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arxiv: 1101.1121 · v3 · pith:DNHPFJRVnew · submitted 2011-01-06 · 🌀 gr-qc · hep-th

A perturbative no-hair of form fields for higher dimensional static black holes

classification 🌀 gr-qc hep-th
keywords staticblackdimensionalfieldshigherno-hairp-formresult
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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.

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