The DOI matches its Crossref record; 1 of the 1 references it cites were found in a registry or an index.
Rotating boson stars andQ-balls
Open accessAbstract
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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Citations
Cites
Wald, R. M. (1984) · doi:10.7208/chicago/9780226870373.001.0001 · Cited by 7,188
Cited by
Yunes, N., & Pretorius, F. (2009) · Physical Review D · doi:10.1103/physrevd.80.122003 · Cited by 497
Liebling, S. L., & Palenzuela, C. (2017) · Living Reviews in Relativity · doi:10.1007/s41114-017-0007-y · Cited by 371
Metadata
- Authors
- Kleihaus, B., Kunz, J., & List, M.
- Venue
- Physical Review D
- Publisher
- American Physical Society (APS)
- Published
- 2005-09-09
- Volume
- 72
- Issue
- 6
- ISSN
- 0556-2821 (ISSN-L)
- 1550-7998
- 1550-2368
- OpenAlex
- W2085641369
- Cited by
- 211
- References
- 1
- FWCI
- 1.72
- Type
- journal article
- Language
- en
- Open access
- green
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- Kleihaus, B., Kunz, J., & List, M. (2005). Rotating boson stars andQ-balls. Physical Review D. https://doi.org/10.1103/physrevd.72.064002
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Bibliographic data: Semantic Scholar, OpenAlex, Crossref.
Contains information from the Semantic Scholar Academic Graph Datasets, made available under the ODC Attribution License (ODC-BY 1.0).
Semantic Scholar’s data is described in: Kinney, R., et al. (2023). The Semantic Scholar Open Data Platform. arXiv:2301.10140.
