Black Holes & Time: A Closer Look

In summary, the conversation is discussing the concept of black holes, particularly their behavior near the event horizon and the existence of a singularity. The participants question why black holes are black and invisible if they are capable of twisting space and time, and discuss potential effects on objects and signals as they approach the event horizon. They also mention the possibility of black holes being larger on the inside than on the outside and the idea of our universe being inside a black hole. However, these theories are not supported by the mathematics behind the Schwarzschild black hole, which is a vacuum solution with zero density and a singularity that is not a physical place in space.
  • #1
charles watson
5
0
I recently was watching a television show and something has lodged in my brain. They claim that as something approaches a black hole, it swirls in thru the accretion disk and speeds up to at times close to light speed before entering. They also claimed that it leaves an impression or image of itself on the black hole such as an observer would see me virtually frozen on its surface or at least for a very long time. If that is so, I am wondering why a black hole would be black or invisible at all? It would seem to me to be very bright. I am assuming photons would do the same thing otherwise how could an observer see me?
 
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  • #2
If you imagine the falling object emitting identical pulses of light at a regular rate then from your vantage point far away, two things will happen. You will receive those pulses at a slower and slower rate and the pulses will be red-shifted to a lower and lower energy. That's gravitational time dilation and gravitational red shift (which are pretty much the same thing). You will only see finitely many such pulses before the faller passes the horizon. In terms of photons, only a finite number will be emitted, only a finite number can be received and you will lose sight of the faller after a finite (and rather short) time.
 
  • #3
People talk of 'Spaghettification". It would be interesting to know how far into the process our bodies (and transport) would start to function noticeably wrongly. Signals passing through the ship would be out of sync from one end to the other. Would we actually feel something going on? Hollywood has a number of ways of showing it but that's just Hollywood.
 
  • #4
I would imagine a long time before you enter the actual even horizon, your dead. The radiation in the accretion disk would kill you not to mention the heat. You'd also have to think, there would be a lot of electromagnetic energy before you arrived which would fry your brain waves and suck the iron right out of your blood the closer you got.

I often wonder why we always seem to think black holes are matter trapped in a tiny little space. It seems to me that if a black hole can twist space and time, it must be dragging space inside it too. If that's so, they could be larger on the inside than on the outside. If that actually happens, its a great concept for the theory that our universe is actually just that and we live inside a black hole.
 
  • #5
I don't know about larger on the inside but they will always be denser past the event horizon. And everything inside is brought down to a singularity because of the immense gravity.
 
  • #6
AstroChris said:
I don't know about larger on the inside but they will always be denser past the event horizon. And everything inside is brought down to a singularity because of the immense gravity.

There is nothing dense about the standard Schwarzschild black hole. It is a vacuum solution to the Einstein field equations and therefore the density inside (as well as outside) of the event horizon is zero. Furthermore, the singularity is not a place in space.

charles watson said:
I often wonder why we always seem to think black holes are matter trapped in a tiny little space. It seems to me that if a black hole can twist space and time, it must be dragging space inside it too. If that's so, they could be larger on the inside than on the outside. If that actually happens, its a great concept for the theory that our universe is actually just that and we live inside a black hole.

Please refrain from personal speculation. The mathematics behind a Schwarzschild black hole are very clear on what is going on (nothing particular) and the space-time inside it is well understood apart from breaking down when you approach the singularity. Of course, there is no way to actually check this without entering the event horizon (not recommended) and how you are affected by other stuff (such as radiation from the accretion disk) is not described by the space-time model itself.
 
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  • #7
Orodruin said:
There is nothing dense about the standard Schwarzschild black hole. It is a vacuum solution to the Einstein field equations and therefore the density inside (as well as outside) of the event horizon is zero. Furthermore, the singularity is not a place in space.

I'm sure you're coming from an angle on this that I'm not thinking of but Black Holes are most definitely dense. A black hole could be as big as an atom and have the mass of a mountain. And the definition of a singularity is a point or region in spacetime in which gravitational forces cause matter to have an infinite density.
 
  • #8
AstroChris said:
I'm sure you're coming from an angle on this that I'm not thinking of but Black Holes are most definitely dense. A black hole could be as big as an atom and have the mass of a mountain. And the definition of a singularity is a point or region in spacetime in which gravitational forces cause matter to have an infinite density.
This is very full of popular misconceptions about what a black hole is.

