Is there a maximum mass for a black hole?

AI Thread Summary
The discussion centers on the mass of black holes, specifically questioning whether there is a maximum mass limit. It is clarified that while calculations of black hole mass can be complex and often miscalculated using Newtonian physics, there is no theoretical maximum mass for a black hole beyond the total mass-energy of the observable universe. The importance of using accurate methods, such as general relativity and considering the gravitational effects of surrounding matter, is emphasized for accurate mass determination. The conversation also touches on the nature of black holes, including the event horizon and the behavior of matter within it, suggesting that the understanding of black holes remains incomplete. Overall, the dialogue illustrates the complexities of black hole physics and the ongoing exploration of their properties.
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I recently tried to calculate the mass of the black hole in the center of the milky way and it came out to 1.8x10e+53 kg, that can't be right, what's going on?
 
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Well your calculation is very wrong, since the mass of the black hole is actually something like 10^{37} kg.

But in short, no there is no theoretical maximum size for a black hole, except for perhaps the sum of all the mass energy in the observable universe.
 
rogerperkins said:
I recently tried to calculate the mass of the black hole in the center of the milky way and it came out to 1.8x10e+53 kg, that can't be right, what's going on?

How did you calculate it?
 
Did you try to calculate the mass with Newtonian physics? Calculating black holes without general relativity can run into problems.
 
Oops, I found an error in my original calculation :eek:. New calculation gives me about 2e41. Yes, I only used Newtonian physics, thought about relativistic effects, but not sure what those would be or how to calculate. I ignored any effects from the mass in the rest of the galaxy, not sure if that's significant. I also ignored any decay in the orbit of the sun. I used wikipedia to get most of the values. Here is my calculation:

F = G (m1 m2 / r^2)
F = ma
a = G (m / r^2)
G = 6.674e-11 N m^2 / kg^2
r = 8.3 kpc
1 parsec = 3.0856802e16 m
r = 2.561e20 m

Vsun = 230,000 m/s
a = v^2 / r
a = 2.066e-10 m/s^2

m = a r^2 / G
m = 2.030e+41 kg

Thanks!
 
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rogerperkins said:
I ignored any effects from the mass in the rest of the galaxy, not sure if that's significant

It is! You wouldn't necessarily know it from just doing a naive calculation, though. The SMBH is in reality something like 10^7 M_{\odot}, while the galaxy as a whole is something like 10^{11} M_{\odot}, so most of the gravitational pull on the sun that would factor into the calculation you've just done is coming from normal (and dark) matter, not the black hole in the center.

To get the mass of the black hole you have to use the orbit of something much much closer to the black hole, so that you're ensured that the majority of the gravitational force is due to it. This is precisely what is done!
 
no calculations here, just logic:

Starting from the, considered true, fact that the black holes occupy space(like other compacted matter objects, stars, neutron stars):

black holes also have a range of mass, why? they express themselves via a volume(area) of space so that means that there is something holding contents of the black hole into a structure that occupies space. If it did not have a maximum mass it would simply be an infinetely small point being able to absorb everything, something like reverse big-bang.
i don't buy the "matter can't be compacted any further" statement...we have clear evidence that it was..
 
morghen said:
no calculations here, just logic:

Starting from the, considered true, fact that the black holes occupy space(like other compacted matter objects, stars, neutron stars):

black holes also have a range of mass, why? they express themselves via a volume(area) of space so that means that there is something holding contents of the black hole into a structure that occupies space. If it did not have a maximum mass it would simply be an infinetely small point being able to absorb everything, something like reverse big-bang.
i don't buy the "matter can't be compacted any further" statement...we have clear evidence that it was..

The diameter of the black hole is usually considered to be where the event horizon is. This is not a "structure". It is simply the distance from the center of the black hole that the gravitational strength becomes great enough to keep light from leaving. We don't know what is behind the event horizon, specifically whether there is an actual singularity or if that is simply a mathematical error that stems from our lack of knowledge about it.
 
So you're saying the observable diameter of the object has no corelation to its mass?
You're satisfied with "simply the distance from the center of the black hole to the event horizon" ?

Even if the event horizon is just a shell around a point with zero/one volume, what's behind the EH is probably not empty, but accelerating material that has passed the event horizon and it is heading towards the maximum gravity point...so there must be a flowing structure.

If however the black hole is a solid globe of compressed matter that occupies space then there must be a critical mass point.
 
