Year: 2025
Type: article
Abstract: We study an overpopulated gas of gravitationally interacting bosons surrounding a droplet of Bose-Einstein condensate---the Bose star. We argue that kinetic evolution of this gas approaches with time a self-similar attractor solution to the kinetic equation. If the scale symmetry of the equation is broken by external conditions, the attractor solution exists, remains approximately self-similar, but has a slowly drifting scaling dimension. The latter new regime of adiabatic self-similarity can determine growth of dark matter Bose stars in cosmological models.
DOI: 10.1103/52sq-jslx
Authors: A. S. Dmitriev, D. G. Levkov, A. G. Panin, I. I. Tkachev
Institutions: Institute for Nuclear Research, Novosibirsk State University
Language: English
Subfield: Astronomy and Astrophysics
Field: Physics and Astronomy
Domain: Physical Sciences
Open Access status: green
Funder: Russian Science Foundation
Award: G7835985756
OpenAlex ID: W4417268241
