# What Lies Inside a Black Hole?

• Jim Graham
In summary, the conversation discusses the concept of velocity and time in relation to particles crossing the event horizon of a black hole. While intuitively it is thought that the particle's velocity approaches the speed of light as it approaches the horizon, it is also argued that time dilation causes the particle to age more slowly, making it reach the horizon only after an infinite amount of time has passed outside the black hole. It is also suggested that the space near the horizon must be incredibly curved to allow for this scenario. The conversation also questions the concept of anything existing inside a black hole and whether there is a difference between the end of the universe at the event horizon and the end of the universe elsewhere.
Jim Graham
I've been reading about relativity for several years, but I'm no physicist or mathematician. This question has been bothering me lately, and I'm hoping someone out there can help me understand. I don't have the math to express this briefly, so here it is in words...

When a particle of matter crosses the event horizon of a black hole, what is its velocity with respect to the outside? Intuitively, I think that the velocity approaches the speed of light, c, as the particle approaches the horizon. At the point that it would hypothetically cross the horizon, I think that the particle would have the velocity c.

In my mental image of what is happening, I see the particle accelerating as it approaches the horizon. Time dilation makes the particle age more and more slowly relative to the rest of the universe, approaching zero as the particle approaches the horizon.

So, in the proper time of the particle, when it crosses the horizon, what time is it outside of the black hole? I think that the answer must be that an infinite time has passed there. The end of time has come and gone. The universe has ended. There is no universe any more.

If that is true, then why would we expect anything to be "inside" a black hole? There has not been enough time since the beginning of the universe for anything to have crossed an event horizon. From the perspective of the outside universe, the inside of a black hole does not exist, and will never exist as long as the universe outside still exists.

I understand that the inside exists for the particle, and that you can follow the particle across the horizon, using the appropriate coordinate system, and that nothing special happens at the horizon. From the particle’s perspective, the space-time inside the black hole (up to the singularity) seems to be a smooth continuation of the space-time outside of the black hole. That does not mean that it exists during the lifetime of the outside universe.

From this point of view, the “contents” of the black hole are essentially a two-dimensional boundary that surrounds a hole in the universe. The black hole, its event horizon and its central singularity don’t exist. The universe ends at the point just outside of the horizon, which is reached by the in-falling particle only after an infinite (outside) time.

For this to be true, the space near the horizon must be fantastically curved. There has to be enough space there for a particle to travel “forever” at almost the speed of light. How can that be reconciled with the low tidal forces that I’ve heard are found at the event horizons of large black holes? I guess that the answer is that the space is not “curved”, but “radially distorted”. Length contraction of the in-falling particle (from the outside view) does not fully explain this. The in-falling particle would still cover the short distance at the speed of light. It must be that space itself is radially stretched at the event horizon, to allow an infinite time for the particle to reach the horizon.

So is there anything inside a black hole? If so, where have I gone wrong? If not, why do we talk about black holes as if they were objects with an inside? I wonder if there is any essential difference between the end of the universe at the event horizon, and the “plain old” end of the universe everywhere else.

Wondering...Jim

since the escape velocity for a black hole exceeds c when you are inside the event horizon I would expect that objects falling towards the black hole horizon will have speeds that approach c.

its probably a bad analogy, but:

if you throw something upwards it reaches a point when it is at rest, then afterwards behaves as if it was falling from rest to the ground.

when it reaches the ground it has the same velocity as when it was launched, but in the opposite direction.

now, with a black hole we can do the same, the nearer we get to the event horizon the nearer to c we must launch our object at... so when it falls back down it should also be falling at a speed near to c...

As for what is inside the hole though? That is why we call it black. We can't see inside it or through it. :p

It's nothing. Everything what the black hole is, is the event horizon. Quantum screen, everything is going on there.

Jim Graham said:
In my mental image of what is happening, I see the particle accelerating as it approaches the horizon. Time dilation makes the particle age more and more slowly relative to the rest of the universe, approaching zero as the particle approaches the horizon.

