Axisymmetric Black Hole Has Only Two Degrees of Freedom
B. CarterInstitute of Theoretical Astronomy, University of Cambridge, Cambridge CB3 0EZ, England
1971en
ABI
Аннотация
A theorem is described which establishes the claim that in a certain canonical sense the Kerr metrics represent "the" (rather than merely "some possible") exterior fields of black holes with the corresponding mass and angular-momentum values.
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