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Proper acceleration of a static Schwarzschild observer
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General relativity
Schwarzschild spacetime
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Words: 26
A static observer at Schwarzschild radius
r
>
2
M
must maintain the outward
proper acceleration
a
=
r
2
1
−
2
M
/
r
M
.
(33)
It approaches the Newtonian value
M
/
r
2
at large radius and diverges at the horizon.
Ancestors
(5)
Schwarzschild spacetime
General relativity
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Physics
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