  1. Schwarzschild black holes are not dense. If you look at the space-time for a Schwarzschild black hole, it is a vacuum solution to the Einstein field equations, leading to the conclusion that the density everywhere is equal to zero. The "mass" of the black hole is a property of the space-time, not due to "an amount of mass assembled in a point".
  2. You really cannot think about black hole size in this way. That it has a Schwarzschild radius ##r## does not mean that it has a volume that is given by ##4\pi r^3/3##.
  3. No, that is not the definition of the singularity. The singularity is not part of the Schwarzschild space-time and it is where the mathematical description of the black hole breaks down.
 
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  • #9
Orodruin said:
There is nothing dense about the standard Schwarzschild black hole.

I looked at Wiki about this and the Schwarzschild density varies with the original mass. The Sun would need to collapse to a radius of about 3km and it would then have a density of 1.84×1016g/cm2. This is pretty high - but I guess you would argue that, to form a black hole, you would need a much bigger object to start with. For the Milky Way Galaxy, the density of the black hole would be only 3.72×10−8g/m2, which is pretty low. What would be the likely density of any black hole you'd be likely to encounter up-close be, I wonder?
But I'm obviously looking at this with my conventional hat on.
 
  • #10
AstroChris said:
Black Holes are most definitely dense

No, they are not. The density of supermassive black holes can be less than the density of water.

As a learning too, it's really better to ask questions than to make incorrect statements hoping they will be corrected.
 
  • #11
"You can use the Schwarzschild radius to calculate the "density" of the black hole - i.e., the mass divided by the volume enclosed within the Schwarzschild radius. This is roughly equal to (1.8x1016 g/cm3) x (Msun / M)2, where M is defined as above." This quote is from a postdoctoral from Cornell.

So, are you saying that they just CAN be less dense than water or they just aren't dense at all, a zero sum?
 
  • #12
sophiecentaur said:
I looked at Wiki about this and the Schwarzschild density varies with the original mass. The Sun would need to collapse to a radius of about 3km and it would then have a density of 1.84×1016g/cm2
This still has nothing to do with the density of the resulting black hole.

You can of course compute 3M/(4piR^3) and it will have the correct dimensions, but as I have already pointed out, this is not "dividing the black hole mass by the black hole volume".
sophiecentaur said:
But I'm obviously looking at this with my conventional hat on.
Your "conventional hat" does not work in curved space-time.

AstroChris said:
"You can use the Schwarzschild radius to calculate the "density" of the black hole - i.e., the mass divided by the volume enclosed within the Schwarzschild radius. This is roughly equal to (1.8x1016 g/cm3) x (Msun / M)2, where M is defined as above." This quote is from a postdoctoral from Cornell.
Note the "" in the quote. He knows he is lying, but he is taking a liberty to do so in order to make something popularised - ending up with something people take too litterally.
 
  • #13
AstroChris said:
So, are you saying that they just CAN be less dense than water or they just aren't dense at all, a zero sum?
Anywhere you are in the Schwarzschild black hole you will observe zero density.
 
  • #14
Ok, so inside there is zero density observed. As we are looking at it mathematically, knowing that a black hole could be measured to be 10 million x our Sun do we calculate density then or is it irrelevant or is it still zero observed density? Getting correct information can be hard I suppose.
 
  • #15
Orodruin said:
Your "conventional hat" does not work in curved space-time.

I realize that but consider a region containing masses. That region will have a density and an object in orbit round it will follow Newton's Laws and, if it's distant enough, the masses can be regarded as a point mass. The volume of that region will be what it is and can shrink a bit, with the mass staying the same. The orbit of the object will not change, once the masses have condensed far enough to form a black hole. (I think that's right) So, the black hole will occupy a certain volume, observable (after a fashion) from the orbiting object. The density, calculated by mass (remembered) / volume (observed) has a meaning to the observer on the object although it is not the same for a reference frame inside the black hole. So it seems that, along with all the other quantities, relativity gives them different values, depending on the reference frame. That's fair enough and it not as unthinkable as talking about how things look from the point of view of a photon, which is just not valid at all.
 
  • #16
sophiecentaur said:
The volume of that region will be what it is and can shrink a bit
This is not correct. Again, you are trying to impose a Euclidean structure on a space-time where curvature is clearly non-negligible.

While the components of the stress-energy tensor (of which energy density is one) generally depend on the observer - all the components are identically zero in the Schwarzshild space-time.
 
