2inquisitive
07-31-07, 12:47 AM
This thread is a sidetrack from zanket's thread: (Alpha) General relativity is self-inconsistent v3 - Pete
zanket,
The OP does not say that the rod was gravitationally accelerating toward the horizon. The only information given about the rod’s motion is that the part of it that is above the horizon is escaping to r=infinity.
Seems James R already addressed this point. Your OP stated "Let a freely falling rod span the horizon of a black hole..." Yes, a 'freely falling rod' is gravitationally accelerating toward the event horizon whether you use those exact words or not, explained earlier. Next, you state "Let the part of the rod above the horizon be excaping to r=infinity". That part of the rod is accelerating in the opposite direction as the 'freely falling' lower part.
Not all of the supporting info in the other thread applies to this thread. The thought experiment in this thread does not rely on SR.
Of course the thought experiment in this thread relies on SR's flat spacetime inertial frames. Your whole gedanken is a challenge to Minkowski flat spacetime and Schwarzchild black holes. Those are both Special Theory formulations, not General Relativity's curved spacetime. GR's curved spacetime was what led to Kerr black holes, the ones we have observational evidence for in the universe. No evidence for Schwarzchild black holes has ever been found, meaning that no black holes have been found that are definitely not rotating. Of course, the properties of all black holes have not been measured to determine if they are rotating or not, just that the ones we were capabale of measuring have a flat accretion disk rotating at very near the speed of light at the event horizon. How could that rotation suddenly cease at the point immediately below the event horizon?
Your references to tidal forces are both based on Schwarzchild formulations which predict a central singularity. They are assuming tidal forces decrease in intensity at an inverse cube ratio radially from that point singularity. Again, that is SR mathematics, not GR's curved spacetime. There is no point singularity in GR's Kerr black holes, but a ring-shaped singularity that lies inside the event horizon. Tidal forces in Kerr black holes are immense near the event horizon because of the proximity of the ring singularity to the event horizon. Tidal forces, however, can be weak in the center of a very large Kerr black hole, a GR black hole.
zanket,
The OP does not say that the rod was gravitationally accelerating toward the horizon. The only information given about the rod’s motion is that the part of it that is above the horizon is escaping to r=infinity.
Seems James R already addressed this point. Your OP stated "Let a freely falling rod span the horizon of a black hole..." Yes, a 'freely falling rod' is gravitationally accelerating toward the event horizon whether you use those exact words or not, explained earlier. Next, you state "Let the part of the rod above the horizon be excaping to r=infinity". That part of the rod is accelerating in the opposite direction as the 'freely falling' lower part.
Not all of the supporting info in the other thread applies to this thread. The thought experiment in this thread does not rely on SR.
Of course the thought experiment in this thread relies on SR's flat spacetime inertial frames. Your whole gedanken is a challenge to Minkowski flat spacetime and Schwarzchild black holes. Those are both Special Theory formulations, not General Relativity's curved spacetime. GR's curved spacetime was what led to Kerr black holes, the ones we have observational evidence for in the universe. No evidence for Schwarzchild black holes has ever been found, meaning that no black holes have been found that are definitely not rotating. Of course, the properties of all black holes have not been measured to determine if they are rotating or not, just that the ones we were capabale of measuring have a flat accretion disk rotating at very near the speed of light at the event horizon. How could that rotation suddenly cease at the point immediately below the event horizon?
Your references to tidal forces are both based on Schwarzchild formulations which predict a central singularity. They are assuming tidal forces decrease in intensity at an inverse cube ratio radially from that point singularity. Again, that is SR mathematics, not GR's curved spacetime. There is no point singularity in GR's Kerr black holes, but a ring-shaped singularity that lies inside the event horizon. Tidal forces in Kerr black holes are immense near the event horizon because of the proximity of the ring singularity to the event horizon. Tidal forces, however, can be weak in the center of a very large Kerr black hole, a GR black hole.