So, in the proper time of the particle, when it crosses the horizon, what time is it outside of the black hole? I think that the answer must be that an infinite time has passed there. The end of time has come and gone. The universe has ended. There is no universe any more.

You need to remember that simultaneity is relative. So the answer of "what age is the universe when the particle crosses the event horizon" does not have an absolute answer.

What you should focus on is when light signals arrive, and when they are received. If an infalling observer watches a distant beam of light, he will observe modest and finite redshifts or blueshifts, depending on his exact trajectory. If the infalling observer free-falls from infinity, he sees the incoming light redshifted to half its original frequency at the event horizon.

Thus the infalling observer does not see the whole history of the universe play out before him.

which was also mentioned (several times) in the last thread.

Won't it take forever for you to fall in? Won't it take forever for the black hole to even form?

Not in any useful sense. The time I experience before I hit the event horizon, and even until I hit the singularity-- the "proper time" calculated by using Schwarzschild's metric on my worldline-- is finite. The same goes for the collapsing star; if I somehow stood on the surface of the star as it became a black hole, I would experience the star's demise in a finite time.

On my worldline as I fall into the black hole, it turns out that the Schwarzschild coordinate called t goes to infinity when I go through the event horizon. That doesn't correspond to anyone's proper time, though; it's just a coordinate called t. In fact, inside the event horizon, t is actually a spatial direction, and the future corresponds instead to decreasing r. It's only outside the black hole that t even points in a direction of increasing time. In any case, this doesn't indicate that I take forever to fall in, since the proper time involved is actually finite.

This is a quote from that Baez article:
If the black hole is eternal, events happening to me (by my watch) closer and closer to the time I fall through happen divergingly later according to you (supposing that your vision is somehow not limited by the discreteness of photons, or the redshift).​
So, if the outside observer never sees anything encounter the event horizon, then from that frame of reference, nothing ever makes it inside during the lifetime of the universe. For an eternal black hole, nothing ever leaves our universe during its lifetime. So nothing is ever “inside” the black hole. The next paragraph in the Baez article says:

If the black hole is mortal, you'll instead see those events happen closer and closer to the time the black hole evaporates. Extrapolating, you would calculate my time of passage through the event horizon as the exact moment the hole disappears! (Of course, even if you could see me, the image would be drowned out by all the radiation from the evaporating hole.) I won't experience that cataclysm myself, though; I'll be through the horizon, leaving only my light behind. As far as I'm concerned, my grisly fate is unaffected by the evaporation.​

So the question of what is inside a black hole applies only to “mortal” black holes. On the other hand, the “mortal” black hole ceases to exist when the in-falling particle reaches the horizon, so nothing is ever “inside” in that case, either. The particle does, however, reach the horizon in a finite (outside) time.

This is where I was headed – if nothing is inside, hidden by the horizon, then why are we concerned about an information paradox. Now I see that the in-falling object can disappear from the universe in finite time, and the information paradox will require some more thought on my part…Jim

Velocity of particle inside even horizon, measured by observer outside?

Hi, Jim,

You have certainly raised many issues here!

Unfortunately, you appear to have rather badly misunderstood what Baez was trying to tell you. He certainly was NOT saying that only "eternal" holes have an interior--- in fact, the whole point was to explain why one should think of "mortal" holes pretty much like one thinks of the eternal ones (the kind modeled by gtr; the "mortality" he refers to requires additional ideas from quantum field theory). I don't want to even try to explain the points which are confusing you (it should help to remark that these points confuse just about everyone when they first encounter gtr), but I DO have a constructive suggestion for you.

You hinted that you don't have a strong mathematical background. In general that is a huge handicap, but fortunately, if you have a strong visual imagination, I believe that you should be able to come to a correct understanding of infall into a black hole, without learning ANY mathematics, from the excellent popular book by Robert Geroch, General Relativity from A to B. Geroch is a leading expert on gtr and he devotes the book to a very careful pictorial exposition which clears up the most common misunderstandings in a very clear but entirely nontechnical manner (as I recall, there is only one equation offered in the entire book--- the pictures will tell you what you need to know.)

