Publications


PhD: Secular evolution of self-gravitating systems over cosmic age

HDR: Stellar Dynamics in Galactic Nuclei

Refereed Publications: ADS

[42] Kinetic Theory of Stellar Systems: A Tutorial
        Hamilton, C., Fouvry, J.-B., Phys. Plasmas, submitted

[41] Non-resonant relaxation of rotating globular clusters
        Tep, K., Fouvry, J.-B., Pichon, C., A&A, submitted

[40] Dynamical large deviations for long-range interacting inhomogeneous systems without collective effects
        Feliachi, O., Fouvry, J.-B., Phys. Rev. E, submitted

[39] Predicting the linear response of self-gravitating stellar spheres and discs with LinearResponse.jl
        Petersen, M., Roule, M., Fouvry, J.-B., Pichon, C., Tep, K., 2024, MNRAS, in press

[38] Kinetic blockings in long-range interacting systems
        Fouvry, J.-B., Roule, M., 2023, Phys. Rev. E, 108, 054108

[37] Constraining intermediate-mass black holes from the stellar disc of SgrA*
        Fouvry, J.-B., Bustamante-Rosell, M. J., Zimmerman, A., 2023, MNRAS, 526, 1471

[36] Milankovitch equations with spinors
        Deme, B., Fouvry, J.-B., 2023, Celest. Mech. Dyn. Astron., 135, 47

[35] Astrophysics with the Laser Interferometer Space Antenna
        Lisa collaboration including Fouvry, J.-B., 2023, Living Rev. Relativ., 26, 2

[34] Kinetic theory of one-dimensional inhomogeneous long-range interacting N-body systems at order 1/N^2 without collective effects
        Fouvry, J.-B., 2022, Phys. Rev. E, 106, 054123

[33] Long-term relaxation of 1D self-gravitating systems
        Roule, M., Fouvry, J.-B., Pichon, C., Chavanis, P.-H., 2022, Phys. Rev. E, 106, 044118

[32] Orbital alignment and mass segregation in galactic nuclei via vector resonant relaxation
        Magnan, N., Fouvry, J.-B., Pichon, C., Chavanis, P.-H., 2022, MNRAS, 514, 3452

[31] Non-resonant relaxation of anisotropic globular clusters
        Tep, K., Fouvry, J.-B., Pichon, C., 2022, MNRAS, 514, 875

[30] Linear response theory and damped modes of stellar clusters
        Fouvry, J.-B., Prunet, S., 2022, MNRAS, 509, 2443

[29] Secular Dynamics around a Supermassive Black Hole via Multipole Expansion
        Fouvry, J.-B., Dehnen, W., Tremaine, S., Bar-Or, B., 2022, ApJ, 931, 8

[28] Mapping the Galactic centre's dark cluster via Resonant Relaxation
        Tep, K., Fouvry, J.-B., Pichon, C., Heissel, G., Paumard, T., Perrin, G., Vincent, F., 2021, MNRAS, 506, 4289

[27] Resonant and non-resonant relaxation of globular clusters
        Fouvry, J.-B., Hamilton, C., Rozier, S., Pichon, C., 2021, MNRAS, 508, 2210

[26] Relaxation in a Fuzzy Dark Matter Halo. II. Self-consistent kinetic equations
        Bar-Or, B., Fouvry, J.-B., Tremaine, S., 2021, ApJ, 915, 27

[25] Kinetic theory of one-dimensional homogeneous long-range interacting systems with an arbitrary potential of interaction
        Fouvry, J.-B., Chavanis, P.-H., Pichon, C., 2020, Phys. Rev. E, 102, 052110

[24] Young stellar cluster dilution near supermassive black holes: the impact of Vector Resonant Relaxation on neighbour separation
        Giral Martìnez, J., Fouvry, J.-B., Pichon, C., 2020, MNRAS, 499, 2714

[23] The Strength of the Dynamical Spiral Perturbation in the Galactic Disk
        Eilers, A.-C., Hogg, D., Rix, H.-W., Frankel, N., Hunt, J., Fouvry, J.-B., Buck, T., 2020, ApJ, 900, 186

[22] Kinetic theory of 1D homogeneous long-range interacting systems sourced by 1/N^2 effects
        Fouvry, J.-B., Bar-Or, B., Chavanis, P.-H., 2019, Phys. Rev. E, 100, 052142

