N Body Simulations, supplied by Makino Inc, used in various techniques. Bioz Stars score: 90/100, based on 1 PubMed citations. ZERO BIAS - scores, article reviews, protocol conditions and more
https://www.bioz.com/product/n+body+simulations/n+body+simulations/10__1093_slash_mnras_slash_stad117-225-1-6
Average 90 stars, based on 1 article reviews
N Body Simulations, supplied by Makino Inc, used in various techniques. Bioz Stars score: 90/100, based on 1 PubMed citations. ZERO BIAS - scores, article reviews, protocol conditions and more
https://www.bioz.com/product/n+body+simulations/n+body+simulations/10__1093_slash_mnras_slash_stad117-225-1-6
Average 90 stars, based on 1 article reviews
n -body simulations - by Bioz Stars,
2026-10
90/100 stars
Images
Related Articles
other:Article Title: Formation of galactic nuclei with multiple supermassive black holes at high redshifts Article Snippet: In N-body simulations, the last stage is known to have a dependence on the number of particles N such that the hardening rate decreases with increasing Article Title: Eccentric binary black hole mergers in globular clusters hosting intermediate-mass black holes Article Snippet: Several attempts have been made in modelling the dynamics of Article Title: Galaxy Core Formation by Supermassive Black Hole Binaries: the Importance of Realistic Initial Conditions and Galaxy Morphology Article Snippet: The main reason for this is that the numerical techniques employed in most work are based either on direct Isolation:Article Title: Collisionless loss-cone refilling: there is no final parsec problem Article Snippet: .. In N-body simulations of isolated spherical models, this regime can be identified by the N-dependence of the binary hardening rate, since the relaxation time scales approximately as Article Title: Collisionless loss-cone refilling: there is no final parsec problem Article Snippet: .. In N-body simulations of isolated spherical models, this regime can be identified by the N-dependence of the binary hardening rate, since the relaxation time-scales approximately as Article Title: Brownian motion of massive black hole binaries and the final parsec problem Article Snippet: .. However, the coalescence of BHBs has been put under scrutiny in the past years due to theoretical arguments on loss cone refilling (e.g. Begelman et al. 1980) and N-body simulations of BHB pairing in isolated Article Title: Brownian motion of massive black hole binaries and the final parsec problem Article Snippet: .. However, the coalescence of BHBs has been put under scrutiny in the past years due to theoretical arguments on loss cone refilling (e.g. Begelman et al. 1980) and N-body simulations of BHB pairing in isolated |