Abstract
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.
Original language | English |
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Pages (from-to) | 247-250 |
Number of pages | 4 |
Journal | Physics Letters B |
Volume | 155 |
Issue number | 4 |
DOIs | |
State | Published - 30 May 1985 |
ASJC Scopus subject areas
- Nuclear and High Energy Physics