  • #10
The Schwarzschild radius is proportional to its mass.
While this is not appropriate close to black holes, if you calculate a "volume" and a "density", it decreases for larger black holes.

If it did not have a maximum mass it would simply be an infinetely small point being able to absorb everything
Where is the problem?

If however the black hole is a solid globe of compressed matter that occupies space then there must be a critical mass point.
It is not, at least not with the Schwarzschild radius. And it does not matter how it looks inside. The event horizon is just a result of GR in a region where GR is valid.
 
  • #11
morghen said:
So you're saying the observable diameter of the object has no corelation to its mass?

No, the more massive a black hole is the larger the diameter of the event horizon.
You're satisfied with "simply the distance from the center of the black hole to the event horizon" ?

Yes.

Even if the event horizon is just a shell around a point with zero/one volume, what's behind the EH is probably not empty, but accelerating material that has passed the event horizon and it is heading towards the maximum gravity point...so there must be a flowing structure.

I would not call infalling material a "flowing structure".

If however the black hole is a solid globe of compressed matter that occupies space then there must be a critical mass point.

What is this critical mass point?
 
  • #12
Drakkith said:
Yes.
hehe, this is a bit like saying: god went click and the light was on :P

Drakkith said:
I would not call infalling material a "flowing structure".
why not? what would you call it? or you think it just infalls without any rules/properties?

Drakkith said:
What is this critical mass point?
why are you being sarcastic? how should i know? but if the black hole occupies any space at all there probably is a certain mass value after which there come changes within/out the black hole.
Why would you believe the black hole is such a rigid and ultimate concept?
 
  • #13
morghen said:
hehe, this is a bit like saying: god went click and the light was on :P

What are you talking about? We have defined the diameter of a black hole to be this way, I can't see a relation between your statement here and the diameter of a black hole.

why not? what would you call it? or you think it just infalls without any rules/properties?

The infalling material is in free fall unless it collides with other infalling material, just like it does outside of the black hole, and it should obey the same rules, at least up to a certain point. I don't know where the rules would begin to break down. If you want to call this a structure, then feel free.
why are you being sarcastic?

I'm not. I actually just now realized what you were talking about.

how should i know? but if the black hole occupies any space at all there probably is a certain mass value after which there come changes within/out the black hole.

Maybe. It's possible a quark star or other exotic stellar remnant could form an event horizon. If more mass is added that star may then collapse into something else. We simply don't know yet.

Why would you believe the black hole is such a rigid and ultimate concept?

Please, don't put words in my mouth, I have said nothing of the sort.
 
  • #14
Sorry for that, just trying to push a bit on fact that you said: Yes after i asked if you're satisfied with answers like "simply the distance from the center of the black hole to the event horizon" when it comes to what's beyound the event horizon.

i would really like to see theories on how the material travels after the event horizon.
 
  • #15
A black hole, in theory, has another 'structure' inside the event horizon called the Cauchy horizon, and has another 'structure' outside the event horizon called the photon sphere. We obviously have no direct knowledge of how matter behaves inside the event horizon because ... it's inside the event horizon. According to theory, it is merely disassembled and and absorbed by the singularity after it passes the event horizon.
 
  • #16
Has anyone ever tried to calculate escape velocity during a stellar collapse. There would be an initial escape velocity due to the mass of the star before collapse. what would be the escape velocity for a neutron star for instance? Or a red dwarf? How would you actually calculate such values?
 
  • #17
Similar to all other objects, if you neglect relativistic effects. v=\sqrt{\frac{2GM}{r}} where M is the mass inside for spherical mass distributions. For neutron stars, it might be useful to add some relativistic corrections, but the formula gives a good approximation.
 
  • #18
mfb said:
Similar to all other objects, if you neglect relativistic effects. v=\sqrt{\frac{2GM}{r}} where M is the mass inside for spherical mass distributions. For neutron stars, it might be useful to add some relativistic corrections, but the formula gives a good approximation.

What about matter compression? To plot the velocity when the compression approaches singularity the increased compression needs to be included. How would the equation be modified to account for this?
 
  • #19
I have found a wikipedia article here.

http://en.wikipedia.org/wiki/Escape_velocity

The second equation under the heading "Calculating an escape velocity" has p for average density but this may be inadequate for my purposes.
 
  • #20
no calculations here, just logic:

QUOTE]

As far as I can tell no a single statement you imagine is correct. I'm not saying there is no 'logic' in your thinking, in fact I can't make any sense of much of that post, but it seems you are extending classical analogies to relativistic black holes. That doesn't apply. It won't work.

