activity
20212026
most citedMapping the Galactic centre's dark cluster via Resonant Relaxation

16 citations · 26 across the 10 of their papers we have counts for

collaborators

10 papers

astro-ph.GA2026

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

Kerwann Tep, Douglas C. Heggie

Globular clusters are systems which are known to be particularly well described by two-body relaxation. In recent decades many studies have shown that Chandrasekhar's orbit-average…

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★ 1 cited

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.GA2024★ 1 cited

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 rotati…

astro-ph.GA2024★ 2 cited

Non-resonant relaxation of rotating globular clusters

Kerwann Tep, Jean-Baptiste Fouvry, Christophe Pichon

The long-term relaxation of rotating, spherically symmetric globular clusters is investigated through an extension of the orbit averaged Chandrasekhar non-resonant formalism. A com…

astro-ph.GA2023★ 1 cited

Predicting the linear response of self-gravitating stellar spheres and discs with LinearResponse.jl

Michael S. Petersen, Mathieu Roule, Jean-Baptiste Fouvry +2

We present LinearResponse.jl, an efficient, versatile public library written in julia to compute the linear response of self-gravitating (3D spherically symmetric) stellar spheres…

astro-ph.GA2022★ 4 cited

Non-resonant relaxation of anisotropic globular clusters

Kerwann Tep, Jean-Baptiste Fouvry, Christophe Pichon

Globular clusters are dense stellar systems whose core slowly contracts under the effect of self-gravity. The rate of this process was recently found to be directly linked to the i…

astro-ph.GA2021★ 1 cited

The NewHorizon Simulation -- To Bar Or Not To Bar

J. Reddish, K. Kraljic, M. S. Petersen +12

We use the NewHorizon simulation to study the redshift evolution of bar properties and fractions within galaxies in the stellar masses range $M_{\star} = 10^{7.25} - 10^{11.4} \ \r…

astro-ph.GA2021★ 16 cited

Mapping the Galactic centre's dark cluster via Resonant Relaxation

Kerwann Tep, Jean-Baptiste Fouvry, Christophe Pichon +4

Supermassive black holes in the centre of galaxies dominate the gravitational potential of their surrounding stellar clusters. In these dense environments, stars follow nearly Kepl…