I am the first in the world

When I lower you all the way to the event horizon, you see the whole evolution of the universe happening in an instant.

Note that Sol said "an observer FALLING through the event horizon". An observer hanging on a rope is under acceleration, in a distinctly non-inertial reference frame, and he knows it. Any observer under this amount of acceleration will expect this type of time distortion---whether they're being accelerated by a rocket, or by a rope holding them just above a black hole.

The distortion is not something special that happens at event horizons.
 
sol invictus said:
But for someone falling through the horizon, at least for a large black hole where tidal forces are small, nothing even slightly unusual happens.
I know that's what they say, but all processes slow and stop on the horizon as viewed from outside.
And that's not at all contradictory.

So imagine I'm lowering you down on a gedanken rope. I lower you down a little, and we compare notes through the comms line wrapped around the rope. ...
Then Sol is held up by the tension of the rope, and so is in an accelerated frame. Even in STR, acceleration gives a one-way horizon attempting to cross which will rip you apart. (Appropriately, near the horizon of a large Schwarzschild black hole locally looks exactly like an acceleration horizon of STR.)

When I lower you all the way to the event horizon, you see the whole evolution of the universe happening in an instant.
If Sol has an idealized body that's both pointlike and lightlike, maybe. Being a static observer the event horizon is a mathematical impossibility. For any remotely realistic body, the tidal forces in this frame will rip him up long before that. But if he's falling inwards instead, then (relative to the stationary frame) he'll be approaching lightspeed near the horizon, so you can think of this as Lorentz contraction keeping the tidal forces on his body finite and small.

Sorry, I didn't look at it. The thing is, mathematics doesn't get this crucial point across. That's why people blithely switch to a different metric I suppose, and do that hop skip and a jump over the end of time without even noticing.
Ok, how about just taking the Schwarzschild geometry in different coordinates?
[latex]\[ds^2 = -dt^2 + \left(dr+\sqrt{\frac{2m}{r}}dt\right)^2 + r^2\left(d\theta^2 + \sin^2\theta d\phi^2\right)\][/latex]
There's indeed an absolute event horizon. No, time doesn't stop there in that frame.

And when all processes slow and stop, you can't measure anything.
You're taking a statement that's true in a particular reference frame and treating as if it was absolute. It isn't. This is the same kind of mistake commonly made in STR, just in a different context.
 
I know that's what they say, but all processes slow and stop on the horizon as viewed from outside.

So?

So imagine I'm lowering you down on a gedanken rope. I lower you down a little, and we compare notes through the comms line wrapped around the rope. We note that initially you experience fairly modest gravitational time dilation. Your parallel-mirror light clock doesn't keep pace with mine, a pulsar a few light years away appears to have speeded up, my voice sounds like Pinky and Perky. I lower you further and the gravitational time dilation becomes so dramatic that a minute of your time is an hour of mine. When I lower you to the very near the event horizon you see suns forming flaring and dying in what seems to be minutes, and galaxies racing across the sky then growing dim. When I lower you all the way to the event horizon, you see the whole evolution of the universe happening in an instant.

That's inaccurate for a number of reasons. But in any case, it is not relevant to what you would see if you fell freely through - as ben and Vorpal point out, you're describing an accelerated observer.

Sorry, I didn't look at it. The thing is, mathematics doesn't get this crucial point across. That's why people blithely switch to a different metric I suppose, and do that hop skip and a jump over the end of time without even noticing.

How do you think we know that time slows down at the horizon as viewed by an external observer, Farsight? It's certainly not from observations - it's what the math tells us. And exactly the same math tells us that observers falling through notice nothing unusual. So on what basis do you accept one conclusion and reject the other?
 
So all processes slow and stop on the horizon. Everything is stopped. Light has stopped. Light isn't moving, it isn't going down any more, so neither are you.

That's inaccurate for a number of reasons. But in any case, it is not relevant to what you would see if you fell freely through - as ben and Vorpal point out, you're describing an accelerated observer.
It doesn't make any difference. Whether you're hanging on a rope or not, the light in your light clock isn't moving. It isn't moving between the mirrors, and it isn't moving downwards either.

How do you think we know that time slows down at the horizon as viewed by an external observer, Farsight? It's certainly not from observations - it's what the math tells us.
The maths tells you that gravitational time dilation occurs, and that maths is backed up by experiment and observation. We allow for it in the GPS clock adjustment. But what the maths doesn't tell you that it isn't time that slows down, it's motion. Including the motion of light in your light clock that you use to determine the thing you call time t.

And exactly the same math tells us that observers falling through notice nothing unusual.
It isn't exactly the same maths. It's further maths that ignores the fact that both you and your clock are both stopped, and blunders on as if nothing unusual happens to conjure up a hop skip and a jump over the end of time. See the Schwarzschild chart on the left here. Look carefully at that conveniently truncated peak. Also see the wiki article which refers to the "coordinate artifact", and note this:

"In 1939 Howard Robertson showed that a free falling observer descending in the Scwharzschild metric would cross the r = rs singularity in a finite amount of proper time even though this would take an infinite amount of time in terms of coordinate time t."

So on what basis do you accept one conclusion and reject the other?
Look a bit further down on the wiki article. See the bit that says:

"However due to the obscurity of the journals in which the papers of Lemaître and Synge were published their conclusions went unnoticed, with many of the major players in the field including Einstein believing that singularity at the Schwarzschild radius was physical."

As ever, I'm with Einstein. My interpretation of general relativity adheres to the original. The "modern interpretation" that you, Vorpal, and benm have been taught, doesn't. There's no other way to say this: in certain important respects, it's wrong. And so relativity remains the Cinderella of modern physics.
 
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It isn't exactly the same maths. It's further maths that ignores the fact that both you and your clock are both stopped, and blunders on as if nothing unusual happens to conjure up a hop skip and a jump over the end of time.

You're directly contradicting every textbook on general relativity. This is a skeptic's forum, so you must provide evidence for such a radical claim. Show us which step in the math is incorrect.

