Abstract
The chapter briefly reviews the properties of static, spherically symmetric configurations of general relativity with a minimally coupled scalar field \(\phi \) whose kinetic energy is negative in a restricted (strong-field) region of space and positive outside it. This “trapped ghost” concept may in principle explain why no ghosts are observed under usual, weak-field conditions. The configurations considered are wormholes and regular black holes without a center, in particular, black universes (black holes with an expanding cosmology beyond the event horizon). Spherically symmetric perturbations of these objects are considered, and it is stressed that, due to the universal shape of the effective potential near a transition surface from canonical to phantom behavior of the scalar field, such surfaces restrict the possible perturbations and play a stabilizing role.
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Notes
- 1.
Our conventions are: the metric signature \((+\ -\ -\ -)\), the curvature tensor \(R^{\sigma }{}_{\mu \rho \nu } = \partial _\nu \varGamma ^{\sigma }_{\mu \rho }-\ldots ,\ R_{\mu \nu }= R^{\sigma }{}_{\mu \sigma \nu }\), so that the Ricci scalar \(R > 0\) for de Sitter spacetime and the matter-dominated cosmological epoch; the sign of \(T_\mu ^\nu \) such that \(T^0_0\) is the energy density, and the system of units \(8\pi G = c = 1\).
- 2.
In what follows we will use different radial coordinates, to be denoted by different letters:
u — a general notation,
x — quasiglobal, such that \(\alpha = -\gamma \),
y — harmonic, such that \(\alpha = 2\beta + \gamma \),
z — “tortoise,” such that \(\alpha = \gamma \).
- 3.
For a detailed description of the properties of Fisher and anti-Fisher solutions see [8, 13, 38, 39] and references therein. Let us here only mention that the metric (7.14) describes wormholes [5, 6] if \(k < 0\), which is only possible with negative h; one flat spatial infinity then corresponds to \(y=0\), the other one to \(y = \pi /|k|\).
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Acknowledgements
This work was supported in part by the Russian Foundation for Basic Research grant 16-02-00602.
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Bronnikov, K.A. (2017). Trapped Ghosts as Sources for Wormholes and Regular Black Holes. The Stability Problem. In: Lobo, F. (eds) Wormholes, Warp Drives and Energy Conditions. Fundamental Theories of Physics, vol 189. Springer, Cham. https://doi.org/10.1007/978-3-319-55182-1_7
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