[21] Vector Resonant Relaxation of Stars around a Massive Black Hole
        Fouvry, J.-B., Bar-Or, B., Chavanis, P.-H., 2019, ApJ, 883, 161

[20] Mapping the stability of stellar rotating spheres via linear response theory
        Rozier, S., Fouvry, J.-B., Breen, P. G., Varri, A. L., Pichon, C., Heggie, D. C., 2019, MNRAS, 487, 711

[19] Instabilities in disc galaxies: from noise to grooves to spirals
        De Rijcke, S., Fouvry, J.-B., Pichon, C., 2019, MNRAS, 484, 3198

[18] Secular dynamics of long-range interacting particles on a sphere in the axisymmetric limit
        Fouvry, J.-B., Bar-Or, B., Chavanis, P.-H., 2019, Phys. Rev. E, 99, 032101

[17] How gravitational softening affects galaxy stability. I. Linear mode analysis of disc galaxies
        De Rijcke, S., Fouvry, J.-B., Dehnen, W., 2019, MNRAS, 485, 150

[16] Relaxation in a Fuzzy Dark Matter Halo
        Bar-Or, B., Fouvry, J.-B., Tremaine, S., 2019, ApJ, 871, 28

[15] Relaxation in self-gravitating systems
        Fouvry, J.-B., Bar-Or, B., 2018, MNRAS, 481, 4566

[14] Revisiting relaxation in globular clusters
        Hamilton, C., Fouvry, J.-B., Binney, J., Pichon, C., 2018, MNRAS, 481, 2041

[13] Scalar Resonant Relaxation of Stars around a Massive Black Hole
        Bar-Or, B., Fouvry, J.-B., 2018, ApJ, 860, 23

[12] The secular evolution of discrete quasi-Keplerian systems. II. Application to a multi-mass axisymmetric disc around a supermassive black hole
        Fouvry, J.-B., Pichon, C., Chavanis, P.-H., 2017, A&A, 609, A38

[11] Distribution functions for resonantly trapped orbits in the Galactic Disc
        Monari, G., Famaey, B., Fouvry, J.-B., Binney, J., 2017, MNRAS, 471, 4314

[10] Resonant thickening of self-gravitating discs: imposed or self-induced orbital diffusion in the tightly wound limit
        Fouvry, J.-B., Pichon, C., Chavanis, P.-H., Monk, L., 2017, MNRAS, 471, 2642

[9] Dressed diffusion and friction coefficients in inhomogeneous multi-component self-gravitating systems
        Heyvaerts, J., Fouvry, J.-B., Chavanis, P.-H., Pichon, C., 2017, MNRAS, 469, 4193

[8] The secular evolution of discrete quasi-Keplerian systems. I. Kinetic theory of stellar clusters near black holes
        Fouvry, J.-B., Pichon, C., Magorrian, J., 2016, A&A, 598, A71

[7] Functional integral derivation of the kinetic equation of two-dimensional point vortices
        Fouvry, J.-B., Chavanis, P.-H., Pichon, C., 2016, Physics Letters A, 380, 2589

[6] Functional integral approach to the kinetic theory of inhomogeneous systems
        Fouvry, J.-B., Chavanis, P.-H., Pichon, C., 2016, Physica A, 459, 117

[5] Secular diffusion in discrete self-gravitating tepid discs. II. Accounting for swing amplification via the matrix method
        Fouvry, J.-B., Pichon, C., Magorrian, J., Chavanis, P.-H., 2015, A&A, 584, A129

[4] Secular diffusion in discrete self-gravitating tepid discs. I. Analytic solution in the tightly wound limit
        Fouvry, J.-B., Pichon, C., Chavanis, P.-H., 2015, A&A, 581, A139

[3] Self-gravity, Resonances, and Orbital Diffusion in Stellar Disks
        Fouvry, J.-B., Binney, J., Pichon, C., 2015, ApJ, 806, 117

[2] Secular resonant dressed orbital diffusion - II. Application to an isolated self-similar tepid galactic disc
        Fouvry, J.-B., Pichon, C., 2015, MNRAS, 449, 1982

[1] Secular resonant dressed orbital diffusion - I. Method and WKB limit for tepid discs
        Fouvry, J.-B., Pichon, C., Prunet, S., 2015, MNRAS, 449, 1967