  • #17
Orodruin said:
This is not correct. Again, you are trying to impose a Euclidean structure on a space-time where curvature is clearly non-negligible.

While the components of the stress-energy tensor (of which energy density is one) generally depend on the observer - all the components are identically zero in the Schwarzshild space-time.
But objects will orbit around a black hole so they must 'see' a mass that's non-zero or they would carry on in a straight line. That mass and the extent of the black hole will give a finite (possibly high) density result. At the distance I am considering, the space time behaves as if it were Euclidian. I am not questioning the theory of what goes on near the singularity.
 
  • #18
sophiecentaur said:
But objects will orbit around a black hole so they must 'see' a mass that's non-zero or they would carry on in a straight line
This is a global property of the space-time. Not a result of there being a non-zero density anywhere.

sophiecentaur said:
At the distance I am considering, the space time behaves as if it were Euclidian. I am not questioning the theory of what goes on near the singularity.
Density is a local concept, not a global one. You also implicitly assume a volume of the black hole that is not well defined. I am sorry, but what you are trying simply does not make sense.
 
  • #19
Orodruin said:
This is a global property of the space-time. Not a result of there being a non-zero density anywhere.Density is a local concept, not a global one. You also implicitly assume a volume of the black hole that is not well defined. I am sorry, but what you are trying simply does not make sense.
I know that what I am saying is going against your detailed knowledge of GR but, imagine we were in orbit around a black hole, instead of a dead Sun and that it was surrounded by a disc of debris that meant we couldn't actually see it. (Ignore our human vision etc). By looking at our surrounding bright astro objects, we could deduce our orbit and we would identify that there was a mass (or equivalent) in there, keeping us in place. There would be an Equivalent Mass in there and we could hazard a guess about how much room it takes up. As far as we are concerned, that would correspond to a density.
By sticking to "what's really going on" in there, you are invalidating every model of the Universe that existed before GR and Black Holes got going because the old model don't tell the whole story. That's not the way Science works.
You are 'right', if you choose your definition of density in your way. Can you really say that the definition that we all know and love is not a possible way of viewing this newly found phenomenon? It's no surprise that density is frame dependent. Most other things seem to be. But we still use the schoolboy formulae for most of our lives. KE is still KE and Mass is still Mass.
The actual volume of a black hole may not be "well defined" but we can surely assign some upper limit on it by occultation and lensing effects.
 
  • #20
sophiecentaur said:
By looking at our surrounding bright astro objects, we could deduce our orbit and we would identify that there was a mass (or equivalent) in there, keeping us in place. There would be an Equivalent Mass in there and we could hazard a guess about how much room it takes up.

Again, this is a global property of the space-time which a priori tells you nothing about the local stress-energy tensor. Furthermore, your assumption on "how much room it takes up" is also predicated on an assumption about a Euclidean space. This is (very) far from the situation in the case of a black hole and your hazarded guess will be wildly speculative at best.
sophiecentaur said:
As far as we are concerned, that would correspond to a density.
No it would not. It would have the physical dimension of a density, but it would tell you nothing of the actual density you would find there.

sophiecentaur said:
you are invalidating every model of the Universe that existed before GR and Black Holes got going because the old model don't tell the whole story.
Good! No model before GR gave a proper description of a black hole! Yes you can compute your "density", but it will not be a density in any usual sense of the word. You are refusing to accept that your classical view of space and time does not apply to the situation of a black hole. That is not how science works. Your model tells you something about the global property of the space-time only and therefore has little to do with the local properties, e.g., the local density.

sophiecentaur said:
Can you really say that the definition that we all know and love is not a possible way of viewing this newly found phenomenon?
The problem of your density definition here is that you are implicitly defining a "volume" of the black hole. Defining this volume requires a simultaneity convention. This is not trivial to do in a black hole as, e.g., the radial coordinate is time-like. You cannot simply refer to "the frame in which the black hole is at rest", there is no good definition of this that extends into the black hole region - the volume of which you want to compute!

sophiecentaur said:
The actual volume of a black hole may not be "well defined" but we can surely assign some upper limit on it by occultation and lensing effects.
No, this is what you do not seem to grasp. The Schwarzschild radius of the black hole does not give you a volume in any reasonable sense of the word. You are trying to squeeze a square block through a round hole.
 