I also have some comments which will go way over your head, but you might make a mental note and ask a followup after you've had a chance to study Geroch, re-read Baez, and so on. These comments may also interest other readers here who may have the background to appreciate them immediately.

The question of what the interior of realistic black hole models in gtr is like is one of current interest in classical gravitation. It is important to note that the "no hair" theorems say in effect that the EXTERIOR of black holes all "look more or lesss alike" (Kerr geometry) once they have radiated away any imperfections, but this does not apply to the INTERIOR, where a key issue (pointed out by Penrose) is that INSIDE the horizon, by definition, perturbations, e.g. from infalling and matter and radiation, certainly cannot be "radiated off to infinity" and indeed they can in a sense "collect" along a Cauchy horizon (say in the interior Kerr geometry). One important development here was the advent of the Poisson-Israel model. Another was the discovery by Chandrasekhar and his students of a beautiful "duality" between models of black hole interiors and models of the "interaction zones" of certain colliding plane wave (CPW) models in gtr. Indeed, it turns out that according to gtr, in principle you can create in some region a geometry which is locally isometric to part of the interior (think roughly of the region m < r < 2m) of a black hole by making two carefully crafted gravitational waves (one or both may be accompanied by EM or other radiation) collide! The adjective LOCALLY is essential here.

Jheriko: you wrote "I would expect that objects falling towards the black hole horizon will have speeds that approach c". This is quite wrong; clearing up your confusion involves explaining some of the same issues about velocities in curved spacetimes which I discussed in another thread earlier today. You added "As for what is inside the hole though? That is why we call it black. We can't see inside it". This raises an interesting and important point: according to gtr, observers can certainly fall into a black hole and make physical measurements there, they cannot report their results back to their colleagues outside! This certainly poses an interesting challenge for the standard viewpoint of the relationship between theory and experiment in physics, although so far, this is only a theoretical philosophical issue, as it were!

Tomaz: I hope you were being facetious, but few if any physicists would agree with your claim. You might be thinking of the "holographic principle", but if so I think you seriously misrepresented that idea (which again goes outside gtr for inspiration; it is helpful to try to always set a theoretical context for discussion in order to avoid confusion).

Chris Hillman

> You might be thinking of the "holographic principle"

Yes, I do think that. Volume is just an illusion.

The weak holographic principle.

http://arxiv.org/PS_cache/hep-th/pdf/0003/0003056.pdf

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Chris Hillman said:
Jheriko: you wrote "I would expect that objects falling towards the black hole horizon will have speeds that approach c". This is quite wrong; clearing up your confusion involves explaining some of the same issues about velocities in curved spacetimes which I discussed in another thread earlier today.

Actually, I think it makes sense to interpret JHeriko's post in terms of speeds with respect to (a sequence of) observers that "hover" with constant r, theta, and phi.

A valid interpretation

Hi, George,

Hmm... OK, I see what you mean, and I agree. But I think his post shows why this line of thinking can be misleading!

Chris Hillman

Thanks for the recommendation, Chris Hillman. I’ve ordered the Geroch book. I just bought “Gravitation” by Misner, Thorne and Wheeler, but it looks like it will take me a long time to get to the answers there.

I understand and believe that a black hole has an interior, from the perspective of someone inside the horizon. My question was posed from the perspective of someone OUTSIDE the horizon. When does the outside observer witness anything being hidden by the horizon?

Perhaps the math would help me. I don’t expect a particle to reach the horizon at all, since the space ahead of the particle is stretched as much as the space behind (probably more). But maybe that is my problem? I’ve been thinking of the particle as accelerating, therefore limited to speeds less than c relative to the outside observer. Since the horizon is receding at c from the outside perspective, I expected the outside observer to never witness the encounter of the particle with the horizon within a finite time. Does stretching space somehow allow the outside observer to see particle speeds exceeding c?

So how long does it take (from the outside observer’s perspective) for a particle to reach the horizon? Starting with solar-system-scale distances and speeds, and having the observer accelerate to remain outside the horizon forever; can someone tell me how to calculate the time?

