A no-go theorem for scalar fields with couplings from Ginzburg-Landau models
arXiv:2204.03833 · doi:10.1140/epjc/s10052-022-10497-5
Abstract
Recently Hod proved a no-go theorem that static scalar fields cannot form spherically symmetric boson stars in the asymptotically flat background. On the other side, scalar fields can be coupled to the gradient according to next-to-leading order Ginzburg-Landau models. In the present work, we extend Hod's discussions by considering couplings between static scalar fields and the field gradient. For a non-negative coupling parameter, we show that there is no asymptotically flat spherically symmetric boson stars made of coupled static scalar fields.
arXiv comment6 pages
References in corpus (46)
- TOPICAL REVIEW: General relativistic boson stars
- Shadows of Kerr black holes with scalar hair
- Kerr-Newman scalar clouds
- Stationary resonances of rapidly-rotating Kerr black holes
- Thermodynamics and phase transitions in the Born-Infeld-anti-de Sitter black holes
- Hairy Black Holes and Null Circular Geodesics
- Black holes have no short hair
- Boson stars with negative cosmological constant
- Non-linear Q-clouds around Kerr black holes
- Stationary scalar configurations around extremal charged black holes
- The superradiant instability regime of the spinning Kerr black hole
- Inside black holes with synchronized hair
- Extended Ginzburg-Landau formalism: systematic expansion in small deviation from the critical temperature
- Chaotic dynamics of strings in charged black hole backgrounds
- Scalar field configurations supported by charged compact reflecting stars in a curved spacetime
- Thermodynamics and Phase Transition of a Nonlinear Electrodynamics Black Hole in a Cavity
- No-scalar-hair theorem for spherically symmetric reflecting stars
- Classical Yang-Mills black hole hair in anti-de Sitter space
- Charged massive scalar field configurations supported by a spherically symmetric charged reflecting shell
- No-hair theorems for a static and stationary reflecting star
- Charged reflecting stars supporting charged massive scalar field configurations
- Synchronous frequencies of extremal Kerr black holes: resonances, scattering and stability
- Conductivity of higher dimensional holographic superconductors with nonlinear electrodynamics
- No nonminimally coupled massless scalar hair for spherically symmetric neutral reflecting stars
- Marginally bound resonances of charged massive scalar fields in the background of a charged reflecting shell
- On instabilities of scalar hairy regular compact reflecting stars
- Static scalar field condensation in regular asymptotically AdS reflecting star backgrounds
- Skyrmions, Skyrme stars and black holes with Skyrme hair in five spacetime dimension
- Hair mass bound in the black hole with nonzero cosmological constants
- Uniqueness of higher-dimensional phantom field wormholes
- Scalar field condensation behaviors around reflecting shells in Anti-de Sitter spacetimes
- Hair distributions in noncommutative Einstein-Born-Infeld black holes
- Scalar condensation behaviors around regular Neuman reflecting stars
- Hair formation in the background of noncommutative reflecting stars
- Ultra-compact spherically symmetric dark matter charged star objects
- An analytic effective model for hairy black holes
- No-go theorem for static boson stars
- Upper bound on the radii of regular ultra-compact star photonspheres
- No hair theorem for spherically symmetric regular compact stars with Dirichlet boundary conditions
- Large regular reflecting stars have no scalar field hair
- Holographic DC SQUID in the presence of dark matter
- No-go theorem for static boson stars with negative cosmological constants
- No scalar hair theorem for neutral Neumann stars: static massive scalar fields nonminimally coupled to gravity
- The absence of superconductivity in the next-to-leading order Ginzburg-Landau functional for Bardeen-Cooper-Schrieffer superconductor
- No-go theorem for spatially regular boson stars made of static nonminimally coupled massive scalar fields
- No scalar condensations outside reflecting stars with coupling terms from Ginzburg-Landau models