I'll help you start. The defining principle of general relativity is the principle of equivalence, which states that observers in freely falling observatories cannot detect the presence of gravitational fields except through tidal effects. Hence, to show that "nothing unusual happens to a freely falling observer" it's necessary and sufficient to show that tidal forces are weak at the horizon of a large black hole. That's rather trivial to do with modern techniques - but you claim it's wrong, so find the mistake.

As ever, I'm with Einstein. My interpretation of general relativity adheres to the original. The "modern interpretation" that you, Vorpal, and benm have been taught, doesn't. There's no other way to say this: in certain important respects, it's wrong. And so relativity remains the Cinderella of modern physics.

Einstein didn't understand the Schwarzschild solution, that's true. Neither did anyone else until the 50s.
 
Note that Sol said "an observer FALLING through the event horizon". An observer hanging on a rope is under acceleration, in a distinctly non-inertial reference frame, and he knows it. Any observer under this amount of acceleration will expect this type of time distortion---whether they're being accelerated by a rocket, or by a rope holding them just above a black hole. The distortion is not something special that happens at event horizons.
It doesn't matter ben. A reference frame isn't something that actually exists, it's isn't something that you're actually "in". It's just something we use to describe the uniformity or not of our measurements of space and time, sometimes when in motion, sometimes when not. We do these measurement using the motion of light, and at the event horizon the coordinate speed of light is zero.

Remember what I said about the coordinate speed of light being the actual speed of light? The cordinate speed of light varies in a non-inertial reference frame, such as the room you're in. We now have super-accurate optical clocks that lose synchronisation when separated by only a foot of vertical elevation. You can simplify them to parallel-mirror light clocks, whereupon you can work out that this is what's happening:

|-------------|
|-------------|

Now imagine the lower clock is at the event horizon. This is what's happening:

|-------------|
|-------------|

At the event horizon it isn't nothing unusual happens, it's nothing happens. There are no more events. The light isn't moving any more. You can't measure space, you can't measure time, you can't see, or think, and your reference frame and coordinate system have utterly collapsed.

Think it through.

Vorpal: sorry, I have to go.
 
You're directly contradicting every textbook on general relativity. This is a skeptic's forum, so you must provide evidence for such a radical claim. Show us which step in the math is incorrect.
No. I've already told you twice that the maths doesn't show you this. I've given you a good explanation, now deal with the argument instead of trying to play the inscrutable mathematics card.

Einstein didn't understand the Schwarzschild solution, that's true. Neither did anyone else until the 50s.
Einstein thought the singularity at the Schwarzschild radius was physical. I'm with Einstein. You're not, and you're attempting to pooh-pooh Einstein by saying he didn't understand it? Come on sol, you can do better than that. Think this thing through.

Now I really must go. Again, apologies Vorpal.
 
No. I've already told you twice that the maths doesn't show you this. I've given you a good explanation, now deal with the argument instead of trying to play the inscrutable mathematics card.

Now you're claiming "the maths doesn't show you this"? So are you saying I'm lying? Are you also denying that this is what all the textbooks say? Do you think they're lying too? If so, you're either delusional or ignorant and extraordinarily arrogant. If not, you think the math in those textbooks is wrong. So, tell us what's wrong with it. If you can't, why should anyone pay any attention to you?

As for your "explanation", no one disputes that time slows down at the horizon as viewed by an external observer. Time also slows down for a moving object as viewed by a stationary observer. Does this mean that something changes in the rest frame of the object? Nope - and the same goes at the horizon.

Einstein thought the singularity at the Schwarzschild radius was physical. I'm with Einstein. You're not, and you're attempting to pooh-pooh Einstein by saying he didn't understand it? Come on sol, you can do better than that. Think this thing through.

I don't know for sure what Einstein thought, and you're obviously not a reliable source. My understanding is that he thought the Schw. solution was simply unphysical. And yes - he was wrong.
 
We do these measurement using the motion of light, and at the event horizon the coordinate speed of light is zero.

The coordinate speed of light according to whom, Farsight? You can't throw three different observers into a problem---observers who, remember, will disagree on that speed---and declare that the speed "actually" has some special value.

At the event horizon it isn't nothing unusual happens, it's nothing happens. There are no more events. The light isn't moving any more. You can't measure space, you can't measure time, you can't see, or think, and your reference frame and coordinate system have utterly collapsed.

For any observer accelerating very strongly, your reference frame and coordinate system have "collapsed". That's true if you are accelerating in flat space (and picking up speed w/r/t reference objects). It's also accelerating near a black hole (and hovering just above the event horizon).

For an inertial observer, your local space is approximately flat, your local light speed is c, Newton's Laws hold, etc.. That's true if you are drifting in (globally) flat space, it's true if you are falling inertially and just outside an event horizon, it's true if you are falling inertially and just inside the event horizon.

Your idea that "your coordinate system does something special at the horizon" is flatly wrong. It's not subtly wrong, it's straightforwardly wrong; and it's been derived explicitly in many places that you have access to; you have found no error in the derivations, you apparently just don't like the answer because your hobby-horse suggested a different one.
 
The maths tells you that gravitational time dilation occurs, and that maths is backed up by experiment and observation. We allow for it in the GPS clock adjustment. But what the maths doesn't tell you that it isn't time that slows down, it's motion. Including the motion of light in your light clock that you use to determine the thing you call time t.
But t isn't the thing I would call time if I was either suspended over a black hole or falling toward in. Actually, no one could naturally call the Schwarzschild t coordinate time except a stationary observer at infinity.

Say I'm in completely ordinary Minkowski spacetime and I have a big rocket tuned to always give me a constant acceleration a in some particular direction. Around me are a bunch of people in astronaut suits. What would I see? I'd see them going toward a horizon away from me, slowdown, get redshifted, with their images hovering above just above it, with the redshift factor diverging to infinity. What would I observe if I tied a rope around one, preventing them from going away from me? I'd observe that the closer they are to the horizon, the more tension is in the rope, with the required force also diverging.

This is basic STR requiring absolutely nothing of GTR. And it works out very analogously. What's important to note here is that despite all my observations of them slowing down or redshifting, the people go on their merry away. Because as far they are concerned, there's no special surface where I see them slowing down. Time goes on--for them.

In Schwarzschild spacetime is that though stationary observers are accelerated, stationary observer at infinity becomes inertial. That's possible because of spacetime curvature.

