A perturbative no-hair of form fields for higher dimensional static black holes
arXiv:1101.1121 · doi:10.1103/PhysRevD.83.084016
Abstract
In this paper we examine the static perturbation of p-form field strengths around higher dimensional Schwarzschild spacetimes. As a result, we can see that the static perturbations do not exist when p\geq 3. This result supports the no-hair properties of p-form fields. However, this does not exclude the presence of the black objects having non-spherical topology.
arXiv commentLatex, 9pages, references added
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Cited by in corpus (5)
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- Note on black hole no hair theorems for massive forms and spin-1/2 fields
- Massive spin-2 and spin-1/2 no hair theorems for stationary axisymmetric black holes
- Higher dimensional Robinson-Trautman spacetimes sourced by p-forms: static and radiating black holes
- Black hole solutions of modified gravity theories