- needed] a
classical black hole is pure
empty spacetime, and the
simplest (
nonrotating and uncharged) is
characterized just by its m**** and
event horizon.: 37–43 ...
- Teukolsky, Saul A. (1
December 1972). "Rotating
Black Holes:
Locally Nonrotating Frames,
Energy Extraction, and
Scalar Synchrotron Radiation". The Astrophysical...
-
emission rates from a
black hole: M****less
particles from an uncharged,
nonrotating hole".
Physical Review D. 13 (2).
American Physical Society (APS): 198–206...
-
centrifugal potential.
Solving for
geopotential in the
simple case of a
nonrotating sphere, in
units of [m2/s2] or [J/kg]: Ψ ( h ) = ∫ 0 h g d z {\displaystyle...
- An
illustration of the
Schwarzschild metric,
which describes spacetime around a spherical, uncharged, and
nonrotating object with m****...
-
emission rates from a
black hole: M****less
particles from an uncharged,
nonrotating hole".
Physical Review D. 13 (2).
American Physical Society (APS): 198–206...
- that the
exterior solution (i.e. the
spacetime outside of a spherical,
nonrotating,
gravitating body) must be
given by the
Schwarzschild metric. The converse...
-
called the
event horizon and
situated at the
Schwarzschild radius for a
nonrotating black hole,
where the
escape velocity is
equal to the
velocity of light...
-
average density. The
Schwarzschild radius of the
event horizon of a
nonrotating and
uncharged superm****ive
black hole of
around 1 billion M☉ is comparable...
-
occurrences of G and of c drop out. For example, the
Schwarzschild radius of a
nonrotating uncharged black hole with m**** m
becomes r = 2m. For this reason, many...