"In 1939 Howard Robertson showed that a free falling observer descending in the Scwharzschild metric would cross the r = rs singularity in a finite amount of proper time even though this would take an infinite amount of time in terms of coordinate time t."
For those interested in a little historical diversion, as far as I'm aware of the first to seriously consider that "collapse goes on" in the formation of a black hole (rather than a "God-given" Schwarzschild geometry) were Oppenheimer and Snyder, also in 1939,
Phys. Rev. 56, 455–459 (1939)
immediately following the Oppenheimer-Volkoff result about neutron degeneracy pressure being unable to stop black hole formation.

As ever, I'm with Einstein. My interpretation of general relativity adheres to the original. The "modern interpretation" that you, Vorpal, and benm have been taught, doesn't. There's no other way to say this: in certain important respects, it's wrong. And so relativity remains the Cinderella of modern physics.
It's the same theory. The mathematics for studying its implications have greatly evolved (compared to today, differential geometry was barely in infacy when Einstein used to formulate GTR).

No. I've already told you twice that the maths doesn't show you this. I've given you a good explanation, now deal with the argument instead of trying to play the inscrutable mathematics card.
It's not inscrutable mathematics. It's basic calculus. Take Einstein's original paper for GTR, which tells you how to calculate geodesics, and the Schwarzschild metric. The radial freefall of an observer is very simple, and it doesn't stop at the horizon. (There's a neat little coincidence that's interesting in itself: for Schwarzschild r-coordinate vs proper time of an radially freefalling observer, the relationship between them is exactly the same as that of radius vs time in Newtonian gravity.)

Most of the other claims in this thread are only marginally more complicated to derive. There's no curvature singularity at the horizon. There's no reason for the manifold to be cut off there.

Einstein thought the singularity at the Schwarzschild radius was physical. I'm with Einstein.
And he was wrong. So what? Einstein made some mistakes, though even your own source (for whatever wiki's worth) even implied he wasn't even aware of Lemaître and Robertson's work.

Your argument is a bit like saying that kinetic energy being relevant to collisions is a nonsensical "modern interpretation" of Newtonian physics because Newton himself thought it was crap.
 
The Information and the Universe

Conclusions:

In my view Susskind’s first mistake: he is talking about bits of information, but today information is measured in qubits.
I do not agree with Susskind-Hawking: the information is located on the ‘area’ of the universe. In my view the information of a system depends of the energy of the system, we need energy to change the state of the qubit.
Susskind is talking about Hawking’s thought experiment; there is one bit per Planck area. This is wrong because inside a Planck volume the Planck energy EP = 1.9561 × 10^9 J.
Today there is more information inside the universe then on the edge of the universe.
The photons from the edge of the universe can not record all the changing information from the whole Universe. All the qubits like photons, electrons, atoms…are generating a lot of information.
Information is lost in the quantum system trough interaction with an observer.
The information within the quantum states cannot entirely be retained once the system has collapsed from a superposition of states into a specific state. That lost information can never be retained, as opposed to classical theory where information transformations can be reversed to obtain a history of the previous states of the system. That’s why in my view Susskind, Hawking, Gerard 't Hooft…theory is wrong.
When a measurement of any type is made to a quantum system, decoherence breaks down and the wave function collapses into a single state.
Susskind is talking about the information from a book; to have a correct discussion we can not mixed bits with qubits, to describe a system we have to stay at the quantum level.
I calculated precisely the lower bound , the lowest number of qubits after the Big Bang:
min Iuniverse = 15.392 × 10^61 qubits.

http://adrianferent.blogspot.com/
 
In my view Susskind’s first mistake: he is talking about bits of information, but today information is measured in qubits.
...
In my view your first mistake: You seem ignorant of the actual topic of this thread.
The topic is what happens to bits of information as they fall into a black hole. Stephen Hawkings asked this at a conference in 1981 and seemed to show that they were lost. The consensus today is that they are not.

Your ignorance also leads you to think that the topic involves the universe, not black holes.
 
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Okay....about not seeing something fall into the black hole.

Spaceship B is watching Spaceship A fall into the black hole. From what I'm reading here Spaceship B will never really see Spaceship A disappear into it.

What if Spaceship B then leaves, the crew is put into cryostasis and a million years later it returns to the same viewing point. Would it still see Spaceship A down there on the edge of the event horizon?
 
Okay....about not seeing something fall into the black hole.

Spaceship B is watching Spaceship A fall into the black hole. From what I'm reading here Spaceship B will never really see Spaceship A disappear into it.

What if Spaceship B then leaves, the crew is put into cryostasis and a million years later it returns to the same viewing point. Would it still see Spaceship A down there on the edge of the event horizon?

It's a good question. The truth is, the whole "never see anything fall into a black hole" statement is rather misleading. What you'd really see as you watch the ship approach the horizon (I'm going to assume this is a black hole in otherwise empty space) is that the light emitted by the ship's windows gets more and more shifted towards the red end of the spectrum, and at the same time fainter and fainter. If it was falling straight in, after a short time you'd cease to see it at all as the light went infra-red and very faint.

If you then did a very, very, very precise measurement with the right instruments, you'd detect an extremely faint spectrum of thermal (at a very cold temperature) radiation emitted almost uniformly by the horizon of the black hole (that's the famous Hawking radiation). The ship falling in would affect that radiation, but the effects dissipate extremely quickly - they decrease exponentially with a time constant set by the light-crossing time of the hole. For a hole with the mass of the sun, that means after a small fraction of a second the effects of the ship falling in would be totally undetectable.

So no - you wouldn't see it there.
 
Okay....about not seeing something fall into the black hole. Spaceship B is watching Spaceship A fall into the black hole. From what I'm reading here Spaceship B will never really see Spaceship A disappear into it. What if Spaceship B then leaves, the crew is put into cryostasis and a million years later it returns to the same viewing point. Would it still see Spaceship A down there on the edge of the event horizon?
Not practically, they won't be actually able to see it because the light can't escape. But that's where it will be. See post #25 above. A free falling observer would cross the r = rs singularity in a "finite amount of proper time", but this takes infinite coordinate time. So he never actually crosses the event horizon. Not in a million years. Not in a billion years. Not ever.
 
