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arxiv: gr-qc/0505143 · v1 · submitted 2005-05-29 · 🌀 gr-qc

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Rotating Boson Stars and Q-Balls

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classification 🌀 gr-qc
keywords bosonstarsq-ballscouplingdetermineflatfrequencylimit
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We consider axially symmetric, rotating boson stars. Their flat space limits represent spinning Q-balls. We discuss their properties and determine their domain of existence. Q-balls and boson stars are stationary solutions and exist only in a limited frequency range. The coupling to gravity gives rise to a spiral-like frequency dependence of the boson stars. We address the flat space limit and the limit of strong gravitational coupling. For comparison we also determine the properties of spherically symmetric Q-balls and boson stars.

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Cited by 1 Pith paper

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  1. Bayesian Analysis of Massive Boson Star Models for Sagittarius A* Using Near-Infrared Astrometry Data

    astro-ph.HE 2026-05 unverdicted novelty 4.0

    Bayesian analysis shows current near-IR astrometry data cannot distinguish massive boson stars from Schwarzschild black holes for Sgr A*.