Are you aware spacetime inside a black hole becomes very distorted...that is very, very curved. So you can't use classical measures of time and distance. Those are based on Eucledean space and a typical BH is described by Schwarzschild coordinates.
The volume of a BH is NOT the classical 4/3[pi]r3...nor is the surface area the classical 4[pi]r2 There is generally believed to be NO matter inside...although some may be infalling at a particular time. Did you know the curvature of a charged BH is different from that of one with no charge...because of the additional energy of an electromagnetic field.

Are you aware the absolute BH horizon begins to grow before matter reaches it? Are you aware that the 'radius' inside a BH is a time dimension, not a distance. That the singularity is a point in time not in space? Are you aware the relative horizon jumps discontinuously with changes in matter/energy? That a newborn BH exhibits violent, chaotic tidal oscillations of a BKL singularity...and these gradually disappear as the BH ages?

These are all things I don't think are available by any convenient logic; they flow from mathematical models of GR.

Here are a few descriptions I keep to remind me how strange BH actually are:

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.

Black Hole Complementarity
Leonard Susskind, THE BLACK HOLE WAR (his arguments with Stephen Hawking)
(p238) Today a standard concept in black hole physics is a stretched horizon which is a layer of hot microscopic degrees of freedom about one Planck length thick and a Planck length above the event horizon.

(p258) From an outside observer’s point of view, an in falling particle gets blasted apart….ionized….at the stretched horizon…before the particle crosses the event horizon. At maybe 100,000 degrees it has a short wavelength and any detection attempt will ionize it or not detect it!

http://www.jimhaldenwang.com/black_hole.htm

{Inside the horizon:}
It is the coordinate with the minus sign that determines the meaning of “timelike. Notice how the minus sign has moved from the t coordinate to the r coordinate. This means that inside the event horizon, r is the timelike coordinate, not t. ... According to GR, inside a black hole, time is defined by the r coordinate, not the t coordinate.

In fact horizons are spheres of coordinate timelike singularities not ones of classical volume.
 
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  • #21
But in short, no there is no theoretical maximum size for a black hole, except for perhaps the sum of all the mass energy in the observable universe.

This is probably the best short answer to the original question.

Near the end of the universe, when things are empty and cold, and entropy is nearing a maximum, there may be several/many BH remaining. These will gradually disappear via Hawking radiation...because individual BH are not repositories of maximum entropy...so they will be unstable...

On the other hand it seems most of these BH will be causally disconnected at some point...very far apart...so maybe their Hawking radiation will simply dissipiate as does the CMBR currently...and eventually in a flat universe:

... in the heat death scenario, the energy density is so low that the system can be thought of as non-gravitational, such that a state in which energy is uniformly distributed is a thermal equilibrium state, i.e., the state of maximal entropy.

http://en.wikipedia.org/wiki/Heat_death_of_the_universe

but apparently this is one of a number of possible scenarios; Anyway, we won't be there to see which one happens!
 
  • #22
Naty1 said:
no calculations here, just logic:

QUOTE]

As far as I can tell no a single statement you imagine is correct. I'm not saying there is no 'logic' in your thinking, in fact I can't make any sense of much of that post, but it seems you are extending classical analogies to relativistic black holes. That doesn't apply. It won't work.

Are you aware spacetime inside a black hole becomes very distorted...that is very, very curved. So you can't use classical measures of time and distance. Those are based on Eucledean space and a typical BH is described by Schwarzschild coordinates.
The volume of a BH is NOT the classical 4/3[pi]r3...nor is the surface area the classical 4[pi]r2 There is generally believed to be NO matter inside...although some may be infalling at a particular time. Did you know the curvature of a charged BH is different from that of one with no charge...because of the additional energy of an electromagnetic field.

Are you aware the absolute BH horizon begins to grow before matter reaches it? Are you aware that the 'radius' inside a BH is a time dimension, not a distance. That the singularity is a point in time not in space? Are you aware the relative horizon jumps discontinuously with changes in matter/energy? That a newborn BH exhibits violent, chaotic tidal oscillations of a BKL singularity...and these gradually disappear as the BH ages?

These are all things I don't think are available by any convenient logic; they flow from mathematical models of GR.

Here are a few descriptions I keep to remind me how strange BH actually are:

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



Black Hole Complementarity
Leonard Susskind, THE BLACK HOLE WAR (his arguments with Stephen Hawking)






In fact horizons are spheres of coordinate timelike singularities not ones of classical volume.

