No response from Clinger then. Quelle Surprise.
Gotta go.
You had no answer for
DeiRenDopa, and I had nothing to add to what he said.
Not at that time, anyway. Now I see you've provided yet more evidence for
DeiRenDopa's thesis:
So don't allow yourself to be distracted by suggestions that you spend years learning differential calculus or that you spend months on the Kerr solution.
FYI: Differential calculus is also called first-semester calculus, or calculus 1. If you had majored in science at a decent university in the United States, you'd have taken it during your first semester---assuming you hadn't already taken it in high school. (In the US,
more students study differential calculus in high school than in college.)
We know of quite a few coordinate transformations that are definitely forbidden by FGR. Can you give an example of a coordinate transformation that is not forbidden by FGR? Even better: Can you describe an objective way for us to determine which coordinate transformations are forbidden, and which are not?
Sure. Remember that light can't go slower than stopped.
I'm glad to see you've changed your mind about Kruskal-Szekeres coordinates, and Eddington-Finkelstein coordinates, and Lemaître coordinates, and Painlevé-Gullstrand coordinates. Light never goes slower than stopped in those coordinates, so now you're saying it's okay to use them in FGR.
Since the FGR oracle has given different answers to that same question on different days, I don't see how your answer could possibly give us an objective way to determine which coordinate transformations are forbidden in FGR.
Clinger, Vorpal, your r=6m noted.
Let's note also that no one knows whether that r=6m calculation can be performed within FGR. My calculation used Painlevé-Gullstrand coordinates, which had definitely not been part of FGR until today.
Vorpal's calculation did not use an explicit coordinate transformation, but he used some GR theory that Einstein derived from principles of covariance that
Farsight had denied in no uncertain terms earlier within this thread.
Before
Farsight changes his mind again tomorrow, let's run through the answer that standard GR gives to
Guybrush Threepwood's question about
what happens to an object that's falling radially into a black hole, starting from rest at infinity.
We'll start by looking at the infalling object's coordinate velocity, as calculated in several different coordinate systems. All of those coordinate systems are okay with
Farsight, according to the rule he gave above. (We have to do this quick, before he comes back tomorrow and changes his mind.)
- In rain coordinates, the object's coordinate velocity is zero throughout the fall.
- In Painlevé-Gullstrand coordinates, the object's coordinate velocity at Schwarzschild r is - β = - 2m/r.
- In Schwarzschild coordinates, outside the event horizon at r=2m, the object's coordinate velocity is - β (1 - β2) (as shown in post #875).
Here's a table of (the absolute values of) those velocities for various values of the Schwarzschild radial coordinate r:
r
............
| 0
....
| β
...........
| β (1 - β
2
)
1000m | 0 | .0447c | .0446c
100m | 0 | .141c | .139c
10m | 0 | .447c | .358c
8m | 0 | .500c | .375c
6m | 0 | .577c | .385c
4m | 0 | .707c | .354c
3m | 0 | .816c | .272c
2m | 0 | 1.000c | 0
1.5m | 0 | 1.155c |
1.0m | 0 | 1.414c |
0.5m | 0 | 2.000c |
0.1m | 0 | 4.472c |
Which of those columns gives the real radially inward velocity of the infalling object?
They all do. This is relativity, so there's more than one way to look at that question.
If you're a passenger on a train, riding along on ribbon rail with all of the windows closed in the cabin, then you may not be aware of any forward movement at all. That's a perfectly legitimate point of view, and it corresponds to the zero column.
If you open a window and calculate your velocity by using your watch to time the interval that passes between mileposts, then you may calculate a nonzero velocity. The β column shows that "milepost" velocity, where I'm assuming mileposts have been planted at fixed values of the Schwarzschild radial coordinate r.
To keep those mileposts planted at fixed values of r, those mileposts have to be accelerated radially outward. Otherwise, they'd fall toward the black hole. For mileposts in the vicinity of the black hole, that acceleration takes a lot of power. For a milepost at the event horizon, it would take infinite power to keep the milepost from falling into the black hole. For mileposts inside the event horizon, it would take
more than infinite power to keep the milepost from falling inward. The supraluminal velocities in the β column therefore correspond to a counterfactual calculation of what the milepost velocity would be if it were possible to maintain mileposts at fixed r even inside the event horizon. That's why you shouldn't get upset by those supraluminal velocities.
The β (1 - β
2) column shows the infalling object's velocity as observed at infinity, or by an observer being held at some fixed r by radially outward acceleration. That as-observed-at-infinity velocity converges to zero at the event horizon, because light emitted by the object at the event horizon can't escape. The observer at infinity will never see the object pass through the event horizon, and will certainly never see the object once it passes inside the event horizon. To the observer at infinity, it looks as though the object starts to slow down inside r=6m, basically because the observed time dilation is increasing faster than the object's momentum is increasing.
The object continues to fall inward, however, passing the event horizon with no great fuss. Pretty soon, within milliseconds or hours (depending on the size of the black hole), the object reaches the black hole's central singularity. General relativity doesn't tell us what happens there. No one knows what happens there.
I'm glad we were able to talk about this today, while
Farsight agrees that all of the coordinate systems mentioned above are allowed by FGR (
Farsight general relativity).
I'm pretty sure he'll deny it tomorrow.