Wavy strings: Black or bright?
Dec, 199645 pages
Published in:
- Phys.Rev.D 55 (1997) 7625-7644
e-Print:
- hep-th/9612248 [hep-th]
Report number:
- MCGILL-96-44,
- WATPHYS-TH-96-17
Citations per year
Abstract:
Recent developments in string theory have brought forth a considerable interest in time-dependent hair on extended objects. This novel new hair is typically characterized by a wave profile along the horizon and angular momentum quantum numbers in the transverse space. In this work, we present an extensive treatment of such oscillating black objects, focusing on their geometric properties. We first give a theorem of purely geometric nature, stating that such wavy hair cannot be detected by any scalar invariant built out of the curvature and/or matter fields. However, we show that the tidal forces detected by an infalling observer diverge at the `horizon' of a black string superposed with a vibration in any mode with . The same argument applied to longitudinal () waves detects only finite tidal forces. We also provide an example with a manifestly smooth metric, proving that at least a certain class of these longitudinal waves have regular horizons.- 04.70.Dy
- 04.50.+h
- 11.25.Mj
- gravitation: action
- field theory: scalar
- astrophysics: string
- black hole
- field equations: solution
- bibliography
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