Rotating boson stars and Q-balls
By B. Kleihaus, Jutta Kunz, Meike List. 2005
156 citations recorded by the source corpus.
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.
Subfields: Astronomy and Astrophysics, Nuclear and High Energy Physics
View Paper: https://www.semanticscholar.org/paper/56b0d1d17899abd4329b0f7adad91a826eca02ae
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Citations in the corpus
- Numerical methods for finding stationary gravitational solutions (2015, methodology): “Conformal gauge has been used successfully in a number of cases [85–97].”
- Superradiance (2015, background): “the scalar eld [12]. One may regard n= 0 as the fundamental conguration and n1 as excited states. Remarkably, these solutions interpolate between a Kerr BH when qQ=2J= 0 and a rotating boson stars [508,509] when q= 1. The latter are (horizonless) gravitating solitons, that are discussed in Sec.6.8.2”
- Superradiance: Energy Extraction, Black-Hole Bombs and Implications for Astrophysics and Particle Physics (2015, background): “Remarkably, these solutions interpolate between a Kerr BH when q ≡ Q/2J = 0 and a rotating boson stars [504, 505] when q = 1.”
- Stationary ring solitons in field theory - knots and vortons (2008, result): “This behavior is found for allm [102] and it is qualitatively the same as in them = 0 case.”
- Dynamical boson stars (2012, unknown): “Rotating, axisymmetric Q-balls were constructed in [234, 235].”