A fixed-proper-length pendulum in Schwarzschild spacetime has small-oscillation period T = 4π r2^2/(c r_s) sqrt(N2(N1-N2)), recovering the Newtonian limit and giving a distinct near-horizon scaling.
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A Simple Pendulum in Schwarzschild Spacetime
A fixed-proper-length pendulum in Schwarzschild spacetime has small-oscillation period T = 4π r2^2/(c r_s) sqrt(N2(N1-N2)), recovering the Newtonian limit and giving a distinct near-horizon scaling.