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And that's not at all contradictory.
No, it isn't contradictory, it's crystal clear. All processes slow and stop on the horizon as viewed from outside. So a parallel-mirror light clock stops. And light stops. It stops moving back and forth between the mirrors. It stops moving, full stop. So it isn't moving down any more.

Then Sol is held up by the tension of the rope, and so is in an accelerated frame. Even in STR, acceleration gives a one-way horizon attempting to cross which will rip you apart. (Appropriately, near the horizon of a large Schwarzschild black hole locally looks exactly like an acceleration horizon of STR.)
It doesn't matter. Make it a supermassive black hole so you don't have to worry about the tidal gradient. And take note: this is a place where light has stopped. The coordinate speed of light is zero. Aim a photon at the black hole and it doesn't get blue-shifted to some infinite frequency as it crosses th event horizon. Instead, it stops.

If Sol has an idealized body that's both pointlike and lightlike, maybe. Being a static observer the event horizon is a mathematical impossibility. For any remotely realistic body, the tidal forces in this frame will rip him up long before that. But if he's falling inwards instead, then (relative to the stationary frame) he'll be approaching lightspeed near the horizon, so you can think of this as Lorentz contraction keeping the tidal forces on his body finite and small.
And what's lightspeed at the horizon? Remember what i said about the coordinate speed of light above. It's zero.

Ok, how about just taking the Schwarzschild geometry in different coordinates?
[latex]\[ds^2 = -dt^2 + \left(dr+\sqrt{\frac{2m}{r}}dt\right)^2 + r^2\left(d\theta^2 + \sin^2\theta d\phi^2\right)\][/latex]
There's indeed an absolute event horizon. No, time doesn't stop there in that frame.
There is no time in that frame. In that frame, you're keeping time on a stopped clock. And you're stopped too. The two don't cancel each other out so that "you don't notice anything unusual". Everything has ground to a halt, light doesn't move, nor do nerve impulses in your head, so you don't notice anything.

You're taking a statement that's true in a particular reference frame and treating as if it was absolute. It isn't. This is the same kind of mistake commonly made in STR, just in a different context.
I'm not making a mistake here Vorpal. In the STR scenario, it's like you travelling at the speed of light. We all know you can't actually do this, but think it through. If you were travelliung at c, you'd be totally time-dilated, you don't notice anything any more. You might imagine that "in your frame" everything is carrying on as normal, but it isn't. And in the real world, everybody sheds a tear, because poor old Vorpal is out there in space frozen and insensible, forever.
 
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Re: #36, but highly relevant to #37.
That doesn't make sense even in STR, Farsight. Take the Rindler chart of Minkowski spacetime, with the coordinate time corresponding to a uniformly accelerated observer seeing inertial (freefalling) objects. The observations made in this frame are in a fair analogy to what a stationary observer in Schwarzschild spacetime would: the slowing, the redshift, the non-crossing, even the thermal radiation. And yet the obviously objects cross the horizon in their own frames.

Proper time is what an actual infalling clock would directly measure. I don't know why you discount it as unreal. If anything, it has far more fundamental than any coordinate because it's completely observer-independent. You're making an huge conceptual mistake.
 
I'm not making a mistake here Vorpal. In the STR scenario, it's like you travelling at the speed of light. We all know you can't actually do this, but think it through. If you were travelliung at c, you'd be totally time-dilated, you don't notice anything any more. You might imagine that "in your frame" everything is carrying on as normal, but it isn't. And in the real world, everybody sheds a tear, because poor old Vorpal is out there in space frozen and insensible, forever.
You write as if there are two worlds: the traveller's and the real world. As I understand it, they are both equally real. The traveller would see our world recede at the speed of light, and for him, our time will stop.
 
Farsight, understanding just a little about the metric in post #17 - which is the Rindler chart of Minkowski spacetime that Vorpal just mentioned - would probably help you realize your mistake. That metric has a horizon that is exactly like the horizon of a large black hole. Time stops at that horizon in exactly the same way, the redshift goes to infinity in the same way, you'd have to accelerate to keep from falling in, etc.

And yet, the horizon of that metric is unquestionably a coordinate artifact - I can choose a different set of coordinates on the same spacetime such that any point I like is on the horizon. So the assertion that objects never "actually" cross such horizons is not even logically self-consistent - it's just wrong.
 
Now you're claiming "the maths doesn't show you this"? So are you saying I'm lying?
No, I'm saying you don't understand this.

Are you also denying that this is what all the textbooks say? Do you think they're lying too? If so, you're either delusional or ignorant and extraordinarily arrogant.
Don't thump your "good book" at me, sol. Deal with the argument and the logic.

If not, you think the math in those textbooks is wrong. So, tell us what's wrong with it. If you can't, why should anyone pay any attention to you?
I've told you before, don't try hiding behind the maths, not with me. Look at this expression:

[latex]t_0 = t_f \sqrt{1 - \frac{2GM}{rc^2}} = t_f \sqrt{1 - \frac{r_0}{r}}[/latex]

t0 is the proper time between events A and B for a slow-ticking observer within the gravitational field,
tf is the coordinate time between events A and B for a fast-ticking observer at an arbitrarily large distance from the massive object...
r is the radial coordinate of the observer...
r0 is the Schwarzschild radius...


It's a simple expression, and it tells you that when r is very very large, when you're a long way from the black hole, t0 tends to tf. It's the infalling observer's clock rate expressed as a fraction of the distant observer's clock rate. I'm the distant observer, you're the other guy. As you fall, when you run the numbers for ever-smaller values of r expressed as a multiple of r0, you can see the way t0 trends.

When r is 4, t0 = .866
When r is 3, t0 = .816
When r is 2, t0 = .707
When r is 1.5, t0 = .577
When r is 1.1, t0 = .301
When r is 1.01, t0 = .099
When r is 1.00, t0 = 0

At the event horizon, your clock rate, expressed as a fraction of mine, is zero. Like you said, all processes slow and stop on the horizon as viewed from outside. And your light clock is a parallel-mirror light clock, remember. With a clock rate of zero. I'll wait a million years. Has your clock ticked yet? No. I'll wait a billion years? Has your clock ticked yet? No.

