Monte Carlo Simulations of Star Clusters

Mirek Giersz (Nicolaus Copernicus Astronomical Center; Poland); Warsaw

Monte Carlo Simulations of Star Clusters

Not yet reviewed by Pith; the record is open.

Re-run · record.json Download PDF Read on arXiv ↗

This paper has not been read by Pith yet. Machine review is queued; the pith claim, tier, and objections will appear here once it completes.

SPECIMEN: schema-true, not a live event

T0 review · schema-true

One-sentence machine reading of the paper's core claim.

pith:XXXXXXXX · record.json · timestamp

arxiv astro-ph/0006438 v1 pith:7UBLRERB submitted 2000-06-30 astro-ph

Mirek Giersz (Nicolaus Copernicus Astronomical Center , Warsaw , Poland) This is my paper · ORCID

classification astro-ph

keywords evolutionstarcarloclustersmontebasesbodycluster

verification ladder T0 review T1 audit T2 compute T3 formal

0 comments

read the original 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. \

Discussion (0). Continue with ORCID to comment.

Forward citations

Cited by 1 Pith paper

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

Detection of Intermediate-Mass Ratio Inspirals in Globular Clusters: Revealing the Brownian Motion with Gravitational Waves
astro-ph.HE 2025-01 conditional novelty 5.0 of 10

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.

Pith tools