Thanks...Jim

Another Schwarzschild vacuum thought experiment

Jim Graham said:
Thanks for the recommendation, Chris Hillman. I’ve ordered the Geroch book. I just bought “Gravitation” by Misner, Thorne and Wheeler

Excellent! I'd encourage you to look at all the pictures in MTW but don't expect to understand very much until Geroch arrives. I think you'll really like both books once you get into them. (Don't worry, Geroch is MUCH shorter and less demanding, but it has really good pictures.)

Jim Graham said:
Perhaps the math would help me. I don’t expect a particle to reach the horizon at all

Either MTW math plus pictures or Geroch pictures should disabuse you of this expection. (I assume you are asking about what is the prediction of gtr, a somewhat different question from the issue of whether or not this prediction is fulfilled in nature.)

Jim Graham said:
since the space ahead of the particle is stretched as much as the space behind (probably more). But maybe that is my problem? I’ve been thinking of the particle as accelerating, therefore limited to speeds less than c relative to the outside observer. Since the horizon is receding at c from the outside perspective, I expected the outside observer to never witness the encounter of the particle with the horizon within a finite time. Does stretching space somehow allow the outside observer to see particle speeds exceeding c?

Gosh, I think I see quite a few common misconceptions here. Fortunately, Geroch and MTW should be just what you need to become accustomed to the many ways in which your Newtonian and flat space intuition needs to adapt in order to give you an adequate intuitive understanding of spacetime and curvature.

Since I just wrote a lengthy post pointing out the existence of multiple competing notions of "distance" in the Schwarzschild geometry, I'll just add that above when you refer to "speed" you are probably tacitly assuming that speeds measured over noninfinitesimal distances have a unique meaning, if we fix an observer and a target. But this isn't true, because noninfinitesimal "distances" do not have a unique meaning,
even if we fix an observer and a target.

Jim Graham said:
So how long does it take (from the outside observer’s perspective) for a particle to reach the horizon? Starting with solar-system-scale distances and speeds, and having the observer accelerate to remain outside the horizon forever; can someone tell me how to calculate the time?

Good grief, Jim, we must be on the same wavelength because you just asked the very question I studied in the very next page of my voluminous notes which I was referring to while writing the post I just mentioned. I'll have to leave that until tommorrow, but the post on distances should keep you happily occupied tonight, though.

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Chris Hillman said:
Hi, Jim,
Jheriko: you wrote "I would expect that objects falling towards the black hole horizon will have speeds that approach c...

George Jones said:
Actually, I think it makes sense to interpret JHeriko's post in terms of speeds with respect to (a sequence of) observers that "hover" with constant r, theta, and phi.

I wasn't considering any particular observer, just that as an object is "launched" and then falls there is a certain symmetry. If the object is launched with some velocity v normal to a sphere creating a spherically symmetric field and then returns to the same point (whilst on its freely falling trajectory) then the 'energy gained' by 'climbing the potential', which is converted from kinetic energy to reach the top, is converted back on the way down. Assuming no losses the velocity should be the same... which ever observer you decide to be this should hold true, even if something else appears to happen because of all the curvature. Correct? Or am I missing something?

Maybe my idea is "too classical" for discussion of a black hole...

Hi, Jheriko, can you clarify the question? Since there has been some confusion over what thought experiment you have in mind, perhaps you can restate this as clearly as possible?

Chris Hillman

Chris Hillman said:
Since I just wrote a lengthy post pointing out the existence of multiple competing notions of "distance" in the Schwarzschild geometry, I'll just add that above when you refer to "speed" you are probably tacitly assuming that speeds measured over noninfinitesimal distances have a unique meaning, if we fix an observer and a target.

Yes, that is what I am thinking about "speed". Is that not true in GTR?

I got tired of slogging through MTW from the beginning, so I skipped ahead, looking at the pictures as you suggested. I think I did find something relevant to my question in Firgure 25.5, page 667 of my copy. It shows a diagram of r/M versus time/M for a particle falling into a black hole, as seen by both a “co-moving observer” labeled “Proper time” and a “faraway observer” labeled “Schwarzschild time”.