Well I am not trying to model black holes I am just playing with ideas. You can humour me or not but I am just experimenting. I simply need a method of calculating a density and acceleration away from a point within that density.
 
  • #23
I have found a page at superstringtheory.com that gives me what I need. Can anyone help in getting an understanding of this. I have no idea how I would translate this into code to produce data that can be graphed.

http://www.superstringtheory.com/blackh/blackh1a.html

Better still is there already a graphical representation.
 
  • #24
Can anyone tell me if the following statement from the above site is true.

"For a planet the mass of the Earth, this distance is only about a centimeter. So if the Earth were less than a centimeter in diameter, the escape velocity at the surface would be greater than the speed of light."
 
  • #25
hubble_bubble said:
Can anyone tell me if the following statement from the above site is true.

"For a planet the mass of the Earth, this distance is only about a centimeter. So if the Earth were less than a centimeter in diameter, the escape velocity at the surface would be greater than the speed of light."

Without doing the math it sounds about right.
 
  • #26
hubble_bubble said:
I have found a page at superstringtheory.com that gives me what I need. Can anyone help in getting an understanding of this. I have no idea how I would translate this into code to produce data that can be graphed.

http://www.superstringtheory.com/blackh/blackh1a.html

Better still is there already a graphical representation.

What exactly do you want to graph?

This website seems a little silly; just looking at it, the author for some reason writes Newtonian gravity in arbitrary D dimensions, then just states the Einstein equations and the schwarzschild solution in D=4... OK. Nothing is flat out wrong, it's just strange (especially since nothing on this page has anything to do with superstring theory).
 
  • #27
Nabeshin said:
What exactly do you want to graph?

This website seems a little silly; just looking at it, the author for some reason writes Newtonian gravity in arbitrary D dimensions, then just states the Einstein equations and the schwarzschild solution in D=4... OK. Nothing is flat out wrong, it's just strange (especially since nothing on this page has anything to do with superstring theory).

Sometimes discoveries are made by mistake. Maybe he may make the right mistake. :-)

I want to plot density of a mass against the calculated escape velocity. As stated above does a 1 cm Earth have an escape velocity that is greater than the speed of light? If so I would assume it has an event horizon. This would technically be equivalent to a black hole, but the mass is too small. I just want to play with the figures to see where I end up. I am not interested in modeling the real universe at this stage. I just want to examine different avenues in related areas. Tweaking the variables in novel ways can bring to light possibilities that have not been taken into consideration.

I would like to graph the density of a spherical mass against the escape velocity at various distances from the centre of said object. So this would be a series of graphs.
 
  • #28
hubble_bubble said:
I want to plot density of a mass against the calculated escape velocity. As stated above does a 1 cm Earth have an escape velocity that is greater than the speed of light? If so I would assume it has an event horizon. This would technically be equivalent to a black hole, but the mass is too small.

No, it would not be too small, it would be a bona fide black hole. (The figure of 1cm is roughly correct)

There is no minimum mass (except for, perhaps, the Planck mass) for a black hole, and as I already stated no [clear] maximum mass. Everything in between is obtainable. Of course, all of the ones which are not ~solar mass to billions of solar masses don't appear to be realized in nature, but that's not really the point.
 
  • #29
It appears you may be under the impression that matter density [pressure] effectively increaes rest mass, due to mass-energy equivalence. This is untrue. The effective mass of a black hole, or condensed matter object, is the same as its uncompressed progenitor mass.
 
  • #30
Chronos said:
It appears you may be under the impression that matter density [pressure] effectively increaes rest mass, due to mass-energy equivalence. This is untrue. The effective mass of a black hole, or condensed matter object, is the same as its uncompressed progenitor mass.

No I know the mass is the same. It is simply in a smaller volume. What I meant was, as the last poster pointed out, is that Earth mass is too low to collapse naturally into a black hole. That is not the point of what I am attempting. I want to start from a simple premise. At the point I have the basic information I need I will be applying that elsewhere.
 
  • #31
How about minimum mass for black holes caused by gravitational collapse. Isn't it something like three solar masses?
 
  • #32
3 solar masses is the mass limit for the star in the calculations, the remaining black hole would have a lower mass (I think something like 2 solar masses?). However, no black holes of this size were detected yet, so this is a bit speculative.
 
  • #33
mfb said:
3 solar masses is the mass limit for the star in the calculations, the remaining black hole would have a lower mass (I think something like 2 solar masses?). However, no black holes of this size were detected yet, so this is a bit speculative.

