Self-similar growth of Bose stars

Fuente: arXiv
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Autori principali: Dmitriev, A. S., Levkov, D. G., Panin, A. G., Tkachev, I. I.
Natura: Preprint
Pubblicazione: 2023
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author Dmitriev, A. S.
Levkov, D. G.
Panin, A. G.
Tkachev, I. I.
author_facet Dmitriev, A. S.
Levkov, D. G.
Panin, A. G.
Tkachev, I. I.
contents We analytically solve the problem of Bose star growth in the bath of gravitationally interacting particles. We find that after nucleation of this object the bath is described by a self-similar solution of kinetic equation. Together with the conservation laws, this fixes mass evolution of the Bose star. Our theory explains, in particular, the slowdown of the star growth at a certain "core-halo" mass, but also predicts formation of heavier and lighter objects in magistral dark matter models. The developed "adiabatic" approach to self-similarity may be of interest for kinetic theory in general.
format Preprint
id arxiv_https___arxiv_org_abs_2305_01005
institution arXiv
publishDate 2023
record_format arxiv
spellingShingle Self-similar growth of Bose stars
Dmitriev, A. S.
Levkov, D. G.
Panin, A. G.
Tkachev, I. I.
Cosmology and Nongalactic Astrophysics
Astrophysics of Galaxies
Statistical Mechanics
High Energy Physics - Phenomenology
We analytically solve the problem of Bose star growth in the bath of gravitationally interacting particles. We find that after nucleation of this object the bath is described by a self-similar solution of kinetic equation. Together with the conservation laws, this fixes mass evolution of the Bose star. Our theory explains, in particular, the slowdown of the star growth at a certain "core-halo" mass, but also predicts formation of heavier and lighter objects in magistral dark matter models. The developed "adiabatic" approach to self-similarity may be of interest for kinetic theory in general.
title Self-similar growth of Bose stars
topic Cosmology and Nongalactic Astrophysics
Astrophysics of Galaxies
Statistical Mechanics
High Energy Physics - Phenomenology
url https://arxiv.org/abs/2305.01005