Spinning gauged boson stars in anti-de Sitter spacetime
arXiv:1310.5434 · doi:10.1016/j.physletb.2013.11.061
Abstract
We study axially symmetric solutions of the Einstein-Maxwell-Klein-Gordon equations describing spinning gauged boson stars in a 3+1 dimensional asymptotically AdS spacetime. These smooth horizonless solutions possess an electric charge and a magnetic dipole moment, their angular momentum being proportional to the electric charge. A special class of solutions with a self-interacting scalar field, corresponding to static axially symmetric solitons with a nonzero magnetic dipole moment, is also investigated.
15 pages, 4 figures
References in corpus (10)
- Stationary ring solitons in field theory - knots and vortons
- Boson Stars in AdS
- Rotating Boson Stars and Q-Balls II: Negative Parity and Ergoregions
- A Rotating Holographic Superconductor
- Compact (A)dS Boson Stars and Shells
- Electric charge on the brane?
- Extremal Surfaces in Asymptotically AdS Charged Boson Stars Backgrounds
- Numerical Boson Stars with a Single Killing Vector I: the Case
- Charged Boson Stars in AdS and a Zero Temperature Phase Transition
- Charged-spinning-gravitating Q-balls
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- On the Structure of Rotating Charged Boson Stars
- ECO-spotting: looking for extremely compact objects with bosonic fields
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- Gauss-Bonnet Boson Stars with a Single Killing Vector
- Self-interacting boson stars with a single Killing vector field in Anti-de Sitter
- Influence of pressure anisotropy and non-metricity parameter on mass-radius relation and stability of millisecond pulsar in gravity
- Self-interacting multistate boson stars
- Compact stars admitting Finch-Skea symmetry in the presence of various matter fields
- Static black holes with axial symmetry in asymptotically AdS spacetime
- On Q-balls in Anti de Sitter Space