Stationary scalar hairy configurations supported by Neumann compact stars
From MaRDI portal
Publication:2230129
DOI10.1016/J.NUCLPHYSB.2019.114879zbMath1472.85001arXiv1909.13393OpenAlexW2975387494WikidataQ126668533 ScholiaQ126668533MaRDI QIDQ2230129
Publication date: 17 September 2021
Published in: Nuclear Physics. B (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/1909.13393
Cites Work
- Unnamed Item
- Thermodynamics of static dyonic AdS black holes in the \(\omega\)-deformed Kaluza-Klein gauged supergravity theory
- No hair for spherically symmetric neutral reflecting stars: nonminimally coupled massive scalar fields
- On instabilities of scalar hairy regular compact reflecting stars
- Hairy black holes in a box
- Studies of a general flat space/boson star transition model in a box through a language similar to holographic superconductors
- Scalar field configurations supported by charged compact reflecting stars in a curved spacetime
- A general holographic metal/superconductor phase transition model
- Inside black holes with synchronized hair
- Asymptotically flat spinning scalar, Dirac and Proca stars
- No skyrmion hair for stationary spherically symmetric reflecting stars
- The extreme orbital period in scalar hairy Kerr black holes
- Spontaneous scalarization of charged black holes at the approach to extremality
- No hair theorem for bound-state massless static scalar fields outside horizonless Neumann compact stars
- Thermodynamics of five-dimensional static three-charge STU black holes with squashed horizons
- Marginally bound resonances of charged massive scalar fields in the background of a charged reflecting shell
- Charged massive scalar field configurations supported by a spherically symmetric charged reflecting shell
- No nonminimally coupled massless scalar hair for spherically symmetric neutral black holes
- No-bomb theorem for charged Reissner-Nordström black holes
- Stationary scalar configurations around extremal charged black holes
- Event horizon in static scalar-vacuum space-times
- Asymptotically flat black holes with scalar hair: A review
- Kerr black holes with Proca hair
- Shadows of Kerr black holes with and without scalar hair
- Charged black hole bombs in a Minkowski cavity
- The large-mass limit of cloudy black holes
- Construction and physical properties of Kerr black holes with scalar hair
- A no-hair theorem for self-gravitating nonlinear sigma models
- Black Holes Have No Short Hair
- A mass bound for spherically symmetric black hole spacetimes
This page was built for publication: Stationary scalar hairy configurations supported by Neumann compact stars
