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Slowly rotating Q-balls
Abstract
Q-balls are non-topological solitons arising in scalar field theories. Solutions for rotating Q-balls (and the related boson stars) have been shown to exist when the angular momentum is equal to an integer multiple of the Q-ball charge Q . Here we consider the possibility of classically long-lived metastable rotating Q-balls with small angular momentum, even for large charge, for all scalar theories that support non-rotating Q-balls. This is relevant for rotating extensions of Q-balls and related solitons such as boson stars as it impacts their cosmological phenomenology. arXiv:2302.11589
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Cited by 8
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Metadata
- Authors
- Almumin, Y., Heeck, J., Rajaraman, A., & Verhaaren, C. B.
- Venue
- The European Physical Journal C
- Published
- 2024-04-07
- Volume
- 84
- Issue
- 4
- ISSN
- 1434-6052
- Cited by
- 8
- Language
- en
- Funders
- National Science Foundation (PHY-2210428, PHY-1915005, PHY-2210067)
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- Almumin, Y., Heeck, J., Rajaraman, A., & Verhaaren, C. B. (2024). Slowly rotating Q-balls. The European Physical Journal C. https://doi.org/10.1140/epjc/s10052-024-12712-x