I assume you mean that the other mass is ejected before or during the collapse.

I am looking at a modified Schwarzschild calculation for the data I need. I want to work in the effects on time too. The fact that e=mc2 leads onto a calculation where c becomes negative and mass compression becomes a component. What does mass compression do to energy levels? Could energy form around a singularity. As you have the event horizon could you have another band near the singularity where time is running at a comparable rate to that of light elsewhere and light itself is stationary?

Imagine a collision of particles within the event horizon. this initiates an energy release in the form of a photon which wants to head toward the event horizon. It will be impossible for the photon to do this. The particle is no longer "experiencing " light as it normally acts. As light may now appear static, time may take its place in the environs of a singularity. Now if c is zero this makes no sense. If c however is negative then this may indicate that time is negative, but this is not necessarily so. If time was negative then particles would be attracting light rather than emitting it. This would indicate an increase in energy which is counter intuitive near the singularity.
 
  • #34
Have a think about this.

"Objects in a gravitational field experience a slowing down of time, called time dilation. This phenomenon has been verified experimentally in the Scout rocket experiment of 1976 [2], and is, for example, taken into account in the GPS system. Near the event horizon, the time dilation increases rapidly. From the point of view of an external observer, it takes an infinite amount of time for an object to approach the event horizon, at which point the light coming from it is infinitely red-shifted. To the distant observer, the object, falling slower and slower, approaches but never reaches the event horizon. The object itself might not even notice the point at which it crosses the event horizon, and will do so in a finite amount of proper time."

This postulation must be false. If everything falling into a black hole appears to take an infinite amount of time to reach the horizon these things would be lit up like christmas trees. Not exactly black. So if one million spacecraft were sent into the event horizon we would see 1 million static spaceships around the horizon for ever. Discussion welcome.
 
  • #35
hubble_bubble said:
This postulation must be false.

I'm sure you'll be able to back that up with something other than your opinion, yes?

I'm waiting.
 
  • #36
phinds said:
I'm sure you'll be able to back that up with something other than your opinion, yes?

I'm waiting.

I will post any calculations. Of course.
 
  • #37
"From the point of view of an external observer, it takes an infinite amount of time for an object to approach the event horizon, at which point the light coming from it is infinitely red-shifted. To the distant observer, the object, falling slower and slower, approaches but never reaches the event horizon."

This is one of those brain-twisters. I agree with Hubble - that the statement above is incorrect. Doesn't seem likely that an object approaching a black hole would move slower - to an external observer - than it would approaching a planet, say. If we had a really good telescope and were able to watch the people inside a spacecraft approaching a black hole, we would see them moving slower and slower and their clock running slower and slower. But the spaceship itself, I believe, would proceed faster and faster into the abyss and disappear. If there were any way to watch a clock inside the event horizon (which there isn't), it would, for all practical purposes, have stopped - but until they were destroyed, any passengers still alive inside the event horizon would see the clock running normally.
 
  • #38
CCWilson said:
"From the point of view of an external observer, it takes an infinite amount of time for an object to approach the event horizon, at which point the light coming from it is infinitely red-shifted. To the distant observer, the object, falling slower and slower, approaches but never reaches the event horizon."

This is one of those brain-twisters. I agree with Hubble - that the statement above is incorrect.

And I'm sure that you, too, will be able to back this up with more than just your opinion.

Since you are both wrong, this is going to be interesting.
 
  • #39
Also it is believed that inside a black hole things would be destroyed quite quickly. Under various gravitational strengths it must be possible for life to survive. As long as the lifeform has developed under the gravity in question. A lifeform that has developed within the confines of a neutron star, think Robert L Forward's Dragon's Egg, would be quite at home within the confines of a black hole up until reaching the singularity. If time inside the singularity, instead of slowing, speeds up then it may take an infinitely long time for travelers to reach the singularity. The boundary for this change would be the event horizon itself. This would be a very strange world with little light available as all the waves would be traveling away from the observer in two directions. Visibilty would be restricted to the band of the collapsing spherical wavefront at either side of this observer. Any movement would be restricted due to the effects of the intense gravity. Thus space within this reference fram is effectively static and balanced by a modification of the speed of time.
 
  • #40
phinds said:
And I'm sure that you, too, will be able to back this up with more than just your opinion.

Since you are both wrong, this is going to be interesting.

Well concerning time dilation there has to be a balance. If you live slower approaching the speed of light what happens when approaching a singularity where light no longer behaves in the normal manner?
 
