Black holes as windows to extra dimensions

Physics

Scientific paper

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Scientific paper

We derive the static three-dimensional spherically symmetric solution of the Einstein equations in an empty five-dimensional universe, and analyse the effective four-dimensional perspective. The radius of the compact fifth dimension is regarded as a local quantity. Our main conclusion is that the extra dimension becomes visible, and the associated Kaluza-Klein gauge interaction singular, when approaching the modified Schwarzschild horizon. The possibility of ``massless'' black holes is noted.

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