Consequences of Overlapping Event Horizons in Supermassive Black Hole Mergers

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When two supermassive black holes pass closely enough for their event horizons to overlap, they begin a merger process, resulting in a single larger event horizon that encompasses the mass of both. The overlapping event horizons create a region where matter and energy are affected, but once the horizons no longer overlap, they are effectively contained within the new, larger horizon. The distinction between merging and being wrapped in a larger horizon is largely semantic, as both scenarios lead to the same outcome. Event horizons are not expansive; they are relatively small compared to the mass they contain, meaning that any matter approaching too closely will inevitably be consumed. Ultimately, the dynamics of black hole mergers highlight the complexities of describing such phenomena using natural language.
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What happens if two supermassive black holes pass each other so close that their event horizons briefly overlap each others? What will happen with matter and energy that is present in the overlapped region when the event horizons no longer overlap?
 
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If they get that close, they will merge. There are numerous threads on this forum that discuss that. I suggest a forum search.
 
I always thought that two event horizons cannot rally cross and black holes don't merge, but get wrapped in a bigger horizon that encloses them both
 
Andrea Panza said:
black holes don't merge, but get wrapped in a bigger horizon that encloses them both

It's a matter of taste whether you say that they "merge" or "get wrapped in a bigger horizon". Either way, you end up with one larger event horizon that encloses all the mass previously contained in the two; the distinction is mostly due to the ambiguity that crops any time we use natural language to describe a physical phenomenon best described mathematically.
 
By the time two black holes approach near enough for their event horizons [EH] to overlap, a merger has already begun. It's not like an event horizon extends outwards for light years. For example Sag A, the supermassive black hole in the Milky Way center has a mass of around 4 million suns, but an EH only about the size of Mercury's orbit. Remember the EH is where escape velocity = c. So obviously nothing can approach that closely and avoid being eaten, regardless of its mass or velocity.
 
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