  • #41
Also we must remember that wave frequency should increase as we reach the singularity. This balances the frequency decrease at or near the speed of light. As this frequency increases we should get an energy band around the singularity. And to be even more controversial, this energy should be lost as darlk matter/energy emissions from the black hole at faster than light speeds.
 
  • #42
hubble_bubble said:
Well concerning time dilation there has to be a balance. If you live slower approaching the speed of light what happens when approaching a singularity where light no longer behaves in the normal manner?

You seem to completely misunderstand time dilation. If you fall into a black hole, then I see you time dilated as you approach the event horizon. I see you approaching the EH asymptotically and never reaching it. You, on the other hand, are not even aware that there IS an EH and you pass through it not noticiing a thing.

As for your statement about what happens at the singularity, that is useless speculation. "Singularity" means "the place where our models break down and we don't know WHAT is happening" so any statement about what photons do there is spreculation and in any even it doesn't matter since we can never observe it anyway.
 
  • #43
hubble_bubble said:
Also we must remember that wave frequency should increase as we reach the singularity. This balances the frequency decrease at or near the speed of light. As this frequency increases we should get an energy band around the singularity. And to be even more controversial, this energy should be lost as darlk matter/energy emissions from the black hole at faster than light speeds.

I REALLY have no idea what you are talking about here but it sure sounds like utter nonsense. FTL ? Really ?
 
  • #44
A way I believe dark matter could be detected would be to lower a mass to as near as absolute zero as possible and detect any energy released. This should be detected BEFORE the event that caused it.
 
  • #45
hubble_bubble said:
Also it is believed that inside a black hole things would be destroyed quite quickly. Under various gravitational strengths it must be possible for life to survive.

nonsense.

As long as the lifeform has developed under the gravity in question. A lifeform that has developed within the confines of a neutron star, think Robert L Forward's Dragon's Egg, would be quite at home within the confines of a black hole up until reaching the singularity.

Clearly you dont' understand tidal forces

If time inside the singularity, instead of slowing, speeds up then it may take an infinitely long time for travelers to reach the singularity. The boundary for this change would be the event horizon itself. This would be a very strange world with little light available as all the waves would be traveling away from the observer in two directions. Visibilty would be restricted to the band of the collapsing spherical wavefront at either side of this observer. Any movement would be restricted due to the effects of the intense gravity. Thus space within this reference fram is effectively static and balanced by a modification of the speed of time.

Nearly as I can tell this is just a bunch of words strung together as blather.
 
  • #46
hubble_bubble said:
A way I believe dark matter could be detected would be to lower a mass to as near as absolute zero as possible and detect any energy released. This should be detected BEFORE the event that caused it.

Once again, what appears to be just a string of words with no relationship to actual physics.
 
  • #47
phinds said:
I REALLY have no idea what you are talking about here but it sure sounds like utter nonsense. FTL ? Really ?

Why do you think it is so hard to detect.
 
  • #48
hubble_bubble said:
Why do you think it is so hard to detect.

Why do I think WHAT is so hard to detect?

EDIT: if you are talking about dark matter, then I have to ask, why did you suddenly bring dark matter into a discussion about black holes? You do realize, I hope, that there is zero relationship between the two.
 
  • #49
"If you fall into a black hole, then I see you time dilated as you approach the event horizon." Yes. As I said above, if we could see what's going on inside a spaceship approaching an event horizon, their clocks would appear to us to be running slowly. If those chaps inside the ship could see us, an external observer, our clocks would appear to them to be running fast. That's time dilation. It sure doesn't mean that something approaching an event horizon moves more slowly. The opposite is true. As to what we would see as an object approaches the event horizon, I believe that we would see a redshifted image of it and then it would become invisible almost immediately. Now maybe there would theoretically be a prolongation of the image but the intensity would fall off rapidly so that it would not be visible very long. Regardless, the object will pass through the event horizon quickly; we might be able to see images of it for a short time, but that's just a quirk of observation. The actual object, from our point of view, is quickly in the clutches of the black hole; it's gone, baby, gone.
 
  • #50
Dark matter is hard to detect. If you look at galactic rotation curves they are flat. Unlike those of the solar system. As well as this implying dark matter driven rotation it also indicates that this dark matter must be spinning in the direction of galactic rotation. As dark matter is said to be expanding the universe then this implies that the dark matter is moving away from the galactic centre. Now what do you think may be theoretically at the galactic centre and spinning?
 

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