The caption says in part “In the one description [co-moving observer], the point r=0 is attained, and quickly. In the other description, r=0 is never reached and even r=2M is attained only asymptotically.” I take this to mean that the “faraway observer” never sees the particle cross the event horizon, so he should never worry that it is hidden by the event horizon. That is what I am trying to understand about the information paradox.

The Baez article did help me see that an evaporating black hole can be a problem in this regard – it disappears in finite time, so I can understand why there might be concern about the information content of the detritus versus the original in-falling objects. I now seem to recall something to this effect in my earlier reading. I guess that maybe I don’t understand what the information paradox is about (just one of the many things that I don’t understand).

I appreciate your patience with me, and I look forward to your future posts on this and other threads. Thanks...Jim

Where oh where is that post where I...?

Hi, Jim,

I wrote "Since I just wrote a...
Chris Hillman said:
[...lengthy post...]
...pointing out the existence of multiple competing notions of "distance" in the Schwarzschild geometry, I'll just add that above when you refer to "speed" you are probably tacitly assuming that speeds measured over noninfinitesimal distances have a unique meaning, if we fix an observer and a target."

(Is there any provision for keeping a running list of posts one might later want to cite? And I obviously haven't yet learned how to cite a post I wrote in a less awkward manner--- can someone tell me what is the markup for an internal link? What is the most efficient way to obtain the numerical ID of a post?)

Jim Graham said:
Yes, that is what I am thinking about "speed". Is that not true in GTR?

I should have provided the link to the post in question earlier, but this is the topic of the post I mentioned and which I have now linked to just above.

In this post, I explained two distinct operationally significant notions of "distance" over an extended region (one not even symmetric) and compared them quantitatively, finding that for radially separated observers the three quantities obey a fairly memorable inequality.

Jim Graham said:
I got tired of slogging through MTW from the beginning, so I skipped ahead, looking at the pictures as you suggested. I think I did find something relevant to my question in Firgure 25.5, page 667 of my copy. It shows a diagram of r/M versus time/M for a particle falling into a black hole, as seen by both a “co-moving observer” labeled “Proper time” and a “faraway observer” labeled “Schwarzschild time”.

Skipping ahead and jumping around is indeed the best way to get your feet wet in MTW. But the pictures I think you should be looking at occur a bit farther on, in section 31.4.

Try the pictures in Box 31.2, which depicts infinitesimal light cones (drawn using a suitable frame field) at various events in a Schwarzschild hole. In a photocopy of the picture on p. 829, sketch a vertical line outside the shaded cylinder; this is the world line of some hovering observer. Looking at the world line labled "world line of infalling particle", you can figure out how to sketch the world line of a particle dropped by the hovering observer. At the event where the particle is dropped, its world line will be tangent to the world line of the hovering observer, but that world line is bending radially outward (in the picture, it appears straight and the falling particle's world line appears curved, but geometrically it is just the other way around!), so the two world lines diverge and the dropped particle falls into the hole in finite proper time by an ideal clock carried with the particle. But radially outgoing light signals from the infalling particle are redshifted out of existence just before it passes through the horizon, and thereafter it cannot send signals to the hovering observer, although it can receive signals which the hovering observer sends after it into the hole for a brief time before it falls into the curvature singularity at r=0.

Jim Graham said:
The caption says in part “In the one description [co-moving observer], the point r=0 is attained, and quickly. In the other description, r=0 is never reached and even r=2M is attained only asymptotically.”

Right, and from Box 31.2 that should make more sense now.

Jim Graham said:
I take this to mean that the “faraway observer” never sees the particle cross the event horizon,

Right.

Jim Graham said:
so he should never worry that it is hidden by the event horizon. That is what I am trying to understand about the information paradox.

I don't know what you mean by "he should never worry".

