Condensation and evaporation of boson stars

Abstract Axion-like particles, including the QCD axion, are well-motivated dark matter candidates. Numerical simulations have revealed coherent soliton configurations, also known as boson stars, in the centers of axion halos. We study evolution of axion solitons immersed into a gas of axion waves wi...

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Main Authors: James Hung-Hsu Chan, Sergey Sibiryakov, Wei Xue
Format: Article
Language:English
Published: SpringerOpen 2024-01-01
Series:Journal of High Energy Physics
Subjects:
Online Access:https://doi.org/10.1007/JHEP01(2024)071
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author James Hung-Hsu Chan
Sergey Sibiryakov
Wei Xue
author_facet James Hung-Hsu Chan
Sergey Sibiryakov
Wei Xue
author_sort James Hung-Hsu Chan
collection DOAJ
description Abstract Axion-like particles, including the QCD axion, are well-motivated dark matter candidates. Numerical simulations have revealed coherent soliton configurations, also known as boson stars, in the centers of axion halos. We study evolution of axion solitons immersed into a gas of axion waves with Maxwellian velocity distribution. Combining analytical approach with controlled numerical simulations we find that heavy solitons grow by condensation of axions from the gas, while light solitons evaporate. We deduce the parametric dependence of the soliton growth/evaporation rate and show that it is proportional to the rate of the kinetic relaxation in the gas. The proportionality coefficient is controlled by the product of the soliton radius and the typical gas momentum or, equivalently, the ratio of the gas and soliton virial temperatures. We discuss the asymptotics of the rate when this parameter is large or small.
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spelling doaj.art-0af78711edc44a3781506829a62713e42024-01-21T12:07:44ZengSpringerOpenJournal of High Energy Physics1029-84792024-01-012024114610.1007/JHEP01(2024)071Condensation and evaporation of boson starsJames Hung-Hsu Chan0Sergey Sibiryakov1Wei Xue2Department of Astrophysics, American Museum of Natural HistoryDepartment of Physics & Astronomy, McMaster UniversityDepartment of Physics, University of FloridaAbstract Axion-like particles, including the QCD axion, are well-motivated dark matter candidates. Numerical simulations have revealed coherent soliton configurations, also known as boson stars, in the centers of axion halos. We study evolution of axion solitons immersed into a gas of axion waves with Maxwellian velocity distribution. Combining analytical approach with controlled numerical simulations we find that heavy solitons grow by condensation of axions from the gas, while light solitons evaporate. We deduce the parametric dependence of the soliton growth/evaporation rate and show that it is proportional to the rate of the kinetic relaxation in the gas. The proportionality coefficient is controlled by the product of the soliton radius and the typical gas momentum or, equivalently, the ratio of the gas and soliton virial temperatures. We discuss the asymptotics of the rate when this parameter is large or small.https://doi.org/10.1007/JHEP01(2024)071Axions and ALPsModels for Dark MatterNew Light ParticlesParticle Nature of Dark Matter
spellingShingle James Hung-Hsu Chan
Sergey Sibiryakov
Wei Xue
Condensation and evaporation of boson stars
Journal of High Energy Physics
Axions and ALPs
Models for Dark Matter
New Light Particles
Particle Nature of Dark Matter
title Condensation and evaporation of boson stars
title_full Condensation and evaporation of boson stars
title_fullStr Condensation and evaporation of boson stars
title_full_unstemmed Condensation and evaporation of boson stars
title_short Condensation and evaporation of boson stars
title_sort condensation and evaporation of boson stars
topic Axions and ALPs
Models for Dark Matter
New Light Particles
Particle Nature of Dark Matter
url https://doi.org/10.1007/JHEP01(2024)071
work_keys_str_mv AT jameshunghsuchan condensationandevaporationofbosonstars
AT sergeysibiryakov condensationandevaporationofbosonstars
AT weixue condensationandevaporationofbosonstars