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2004/09/10 | Kerr-Newman黑洞[Kerr-Newman Black Hole]
类别(Ω〖物理〗)
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发表于 13:32
A rotating charged
black hole
. An exact, unique, and complete solution to the
Einstein field equations
in the exterior of such a black hole was found by Newman
et al
. (1965), although its connection to black holes was not realized until later (Shapiro and Teukolsky 1983, p. 338). In the coordinates of Boyer and Lindquist (1967), the exterior metric for a black hole with mass
M
, angular momentum
J
, and charge
Q
has the form
(1)
where
(2)
(3)
(4)
The corresponding
electromagnetic field tensor
, written as a two-form, is given by
(5)
(Misner
et al
. 1973, p. 877).
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