As for the information paradox, I think that is far beyond your level right now (if it's too hard, as I believe, for Hawking and other leading researchers, given the present state of physics, it's certainly much too hard for a gtr newbie!). I'll just remind you that this involves other ideas (from quantum field theory) while lie outside the domain of classical relativistic physics, and that QFT is far more counterintuitive than gtr, so I'd advise you to focus on acquiring good intuition for the geometric features of classical black hole models.

Chris Hillman

Chris Hillman:

The kicker for me was the Geroch book, which arrived this weekend. It helped me a lot. I can now understand that an external observer is not completely disconnected from the space-time inside the horizon of a black hole – he can cross the horizon himself, and still encounter someone who fell in earlier, if things are arranged properly.

On the other hand, in this situation, I’m not convinced that there ever was a horizon separating the two travelers. The observer would see every instant of his friend’s existence as the observer caught up with and encountered his friend. No light would be “redshifted out of existence just before it passes through the horizon”.

It is hard to imagine what is going on when presented with a concrete image of a “horizon”. The horizon is really a more ephemeral thing, describing the relationship between the observer and the black hole. I’m feeling better about it now. The “twisted” space-time is still hard to imagine, but I think I am getting the flavor of it.

I did see your earlier post on the thread https://www.physicsforums.com/showthread.php?t=14019" and left a few comments there. (I see you’ve posted some more since then)…Jim

PS - about embedding links - I copied the address from my browser while looking at the other thread, then used the "go advanced" option to create the link. (I think that will work). You could probably keep the resulting URL text string in a file on your machine for pasting in later posts.

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Progress toward understanding event horizons

Jim Graham said:
the Geroch book, which arrived this weekend. It helped me a lot. I can now understand that an external observer is not completely disconnected from the space-time inside the horizon of a black hole – he can cross the horizon himself, and still encounter someone who fell in earlier, if things are arranged properly.

Good!

Jim Graham said:
On the other hand, in this situation, I’m not convinced that there ever was a horizon separating the two travelers. The observer would see every instant of his friend’s existence as the observer caught up with and encountered his friend. No light would be “redshifted out of existence just before it passes through the horizon”.

Who said that "light would be “redshifted out of existence just before it passes through the horizon"? Certainly not I--- gtr doesn't say anything like that, and I don't know how you might have gotten this impression. Keep studying the Geroch book, maybe you'll figure out on your own why I objected here.

Jim Graham said:
It is hard to imagine what is going on when presented with a concrete image of a “horizon”. The horizon is really a more ephemeral thing, describing the relationship between the observer and the black hole. I’m feeling better about it now. The “twisted” space-time is still hard to imagine, but I think I am getting the flavor of it.

Well, no-one said this is supposed to be easy! (I might have implied that in my post about my own first encounter with gtr, but you shouldn't assume that everyone will take to curved Lorentzian manifolds quite so painlessly.) Keep reading Geroch and keep drawing your own spacetime diagrams.

Jim Graham said:
PS - about embedding links - I copied the address from my browser while looking at the other thread, then used the "go advanced" option to create the link. (I think that will work).

That's basically what I've been doing to obtain a link to a post/thread, but I assume there is a one-step process, and I still don't know the proper Physics Forums markup to link to a specific post "by hand" if you don't want to quote text from it.

Chris Hillman

I have a "quick" question, then. Let me just say that I am a COMPLETE newb at this entire subject and that it intrigues me to no end. I don't have a "strong" mathematical background, but have normally been good at math, I just never pursued it. Due to that, I have been reading several forums on the subject of black holes in the past week. But after reading the latest posts in this thread, I have a new question that I just assumed about before.

If the observer dropped the particle and it started on its trip toward the black hole, would the observer not lose "sight" of the particle because of the fact (or at least I think it's a fact) that light cannot exit a black hole? So the observer would not be able to receive the particle in a visual sense, correct?

Apologies of that is completely and utterly wrong. Ha.

Matt

Jim: An excellent book is Kip Thorne's BLACK HOLES AND TIME WARPS. Loads of concepts explanations and diagrams, no really math. Another is THE BLACK HOLE WAR by Leonard Susskind which features the arguments between Susskind and Hawking...and again no math...both sources very detailed and insightul.