  • #21
I am not disagreeing with most of what you are saying and this:
Orodruin said:
The Schwarzschild radius of the black hole does not give you a volume in any reasonable sense of the word.
Is meaningful for me - as long as you can say what that radius implies - to an external observer. Is it to do with how close you can get to the black hole before things apparently change from what you would expect from Newton. So far you have only told me what it is 'not'. :smile:
But do you not acknowledge the idea of an Equivalent Mass for a black hole?
 
  • #22
I have been reading a bit about astronomical observations of deep space objects and 'rough' measures of the quantities involved are quite acceptable there - because they have little else to go on. A ball park figure is often used in the formation of Cosmological theories, which is where Dark Energy and suchlike become a bit fuzzy. I appreciate that's all I can expect here. Or perhaps the Swartzschild radius is not what I need.
 
  • #23
sophiecentaur said:
Is it to do with how close you can get to the black hole before things apparently change from what you would expect from Newton.
No it is not, things will start deviating from Newtonian gravity long before you reach the Schwarzschild radius. You can even see the effects of GR on the orbital precession of Mercury and the Sun is luckily far from being a black hole.

sophiecentaur said:
But do you not acknowledge the idea of an Equivalent Mass for a black hole?

There are several ways of properly defining this in terms of global properties of the space-time (however, not all of them agree for all space-times). The problem comes mainly when you try to assign a "volume" to a black hole. Euclidean geometry (or Minkowski geometry since we are talking about a space-time) is far from a good description of a black hole and you cannot just apply this kind of thinking to it.
 
  • #24
You are missing the original premise of my thoughts: If space is dragged into a black hole, (As I originally stated) There is no reason, that matter need be clumped or dragged into a singularity. The matter and space would simply enter and along with the space spread out evenly where it could grow to an unimaginable size. (Some black holes are 30 billion solar masses)

It would fit an expanding universe quite nicely and especially one that accelerates. Our universe would simply reside inside a black hole of another universe.
 
  • #25
AstroChris said:
I don't know about larger on the inside but they will always be denser past the event horizon. And everything inside is brought down to a singularity because of the immense gravity.

What we observe from the outside would appear...that way because the black hole is smaller on our side of our universe than it is on the inside. IF...black holes eat space as well as matter, it would certainly be composed of much more space than matter. After all, it would constantly be dragging space inside but not necessarily matter.

I have no data to confirm this of course: It is just something that passed thru my mind once. There are scientists that believe we could actually be living inside a black hole though.
 
  • #26
charles watson said:
If space is dragged into a black hole, (As I originally stated)
Please specify what you mean by this and give a proper scientific reference. Space is not a substance, it is an arbitrary assignment of directions in a space-time. Without proper defiition, this statement is meaningless.
 
  • #27
Orodruin said:
Please specify what you mean by this and give a proper scientific reference. Space is not a substance, it is an arbitrary assignment of directions in a space-time. Without proper defiition, this statement is meaningless.
I believe its called frame dragging. And space IS a substance in my opinion. If it were just composed of nothing, gravity would not affect it. We don't understand enough about the nature of space really to determine that.
 
  • #28
charles watson said:
I believe its called frame dragging. And space IS a substance in my opinion. If it were just composed of nothing, gravity would not affect it. We don't understand enough about the nature of space really to determine that.
Please refrain from personal speculation, it is not allowed at Physics Forums.

Thread closed.
 

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 from it. This occurs when a massive star collapses in on itself, creating a singularity with infinite density and zero volume.

2. How do black holes affect time?

According to Einstein's theory of relativity, gravity affects the fabric of space-time. In the case of a black hole, the intense gravitational pull creates a distortion in space-time, causing time to slow down for an observer near the black hole.

3. Can anything escape a black hole?

No, according to current scientific understanding, nothing can escape from a black hole once it crosses the event horizon, which is the point of no return. However, some theories suggest that quantum effects may allow for particles to escape from a black hole over an immensely long period of time.

4. Can black holes be observed?

Yes, although black holes themselves cannot be observed directly, scientists can detect their presence through the effects they have on their surroundings. This includes observing the gravitational lensing of light, as well as the radiation emitted from matter falling into the black hole.

5. Are there different types of black holes?

Yes, there are three types of black holes: stellar, intermediate, and supermassive. Stellar black holes are formed from the collapse of a single star, while intermediate and supermassive black holes are thought to form from the merging of multiple stellar black holes or from the collapse of large gas clouds. Supermassive black holes, found at the center of most galaxies, can have masses equivalent to billions of suns.

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