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From the 1 of 5 linked papers with an AI index.

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5 papers

astro-ph.GA2026

Discrepancies between Chandrasekhar's theory of relaxation and -body simulations

Kerwann Tep, Douglas C. Heggie

The paper compares Chandrasekian orbit‑averaged relaxation theory with high‑precision N‑body simulations of anisotropic globular clusters, finding reduced but still position‑depend…

astro-ph.GA2026

Very long-term relaxation of harmonic 1D self-gravitating systems

Kerwann Tep, Jean-Baptiste Fouvry, Christophe Pichon

One-dimensional self-gravitating systems admit genuine thermodynamical equilibria. For systems with strictly monotonic orbital frequency profile, the Landau and Balescu-Lenard theo…

astro-ph.GA2026

Modeling Globular Cluster Stellar Streams with a Basis-Expansion N-body Code

Brian T. Cook, Kerwann Tep, Carl L. Rodriguez +6

Globular cluster stellar streams probe galaxy-formation processes and can potentially reveal the distribution of dark matter in galaxies. In many theoretical studies, streams are m…

astro-ph.GA2025

KRIOS: A new basis-expansion -body code for collisional stellar dynamics

Kerwann Tep, Brian T. Cook, Carl L. Rodriguez +4

The gravitational -body problem is a nearly universal problem in astrophysics which, despite its deceptive simplicity, still presents a significant computational challenge. For…

astro-ph.GA2025

Linear response of rotating and flattened stellar clusters: the oblate Kuzmin-Kutuzov Stäckel family

Kerwann Tep, Christophe Pichon, Michael S Petersen

This paper investigates the linear response of a series of spheroidal stellar clusters, the Kuzmin-Kutuzov Stäckel family, which exhibit a continuous range of flattening and rotat…