Yes!
Also, it is not the 'Planck Power' (despite what you might have read in Misner, Thorne and Wheeler, P.980). The existence of black hole horizons implies a maximum luminosity (power) limit in General Relativity. Not even gravitational waves can escape a black hole. Consider
an (almost) black hole made of light (this is called a Kugelblitz) sphere
of radius
\begin{equation}
\notag
R \geq \frac{2Gp}{c^3}
\end{equation} which is filled with photons with a total mass-energy of momentum $p$ times speed of light $c$ \begin{equation}
\notag
E=p \ c
\end{equation} that leave after a time
\notag
R \geq \frac{2Gp}{c^3}
\end{equation} which is filled with photons with a total mass-energy of momentum $p$ times speed of light $c$ \begin{equation}
\notag
E=p \ c
\end{equation} that leave after a time
\begin{equation}
\notag
t=R/c
\end{equation} with average power (luminosity)
\notag
t=R/c
\end{equation} with average power (luminosity)
\begin{equation}
\notag
P = \frac{E}{t}=\frac{p \ c^2}{R}=\frac{c^5}{2G}
\end{equation} This is maximum power in GR, regardless of the nature of the system. You might be tempted to call this half a 'Planck Power' but there is no $\hslash$ in this expression, it is purely classical. This is why you won't see an equation for 'Planck Power' in wiki
\notag
P = \frac{E}{t}=\frac{p \ c^2}{R}=\frac{c^5}{2G}
\end{equation} This is maximum power in GR, regardless of the nature of the system. You might be tempted to call this half a 'Planck Power' but there is no $\hslash$ in this expression, it is purely classical. This is why you won't see an equation for 'Planck Power' in wiki
Source: Cardoso (2018)
OK, so what if there is a maximum power limit in GR? It leads you to think about other possible conjectures, like...maximum tension, acceleration and so on. And in the end, all these roads lead toward contemplating the nature of quantum gravity. Stay tuned!
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