Has the penny dropped yet?

As for your "explanation", no one disputes that time slows down at the horizon as viewed by an external observer. Time also slows down for a moving object as viewed by a stationary observer. Does this mean that something changes in the rest frame of the object? Nope - and the same goes at the horizon.
Are you being deliberately obtuse? Read post #25 again, and this time pay attention: what the maths doesn't tell you that it isn't time that slows down, it's motion. Including the motion of light in your light clock that you use to determine the thing you call time t. You've got a clock rate of zero. See what I told Vorpal. You're like the gedanken observer travelling at c. You observe nothing.

I don't know for sure what Einstein thought, and you're obviously not a reliable source. My understanding is that he thought the Schw. solution was simply unphysical. And yes - he was wrong.
You know how you get all those cranks and crackpots who know b*ggar all physics and who insist that Einstein was wrong? Well, take a look at which side of the fence you're on.
 
I've told you before, don't try hiding behind the maths, not with me. Look at this expression:

[latex]t_0 = t_f \sqrt{1 - \frac{2GM}{rc^2}} = t_f \sqrt{1 - \frac{r_0}{r}}[/latex]

Farsight, please write down the tension in the rope holding this observer in place. Got it? Good. Reexpress the above, not in terms of r but in terms of tension. Got it?

Farsight, please forget about the black hole; consider this same rope, under the same tension, towing this observer through flat space. Find the equivalent expression for this observer. (You'll want to compare his clock that of an inertial observe with respect to whom he is momentarily at rest.) Got it?
 
The coordinate speed of light according to whom, Farsight? You can't throw three different observers into a problem---observers who, remember, will disagree on that speed---and declare that the speed "actually" has some special value.
According to distant observers. People who aren't falling into the black hole. Even if their measurements don't quite agree they can account for that from their knowledge of relativity - the coordinate speed of light is only constant in an inertial reference frame. In a non-inertial reference frame, such as the room you're in, it isn't constant. They can all see the black hole and the infalling observer, any differences in their measurements are miniscule and well-understood.

For any observer accelerating very strongly, your reference frame and coordinate system have "collapsed". That's true if you are accelerating in flat space (and picking up speed w/r/t reference objects). It's also accelerating near a black hole (and hovering just above the event horizon).
It isn't "collapsed", it's non-inertial.

For an inertial observer, your local space is approximately flat, your local light speed is c, Newton's Laws hold, etc.. That's true if you are drifting in (globally) flat space, it's true if you are falling inertially and just outside an event horizon..
Your local light speed is your measured speed of light. You always measure wave speed to be the same value because of the wave nature of matter. Remember pair production, and how you can create and electron (and a positron) from light? And how you can diffract electrons? And neutrons? And have you read what I've said about how the NIST caesium fountain clock works? In a nutshell, you calibrate your rods and clocks using the local motion of electromagnetic phenomena. Light in the wider sense. Then you use them to measure the local speed of light. That's why you always measure the same value. I'm not kidding you about this ben.

it's true if you are falling inertially and just inside the event horizon.
It isn't. Remember what sol said: all processes slow and stop on the horizon as viewed from outside. Now imagine that you're a light wave bouncing back and forth inside his parallel-mirror light clock. At the event horizon, you stop forever.

Your idea that "your coordinate system does something special at the horizon" is flatly wrong.
This isn't my idea, this is the original frozen star idea, in line with Schwarzschild and Einstein. Typical textbooks do that hop skip and a jump over the Schwarzschild event-horizon singularity and write it off as a coordinate artefact, missing the whole point that when light stops you don't have any coordinates any more. Again, see what I said to Vorpal. It's the GR equivalent of the SR case where you're travelling through flat space at c. You don't carry on observing as if nothing happened. You observe nothing.

It's not subtly wrong, it's straightforwardly wrong; and it's been derived explicitly in many places that you have access to; you have found no error in the derivations, you apparently just don't like the answer because your hobby-horse suggested a different one.
If it's "straightforwardly wrong", try explaining it. Or try addressing my straightforward argument. When you can't do either, stop digging, and yield.
 
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I've told you before, don't try hiding behind the maths, not with me. Look at this expression:

[latex]t_0 = t_f \sqrt{1 - \frac{2GM}{rc^2}} = t_f \sqrt{1 - \frac{r_0}{r}}[/latex]

t0 is the proper time between events A and B for a slow-ticking observer within the gravitational field,
tf is the coordinate time between events A and B for a fast-ticking observer at an arbitrarily large distance from the massive object...
r is the radial coordinate of the observer...
r0 is the Schwarzschild radius...


It's a simple expression, and it tells you that when r is very very large, when you're a long way from the black hole, t0 tends to tf. It's the infalling observer's clock rate expressed as a fraction of the distant observer's clock rate.
Oh, Farsight. I'm afraid that's completely wrong. The infalling observer's clock rate expressed as a fraction of the distant stationary observer's clock rate is:
[latex]\[ \frac{d\tau}{dt} = \sqrt{\left(1-\frac{r_0}{r}\right)-\left(1-\frac{r_0}{r}\right)^{-1}\frac{dr^2}{dt^2} - r^2\left(\frac{d\theta^2}{dt^2}+\sin^2\theta\frac{d\phi^2}{dt^2}\right)} \][/latex]
Now, if I take a stationary observer, dr = dθ = dφ = 0, sure enough, that's [latex]$ d\tau = dt\sqrt{1-\frac{r_0}{r}}$[/latex]. But not an infalling observer.

What did you think the Schwarzschild metric was for, anyway? Window dressing?

There is actually something almost right about your post, but I'm afraid that if I tell you, you'll simply latch on to that and learn nothing, because your conceptual problems are quite deep. Let me instead ask you about how much you know of Einstein's work.
1) Are you aware of the geodesic equation and Christoffel symbols? They're featured quite prominently in Einstein's papers on GTR. I know--I read them.
2) Are you capable of calculating an orbit using them? Even a simple radial one, dθ = dφ = 0?

You know how you get all those cranks and crackpots who know b*ggar all physics and who insist that Einstein was wrong? Well, take a look at which side of the fence you're on.
You've not understood Einstein at all. You're just cherry-picking specific cases with no understanding of the bigger picture. Yes, the bigger picture Einstein himself explained.
 
