0 Members and 1 Guest are viewing this topic.
maybe the new BH wont spin as much?
Quote from: CZARCAR on 15/11/2011 11:53:30maybe the new BH wont spin as much? angular momentum will be preserved - it was this problem with rotation that stopped me venturing an opinion on this question
I believe that they won't collide because of their gravitational interaction which causes them to orbit about a common center of mass.
Quote from: Daylights on 19/11/2011 16:04:50 I believe that they won't collide because of their gravitational interaction which causes them to orbit about a common center of mass.I suspect you are right. Unless the BHs are on a perfect collision path, or one is much smaller than the other, they will probably go into orbit.
Quote from: Geezer on 19/11/2011 20:56:59Quote from: Daylights on 19/11/2011 16:04:50 I believe that they won't collide because of their gravitational interaction which causes them to orbit about a common center of mass.I suspect you are right. Unless the BHs are on a perfect collision path, or one is much smaller than the other, they will probably go into orbit.I think someone else has pointed out elsewhere that orbits are tricky-business. That essentially for two objects that aren't locked in orbit to become locked in orbit, it requires a third object which can absorb kinetic energy of the system. And, with black holes, this might mean either a very large star, or a third black hole.One can still imagine many interesting scenarios happening as two equal sized black holes approached each other. When considering two distant black holes, the center of mass in the 2-body system would be outside of their event horizons. For distance objects, that might not mean much, but it could be a problem as they approached.What if they approached so that the event horizons merged, but still distant enough that the center of the black holes remained outside of the other's event horizon?What if they approached on a tangent so that the center of each black hole just skimmed the other's event horizon, yet carrying with it an extraordinary amount of kinetic energy which one would anticipate could take them out of orbital range.