Here’s my theorey about the size of a star composed of relativistic material:

The gravitational energy could be as low as (4GM^2)/(5R) for a typical density profile, or possibly as high as (GM^2)/R (unlikely) if the star has a high density core. The total energy creating pressure would be (Mc^2)/3. Using the viral theorem (the energy creating pressure equals half the gravitational energy), a non-rotating star of relativistic material would have a radius as small as (1.2GM)/(c^2) or as large as (1.5GM)/(c^2), or between 60 - 75% of the Schwarzschild radius.

If this model is true, it could be verified someday by the observation of the merger of two approximately equal mass black holes: a massive ejection from the relativistic stars would occur.

This also presents a different possible “origin” of our universe other than the big bang. Consider if two massive orbiting black holes merged, with each approximately half the mass of the universe. They would eject relativistic material for millions of years.

the Geroch book, which arrived this weekend. It helped me a lot. I can now understand that an external observer is not completely disconnected from the space-time inside the horizon of a black hole –

An external observer IS 'disconnected' from inside...that is precisely what a horizon entails.

This quote shows why nothing we observe from the outside can be inside the horizon (and a little about what is inside) :

Kip Thorne says (Lecture in 1993 Warping Spacetime, at Stephan Hawking's 60th birthday celebration, Cambridge, England,)

The flow of time slows to a crawl near the horizon, and beneath the horizon time becomes so highly warped that it flows in a direction you would have thought was spacial: it flows downward towards the singularity. That downward flow, in fact, is why nothing can escape from a black hole. Everything is always drawn inexorably towards the future, and since the future inside a black hole is downward, away from the horizon, nothing can escape back upward, through the horizon.

Here is a good online discussion about what is inside...

C:\Users\Owner\Documents\PHYSICS\RELATIVITY black holes,Gravity\Black Holes\Inside a black hole.mht

You may find this one interesting too :

http://en.wikipedia.org/wiki/Fuzzball_(string_theory )

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So why not calculate the radius of a fuzzball or quark star? At any point pressure should be given by P = (rho)(c^2)/3, where rho is the density.

Naty1 said:
Here is a good online discussion about what is inside...

C:\Users\Owner\Documents\PHYSICS\RELATIVITY black holes,Gravity\Black Holes\Inside a black hole.mht

I use a Mac via aol.com on a telephone line so I can't use the shortcuts you use. Do you have a URL for: :\Users\Owner\Documents\PHYSICS\RELATIVITY black holes,Gravity\Black Holes\Inside a black hole.mht ?

Will be back this afternoon.

Naty1 said:
Here is a good online discussion about what is inside...

C:\Users\Owner\Documents\PHYSICS\RELATIVITY black holes,Gravity\Black Holes\Inside a black hole.mht

I'm not concerned about someone accessing files on my computer. I just have no idea how to access the information at: C:\Users\Owner\Documents\PHYSICS\RELATIVITY black holes,Gravity\Black Holes\Inside a black hole.mht

## 1. What exactly is a black hole?

A black hole is a region in space where the gravitational pull is so strong that nothing, including light, can escape. It is formed when a massive star collapses under its own weight.

## 2. What is inside a black hole?

The exact interior of a black hole is still unknown, but it is believed that it contains a singularity, which is a point of infinite density and zero volume. The gravitational pull of the singularity is what creates the event horizon, the point of no return for anything that enters the black hole.

## 3. Can anything escape from a black hole?

No, once something crosses the event horizon of a black hole, it cannot escape. The gravitational pull is too strong for even light to escape, which is why it appears black.

## 4. Is time affected inside a black hole?

Yes, time is affected inside a black hole due to the strong gravitational pull. Time moves slower the closer you get to the event horizon, and at the singularity, time stops completely.

## 5. Can black holes ever be seen?

No, black holes cannot be seen directly since they do not emit or reflect any light. However, their presence can be detected through their effects on nearby matter and light, such as the distortion of starlight or the radiation emitted from matter falling into the black hole.

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