Farsight, please write down the tension in the rope holding this observer in place. Got it? Good. Reexpress the above, not in terms of r but in terms of tension. Got it? Farsight, please forget about the black hole; consider this same rope, under the same tension, towing this observer through flat space. Find the equivalent expression for this observer. (You'll want to compare his clock that of an inertial observe with respect to whom he is momentarily at rest.) Got it?
No. It isn't relevant. The coordinate speed of light varies with gravitational potential. The tension in the rope is merely an indicator of the difference in gravitational potential between the bottom and the top. Whether the observer at the event horizon has fallen, or has been gently lowered on a gedanken rope doesn't make any difference. Either way, he is at a place where the coordinate speed of light is zero. Please don't clutch at straws to cling to something that you've been taught. Think for yourself instead.

Gotta go. You know guys, I enjoy talking to you.
 
No. It isn't relevant. The coordinate speed of light varies with gravitational potential.

The coordinate speed of light is a weird, non-localized quantity that you cook up by comparing two particular observers. Yes, it does weird and divergent things. Many observer-observer comparisons do similarly weird things. You are pointing out one specific weirdness that occurs when you compare an observer in flat space to an observer hanging on a rope under diverging tension. Why should anyone care? "The coordinate speed of light varies with potential" is no more interesting a statement than "the tension on the rope varies with potential".

Whether the observer at the event horizon has fallen, or has been gently lowered on a gedanken rope doesn't make any different

Sure it does. A falling observer is in a different reference frame than the rope-hanging observer. You keep constructing "coordinate time" using the rope-hanging observer's clock, NOT the falling clock, so you do not have the luxury of saying "the rope makes not difference". It does make a difference---it imparts an acceleration, and acceleration affects clocks, and you're trying to prove everyone wrong by arguing about clocks. Under the circumstances, you do NOT have the luxury of ignoring differences between clocks.
 
No, I'm saying you don't understand this.

Me, and every other physicist since the 1960s? Ooookaaay.... <backs away slowly>

I've told you before, don't try hiding behind the maths, not with me. Look at this expression:

[latex]t_0 = t_f \sqrt{1 - \frac{2GM}{rc^2}} = t_f \sqrt{1 - \frac{r_0}{r}}[/latex]

t0 is the proper time between events A and B for a slow-ticking observer within the gravitational field,
tf is the coordinate time between events A and B for a fast-ticking observer at an arbitrarily large distance from the massive object...
r is the radial coordinate of the observer...
r0 is the Schwarzschild radius...


It's a simple expression, and it tells you that when r is very very large, when you're a long way from the black hole, t0 tends to tf. It's the infalling observer's clock rate expressed as a fraction of the distant observer's clock rate. I'm the distant observer, you're the other guy. As you fall, when you run the numbers for ever-smaller values of r expressed as a multiple of r0, you can see the way t0 trends.

When r is 4, t0 = .866
When r is 3, t0 = .816
When r is 2, t0 = .707
When r is 1.5, t0 = .577
When r is 1.1, t0 = .301
When r is 1.01, t0 = .099
When r is 1.00, t0 = 0

At the event horizon, your clock rate, expressed as a fraction of mine, is zero. Like you said, all processes slow and stop on the horizon as viewed from outside. And your light clock is a parallel-mirror light clock, remember. With a clock rate of zero. I'll wait a million years. Has your clock ticked yet? No. I'll wait a billion years? Has your clock ticked yet? No.

Has the penny dropped yet?

Your math (or rather, your interpretation of it) is wrong. But never mind that, because there's a very simple argument that doesn't even involve doing any math. Look at the metric in post #17. It's exactly the same as the near-horizon metric of a black hole. But it's also a metric on flat spacetime, and I can put the horizon anywhere I want in flat spacetime. Therefore, any conclusion that the horizon must be special because of some feature in that metric is manifestly, unambiguously wrong.

You know how you get all those cranks and crackpots who know b*ggar all physics and who insist that Einstein was wrong? Well, take a look at which side of the fence you're on.

That's the classic "appeal to authority" logical fallacy. Just because Einstein said something - and so far, you haven't even presented a quote from him, and I don't take your word for it - doesn't make it true. Since Einstein was an expert on this topic it certainly makes it worth considering, and it means that establishing it as incorrect requires careful argument and the agreement of other experts. But that's been done, over and over and over again. This analysis is in every textbook on relativity. I've derived it myself. Vorpal has derived it. ben has derived it. In fact, the only one in this conversation that can't do the math and hasn't derived it is - you guessed it - you.
 
Has the penny dropped yet?

Here's the other thing, Farsight. You seem to think that you're presenting us stuff we've never through about before. You're expecting people to say "Holy cow---you're right! His clock hasn't budged! I never looked at it that way, that changes everything!

This is comically wrong.

This is where it becomes obvious that you've never taken a GR course or paged through a GR textbook. No, Farsight, none of your statements (the ones that are correct, anyway) are even the slightest bit surprising. You see, this is what learning GR consists of. You take a bunch of spacetimes, and a bunch of metrics, and you do dozens of exercises working through different scenarios. Your conclusion---minus the "OMG this changes everything" wrapper---is a familiar one, and it's one of dozens and dozens of exercises of this form that anyone who has taken a GR class has completed.

"Has the penny dropped yet?" No, Farsight. The penny has not dropped. Heck, the Canadian Tire Money has not dropped. There's nothing to drop; there's nothing confusing about any of this.

Here's an analogy to what you are doing.

"Look at this optics equation---if you put something right at the focal point of a lens, the magnification is INFINITY."
"Sure, so what?"
"Don't you see! That violates conservation of energy."
"No it doesn't."
"1/(f-d). Make f=d. Try it, I'll wait. Has the penny dropped yet?"
 
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Here's the other thing, Farsight. You seem to think that you're presenting us stuff we've never through about before. You're expecting people to say "Holy cow---you're right! His clock hasn't budged! I never looked at it that way, that changes everything!

