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Physics, Astronomy & Cosmology / Re: What Is The Final Parsec Problem ?
« on: 06/01/2025 18:47:47 »When galaxies collide, their central supermassive black holes (SMBHs) should also eventually merge.The quote you give kind of says it. To get closer, their kinetic energy must go somewhere, else, like Earth, it just keeps orbiting the sun without getting closer.
However, as the SMBHs approach each other within about a parsec (3.26 light-years), the density of stars and gas in the galactic core becomes too low to effectively remove the energy and momentum needed for the final plunge and merger.
This "energy loss problem" prevents the black holes from spiraling inward and merging within a reasonable timeframe.
So how do Black Holes merge then ?
Thing is, the way this energy is dissipated is by flinging other matter away, giving that matter the orbital energy of the pair. Once the material is all gone, only new (not orbiting) material can contribute further to this process, and that takes a lot of time.
They will eventually merge, just all all planets will eventually fall into the sun given enough time and no external dissturbance. Any pair of orbiting objects emits gravitational waves and that energy comes from kinetic energy.. Earth for instance emits GWs at the rate of about 200 watts, and the kinetic energy of Earth will run a pair of 100W light bulbs for an awfully long time. The sun will swallow Earth before that has time to happen, but that's the fate of say Jupiter.
Likewise, all black hole binaries like the undoctored picture you took will eventually merge, but the universe is only 14 billion years old, nowhere near long enough for gravitational waves to do the job at a full parsec away.
Fun fact: Two sheep circling each other will emit Baaavitational waves.
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