Charged exceptional Brans-Dicke wormholes with omega = 0 are stable against radial perturbations; neutral ones are unstable.
Electrically charged and neutral wormhole instability in scalar-tensor gravity
1 Pith paper cite this work. Polarity classification is still indexing.
abstract
We study the stability of static, spherically symmetric, traversable wormholes with or without an electric charge, existing due to conformal continuations in a class of scalar-tensor theories with zero scalar field potential (so that Penney's or Fisher's well-known solutions hold 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 with zero or small electric charge 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 numerical computations.
citation-role summary
citation-polarity summary
fields
gr-qc 1years
2025 1verdicts
CONDITIONAL 1roles
background 1polarities
support 1representative citing papers
citing papers explorer
-
On the stability of exceptional Brans-Dicke wormholes
Charged exceptional Brans-Dicke wormholes with omega = 0 are stable against radial perturbations; neutral ones are unstable.