And that's why the arrow can never hit the tortoise! [/zeno]
 
"You know, what Mr. Einstein said is not so stupid..." -- Pauli
That's the classic "appeal to authority" logical fallacy. Just because Einstein said something - and so far, you haven't even presented a quote from him, and I don't take your word for it - doesn't make it true.
Logically, it could dismissed by those grounds, but there's indeed something pretty fishy and very questionable about all this attribution to Einstein in the first place, particularly in support of Farsight's rather strong misconceptions, such as
Your proper time is being measured on a stopped clock. Just because you're stopped too doesn't mean that nothing even slightly unusual happens. It means nothing happens.
and especially statements such as
At the event horizon it isn't nothing unusual happens, it's nothing happens. There are no more events.
It does not make that Einstein, who derived such results as this in collaboration with Rosen: Phys. Rev. 48, 73–77 (1935), would now suddenly take the point of view that spacetime just gets cut off at the horizon of black hole, and then suddenly advance a solution that amounts to gluing two Schwarzschild exteriors together at the horizon.

The Einstein-Rosen "bridge" paper also reveals Einstein's motivation for it: he may have disliked the Schwarzschild interior, his main problem with it was definitely the genuine curvature singularity at the center, not the horizon itself, which, after all, the "bridge" does not get rid of it at all, and rather puts a whole universe of events beyond it.

This also shows that whatever he might have thought about the Schwarzschild horizon at some point, he clearly didn't think it was a genuine physical singularity by at least 1935 (and I don't know if ever and to what extent). In fact, one can even quote Einstein pretty much explicitly telling Farsight that his argument is baloney, both in reasons and conclusion:
If, however, we replace the variable r by ρ defined by the equation
[latex]$\rho² = r - 2m$[/latex]​
we obtain
[latex]\[ds^2 = -4(2m+\rho^2)d\rho^2 - (2m+\rho^2)^2(d\theta^2+\sin^2\theta d\phi^2)+\frac{\rho^2}{2m+\rho^2}dt^2\][/latex]​
This solution behaves regularly for all values of ρ. The vanishing of the coefficient of dt² i.e. (g44) for ρ = 0 results, it is true, in the consequence that the determinant g vanishes for this value; but, with the methods of writing the field equations actually adopted, this does not constitute a singularity.​
From Relativity Theory and Corpuscules essay included in many different books, such as this one.
 
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The Big Bang

I answered to this question:
Physics major question: Big Bang: What Banged?

The Big Bang is the dominant (and highly supported) theory of the origin of the universe.
What Banged? In my view: a qubit of information (a photon) with a very high oscillation frequency.
The frequency of the qubit:
f = (Energy of the universe) / h = Muniverse × c^2 / h = 3.35 × 10^54 × (2.99792458 × 10^8)^2 / (6.62606896 × 10^(-34))
f = 4.544 × 10^104 Hz

Like I said before:
"In the beginning was the qubit" Adrian Ferent
 
What Banged? In my view: a qubit of information (a photon) with a very high oscillation frequency.
Your view is wrong since what Banged was spacetime.
There is also more than one photon in the universe!

The Big Bang was an explosion of spacetime. Ignorant cranks often think that it was an actual explosion of something within spacetime.
 
The photon is an example of qubit
Are a lot of solutions for the Big Bang, this is related to the information…
 
The Big Bang

I answered to this question:
Physics major question: Big Bang: What Banged?

The Big Bang is the dominant (and highly supported) theory of the origin of the universe.
What Banged? In my view: a qubit of information (a photon) with a very high oscillation frequency.
The frequency of the qubit:
f = (Energy of the universe) / h = Muniverse × c^2 / h = 3.35 × 10^54 × (2.99792458 × 10^8)^2 / (6.62606896 × 10^(-34))
f = 4.544 × 10^104 Hz

Like I said before:
"In the beginning was the qubit" Adrian Ferent

Who is this Adrian Ferret?
 
Oh, Farsight. I'm afraid that's completely wrong...
It isn't completely wrong. Yeah yeah, I should have said stationary observer, where his clock rate is a function of gravitational potential. But if you have that observer accelerating, his clock rate tends to zero even faster.

The infalling observer's clock rate expressed as a fraction of the distant stationary observer's clock rate is:
[latex]\[ \frac{d\tau}{dt} = \sqrt{\left(1-\frac{r_0}{r}\right)-\left(1-\frac{r_0}{r}\right)^{-1}\frac{dr^2}{dt^2} - r^2\left(\frac{d\theta^2}{dt^2}+\sin^2\theta\frac{d\phi^2}{dt^2}\right)} \][/latex]
Now, if I take a stationary observer, dr = dθ = dφ = 0, sure enough, that's [latex]$ d\tau = dt\sqrt{1-\frac{r_0}{r}}$[/latex]. But not an infalling observer.
So come on then, run the numbers like I did. Let's see that clock rate.

What did you think the Schwarzschild metric was for, anyway? Window dressing?
I'm the one who's saying it's more than just some coordinate artefact. People who swallow Kruskal-Szekeres coordinates treat the event-horizon singularity like window dressing to be disregarded.

There is actually something almost right about your post, but I'm afraid that if I tell you, you'll simply latch on to that and learn nothing, because your conceptual problems are quite deep.
Baloney. What I'm saying is right, you're dodging.

Let me instead ask you about how much you know of Einstein's work.
1) Are you aware of the geodesic equation and Christoffel symbols? They're featured quite prominently in Einstein's papers on GTR. I know--I read them.
2) Are you capable of calculating an orbit using them? Even a simple radial one, dθ = dφ = 0?
You've not understood Einstein at all. You're just cherry-picking specific cases with no understanding of the bigger picture. Yes, the bigger picture Einstein himself explained.
Aw here we go, hiding behind inscrutable mathematics. If I say yes you sidetrack the discussion demanding that I support my claim, if I say no you say well there you go then. It isn't good enough Vorpal. Everybody can see you're ducking the argument. Let me take a look at the other posts, then I'll nail you to the floor. Hurry up and start backing down, because it's going to be embarrassing.
 
