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  Are values above c^5/4G or c^4/4G or c^3/4G observed in black hole mergers?

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Some people conjecture that the emitted power of a system is always below $c^5/4G$, the maximum force of attraction (in any frame of reference) always below $c^4/4G$, and the maximum mass flow rate (in any frame of reference) always below $c^3/4G$.

Is this the case in all the observed black hole mergers?

asked Jun 10, 2017 in Theoretical Physics by Jules [ no revision ]

1 Answer

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Partial answer. It seems that one or two solar masses were radiated away in 0.1 seconds. That is more than a factor 1000 away from the limit value.

answered Jun 10, 2017 by anonymous [ no revision ]

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