No-go theorem for static boson stars
arXiv:1902.05230 · doi:10.1016/j.physletb.2018.01.036
Abstract
It is proved that self-gravitating static scalar fields whose self-interaction potential is a monotonically increasing function of its argument cannot form spherically symmetric asymptotically flat bound matter configurations. Our compact theorem rules out, in particular, the existence of spatially regular static boson stars made of nonlinear massive scalar fields.
arXiv comment8 pages
References in corpus (37)
- Kerr black holes with scalar hair
- TOPICAL REVIEW: General relativistic boson stars
- Shadows of Kerr black holes with scalar hair
- Kerr black holes with Proca hair
- Stationary Scalar Clouds Around Rotating Black Holes
- No hair for spherical black holes: charged and nonminimally coupled scalar field with self--interaction
- Kerr-Newman scalar clouds
- Stationary resonances of rapidly-rotating Kerr black holes
- Kerr-Newman black holes with stationary charged scalar clouds
- Kerr black holes with self-interacting scalar hair: hairier but not heavier
- On the instability regime of the rotating Kerr spacetime to massive scalar perturbations
- Asymptotically flat scalar, Dirac and Proca stars: discrete vs. continuous families of solutions
- Hairy Black Holes and Null Circular Geodesics
- A new spin on black hole hair
- Analytic treatment of the black-hole bomb
- Non-linear Q-clouds around Kerr black holes
- Scalar hairy black holes and solitons in asymptotically flat spacetimes
- Upper bound on the radii of black-hole photonspheres
- Scalarized Hairy Black Holes
- Myers-Perry black holes with scalar hair and a mass gap
- The large-mass limit of cloudy black holes
- Extremal Kerr-Newman black holes with extremely short charged scalar hair
- The superradiant instability regime of the spinning Kerr black hole
- Inside black holes with synchronized hair
- Rotating black holes can have short bristles
- The fastest way to circle a black hole
- Myers-Perry black holes with scalar hair and a mass gap: unequal spins
- How fast can a black hole rotate?
- Spinning boson stars and Kerr black holes with scalar hair: the effect of self-interactions
- A Mass Bound for Spherically Symmetric Black Hole Spacetimes
- Wiggly tails: a gravitational wave signature of massive fields around black holes
- A no-short scalar hair theorem for rotating Kerr black holes
- Self-gravitating field configurations: The role of the energy-momentum trace
- No nonminimally coupled massless scalar hair for spherically symmetric neutral black holes
- Effect of scalar field mass on gravitating charged scalar solitons and black holes in a cavity
- No-go theorem for static scalar field dark matter halos with no Noether charges
- AdS solitons with conformal scalar hair
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- Dynamical Boson Stars
- Selected topics in scalar-tensor theories and beyond
- Kerr black holes with synchronised scalar hair and boson stars in the Einstein-Friedberg-Lee-Sirlin model
- On Derrick's theorem in curved spacetime
- Horndeski stars
- No scalar hair theorem for neutral Neumann stars: static massive scalar fields nonminimally coupled to gravity
- No-go theorem for static boson stars with negative cosmological constants
- No-go theorem for spatially regular boson stars made of static nonminimally coupled massive scalar fields
- Compact stars in Einstein-scalar-Gauss-Bonnet gravity: regular and divergent scalar field configurations
- A no-go theorem for scalar fields with couplings from Ginzburg-Landau models
- Light Rings, Accretion Disks and Shadows of Hayward Boson Stars