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The coordinate speed of light is a weird, non-localized quantity that you cook up by comparing two particular observers. Yes, it does weird and divergent things. Many observer-observer comparisons do similarly weird things.
There's nothing "weird" about it all. The coordinate speed of light varies in a non-inertial reference frame, like the room you're in. Take a look at this report on a super-accurate optical clock. It's so precise that you can see two of these clocks losing synchronisation when they're separated by only a foot of vertical elevation. Now take a look at wiki re time dilation, and note the bit that says consider a simple clock consisting of two mirrors A and B, between which a light pulse is bouncing. When you simplify those optical clocks to parallel-mirror light clocks, when they lose synchronisation at different elevations this is what's happening:

|---------------|
|---------------|

That's the coordinate speed of light varying in a non-inertial reference frame. Only it isn't actually the coordinate speed of light, it's the speed of light. It varies with gravitational potential. If it didn't, those two optical clocks would stay synchronised. So please, spare us the "weird".

You are pointing out one specific weirdness that occurs when you compare an observer in flat space to an observer hanging on a rope under diverging tension. Why should anyone care? "The coordinate speed of light varies with potential" is no more interesting a statement than "the tension on the rope varies with potential".
See above. Don't dismiss this as uninteresting. This is physics ben. It's not what your good book tells you, but it's simple, and it's right.

Sure it does. A falling observer is in a different reference frame than the rope-hanging observer. You keep constructing "coordinate time" using the rope-hanging observer's clock, NOT the falling clock, so you do not have the luxury of saying "the rope makes not difference". It does make a difference---it imparts an acceleration, and acceleration affects clocks, and you're trying to prove everyone wrong by arguing about clocks. Under the circumstances, you do NOT have the luxury of ignoring differences between clocks.
I'm not ignoring the difference between clocks. I'm addressing it. Clocks clock up some kind of motion. All clocks do this. A light clock clocks up the motion of light. Nothing is weird, it's all very simple. When we see optical clocks at different elevations lose synchronisation, we say gravitational time dilation occurs. And if that goes infinite, the lower clock has stopped. And if light has stopped, it doesn't matter whether the light was falling into the black hole or bouncing back and forth between mirrors.
 
Here's the other thing, Farsight. You seem to think that you're presenting us stuff we've never through about before. You're expecting people to say "Holy cow---you're right! His clock hasn't budged! I never looked at it that way, that changes everything! This is comically wrong.
You haven't thought it through. If you had, you wouldn't be trying the you haven't taken a GR course defence. You'd address the argument. Now come on, give it a shot.

This is where it becomes obvious that you've never taken a GR course or paged through a GR textbook. No, Farsight, none of your statements (the ones that are correct, anyway) are even the slightest bit surprising. You see, this is what learning GR consists of. You take a bunch of spacetimes, and a bunch of metrics, and you do dozens of exercises working through different scenarios. Your conclusion---minus the "OMG this changes everything" wrapper---is a familiar one, and it's one of dozens and dozens of exercises of this form that anyone who has taken a GR class has completed.
Pompous erudite flannel.

"Has the penny dropped yet?" No, Farsight. The penny has not dropped.
No, it hasn't, has it? It will.

Heck, the Canadian Tire Money has not dropped. There's nothing to drop; there's nothing confusing about any of this.
But you think the coordinate speed of light is weird.

"Here's an analogy to what you are doing. "Look at this optics equation---if you put something right at the focal point of a lens, the magnification is INFINITY."
"Sure, so what?"
"Don't you see! That violates conservation of energy."
"No it doesn't."
"1/(f-d). Make f=d. Try it, I'll wait. Has the penny dropped yet?"
Is that the best you can do? A febrile accusation instead of addressing the point of issue? Here's an analogy for what you're doing: Huff, puff, waffle, the man doesn't understand Latin.
 
Me, and every other physicist since the 1960s? Ooookaaay.... <backs away slowly>
Not every physicist. Just those who thump your good book. Try emailing Steven Weinberg to see what he thinks.

Your math (or rather, your interpretation of it) is wrong. But never mind that, because there's a very simple argument that doesn't even involve doing any math. Look at the metric in post #17. It's exactly the same as the near-horizon metric of a black hole. But it's also a metric on flat spacetime, and I can put the horizon anywhere I want in flat spacetime. Therefore, any conclusion that the horizon must be special because of some feature in that metric is manifestly, unambiguously wrong.
No it isn't. I've said this and I'll say it again. Gravitational time dilation goes infinite at the event horizon, so your clock has stopped and you've stopped too. Light has stopped, so you can't measure anything, and there is no metric. Flat spacetime is irrelevant here because spacetime has gone. And you have in no way addressed the issue. The whole point of this discussion is the fallacy that a stopped clock carries on ticking. You said nothing unusual happens to observer. But everything has stopped, so nothing happens.

That's the classic "appeal to authority" logical fallacy.
Oh yes? Now remind me, what did you say above? "Me, and every other physicist since the 1960s? Ooookaaay.... <backs away slowly>". You've been hoisted by your own petard sol.

Just because Einstein said something - and so far, you haven't even presented a quote from him, and I don't take your word for it - doesn't make it true. Since Einstein was an expert on this topic it certainly makes it worth considering...
I haven't presented Einstein quotes because the scientific evidence is more important than Einstein's view. I can if you wish, but I seem to recall that you dismissed them as "out of context". Look at what I said to ben about the coordinate speed of light. It varies. You and I know this, and we know about the Shapiro delay. We also know that if you were travelling at the speed of light, you wouldn't see anything. We know that as far as you're concerned, it isn't nothing unusual happens, it's nothing happens. And we understand the principle of equivalence.

...and it means that establishing it as incorrect requires careful argument and the agreement of other experts. But that's been done, over and over and over again. This analysis is in every textbook on relativity.
Ah, the argument from authority again. I don't care what some expert declares to be right, I care about scientifc evidence, and logic, and sound argument. This is a discussion forum, not a scripture class.

I've derived it myself. Vorpal has derived it. ben has derived it. In fact, the only one in this conversation that can't do the math and hasn't derived it is - you guessed it - you.
Don't hide behind erudition sol. Instead just shoot a light beam between two stars. Slows down, doesn't it. And travels in a straight line. Now make the stars a bit more massive. Then repeat. You know where I'm going with this, so buck your ideas up, pull your finger out, and let's have a sincere discussion about a very interesting subject that takes us places.
 

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