Conformal continuations and wormhole instability in scalar-tensor gravity
arXiv:gr-qc/0411063
Abstract
We study the stability of static, spherically symmetric, traversable wormholes existing due to conformal continuations in a class of scalar-tensor theories with zero scalar field potential (so that Fisher's well-known scalar-vacuum solution holds in the Einstein conformal frame). Specific examples of such wormholes are those with nonminimally (e.g., conformally) coupled scalar fields. All boundary conditions for scalar and metric perturbations are taken into account. All such wormholes are shown to be unstable under spherically symmetric perturbations. The instability is proved analytically with the aid of the theory of self-adjoint operators in Hilbert space and is confirmed by a numerical computation.
8 two-column pages, latex, gc style
Cited by in corpus (16)
- Instability of wormholes supported by a ghost scalar field. I. Linear stability analysis
- Wormholes without exotic matter in Einstein-Cartan theory
- Thin-shell wormholes in dilaton gravity
- Scalar fields as sources for wormholes and regular black holes
- Wormhole geometries in Eddington-inspired Born-Infeld gravity
- Self-stabilization of extra dimensions
- Echoes of Compact Objects in Scalar-Tensor Theories of Gravity
- Traversable wormholes in beyond Horndeski theories
- Wormhole Structures in Logarithmic-Corrected Gravity
- Magnetic wormholes and black universes with invisible ghosts
- Constraining modified gravity theories with scalar fields using black-hole images
- Thin-shell wormholes constrained by cosmological observations
- Formation of Bound States of scalar fields in AdS-asymptotic Wormholes
- Electrically charged and neutral wormhole instability in scalar-tensor gravity
- On the stability of spherically symmetric space-times in scalar-tensor gravity
- Damour-Solodukhin Wormhole as a Black Hole Mimicker: The Role of Observers' Location