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does it destroy it or does it get sent back in time like movies suggest?
According to GR, the collapsing star that formed the black hole will continue to collapse inside the event horizon, turning into a singularity of infinite density, everything between the singularity and the event horizon is just empty space (aside from any objects that fall through the horizon later). A theory of quantum gravity would probably get rid of the singularity, replacing it by who-knows-what, but it's expected that quantum gravity would probably only differ significantly from GR at the Planck scale (when the collapsing star has crunched down to such a small size that it reaches the Planck density, perhaps), so at macroscopic distances from the point where GR predicts a singularity I think that means you'd probably see about the same things as would be predicted by GR plus ordinary quantum field theory.peter0302 said:I've actually wondered about this - does the black hole consist of matter or is it purely localized energy? Are there still quarks/other particles inside the black hole or are they an entirely different animal from anything in the standard model?
Quantum gravity may prevent the singularity from ever forming, but that really doesn't matter here. The spin of a black hole is a geometrical property of spacetime, so it doesn't matter if singularities exist or not. Black holes can still spin. One effect caused by the spin is that falling matter is dragged "sideways". The world line of a falling piece of matter is still "straight" (a geodesic) but a different set of lines are straight in this geometry.Wallis said:I presume conservation of momentum and angular momentum apply inside a black hole. If a black hole is to spin, it can't disappear to a singularity. A singularity has 0 radius (definition) so has 0 angular momentum (definition) therefore does not spin.
If a black hole is to spin, it must have a radius at the "singularity" in order to exert angular momentum. Don't go telling me 0 times infinity is going to give the exact right angular momentum for each black hole by magic... it's not going to convince me :-)
JesseM said:According to GR, the collapsing star that formed the black hole will continue to collapse inside the event horizon, turning into a singularity of infinite density, everything between the singularity and the event horizon is just empty space (aside from any objects that fall through the horizon later). A theory of quantum gravity would probably get rid of the singularity, replacing it by who-knows-what, but it's expected that quantum gravity would probably only differ significantly from GR at the Planck scale (when the collapsing star has crunched down to such a small size that it reaches the Planck density, perhaps), so at macroscopic distances from the point where GR predicts a singularity I think that means you'd probably see about the same things as would be predicted by GR plus ordinary quantum field theory.
But by "inside" do you mean everything inside the event horizon, or just the immediate neighborhood of the singularity? As I said, the region between the singularity is mostly empty space aside from anything that falls in after the black hole forms, and falling objects would continue to be made of the same materials behaving the same way, until they reached the singularity.peter0302 said:Thanks but that's not really my question. My question is, what is the "stuff" inside the black hole?
GR is not a quantum theory, it treats matter in a classical way and doesn't address any quantum concerns. If you want to talk about what's going on quantum-mechanically at the center of the black hole, you'd need a theory of quantum gravity, and as I said no one really knows what such a theory would say about the center once you reach the Planck scale (but I think most physicists would bet that you'd no longer have a singularity of infinite density...it might not be meaningful to talk about densities higher than the Planck density in quantum gravity).peter0302 said:a) An infinitely dense mesh of standard model particles (if so, why doens't the pauli exclusion principle apply?)
Yes, that's the one. That's what I meant when I said "A theory of quantum gravity would probably get rid of the singularity, replacing it by who-knows-what".peter0302 said:e) Unknown
I would not say that at all.peter0302 said:Gotcha. So in GR, we'd not worry about Pauli and we'd just say that the matter is packed infinitely tightly because the electrostatic and other forces are overtaken by gravity. But because of QM, we cannot reconcile that idea with the exclusion principle so we're not sure what the signularity is "made of."
Borek said:You can calculate Schwarzschild radius for any given density. That means that any volume of the space can be a black hole if it is contains enough matter. It may as well mean that the black hole is pretty huge (in terms of radius) but relatively light (in terms of mass). If the density inside is low anough matter inside should not differ much from what we observe around us. Could be we already are in the black hole
MeJennifer said:I would not say that at all.
You might want to read http://en.wikipedia.org/wiki/Chandrasekhar_Limitpeter0302 said:Care to elaborate?
Electron (and neutron) degeneracy pressure is a direct consequence of the Pauli exclusion principle, and the Chandrasekhar limit tells you that for sufficiently massive white dwarfs the electron degeneracy pressure is insufficient to overcome their gravity, so they collapse further into a neutron star. There is a similar limit to how large neutron stars can be before gravity overcomes neutron degeneracy pressure, beyond that point they'll collapse into black holes. Presumably as the star continues to collapse inside the event horizon, the degeneracy pressure continues to get higher and higher as the matter is packed more and more tightly, but the inward gravitational pull continues to become greater too. In the limit as you approach the singularity, I imagine the degeneracy pressure due to the exclusion principle would approach infinity, but the gravitational pull would approach infinity at an even greater rate so the matter would keep collapsing. Perhaps it would even be possible to deal with the exclusion principle by just treating it as a type of pressure which you could feed into the equations of GR--my understanding is that the stress-energy tensor does include a notion of pressure, although I'm not actually sure how free you are to let the pressure vary in any way you want (and I'm also not sure whether the degeneracy pressure would vary with compression in exactly the same way as more classical notions of pressure).peter0302 said:You might want to explain to me what that has to do with the composition of the singularity.
It's not a force like the four fundamental forces, as I understand it it's basically due to the fact that fermions can't occupy the same quantum state, so instead of each particle's wavefunction being able to be spread throughout the whole volume the position gets much more compressed to avoid overlapping too much with other particles, and because of the uncertainty principle this gives them a much greater range of momenta which increases the pressure. But where did you get the idea that degeneracy pressure doesn't increase in magnitude as matter is compressed? It does, the pressure is proportional to density raised to the 4/3 power, see here.peter0302 said:Except quantum physicists are pretty adamant that the PEP is not a force, and therefore it should not increase in magnitude as densities increase. Thus there is a serious conflict here unelss I'm smoking something.
peter0302 said:Thanks but that's not really my question. My question is, what is the "stuff" inside the black hole?
The degeneracy pressure, I thought, was due to the strong and electrostatic forces, not a "pauli exclusion" force or a "quantum" force.JesseM said:It's not a force like the four fundamental forces, as I understand it it's basically due to the fact that fermions can't occupy the same quantum state, so instead of each particle's wavefunction being able to be spread throughout the whole volume the position gets much more compressed to avoid overlapping too much with other particles, and because of the uncertainty principle this gives them a much greater range of momenta which increases the pressure. But where did you get the idea that degeneracy pressure doesn't increase in magnitude as matter is compressed? It does, the pressure is proportional to density raised to the 4/3 power, see here.
Nope, degeneracy pressure isn't due to any actual force, but due to the fact that the exclusion principle says the probability of multiple fermions occupying precisely the same quantum state (including same position) is zero, which as I understand it forces the fermions to occupy more distinct energy states (although I've also seen it explained in terms of each fermion's position becoming more confined so they avoid overlapping, which increases their range of momenta via the uncertainty principle...I'm not sure if this second conceptual explanation makes sense, and if it does how it would relate to the first one, but maybe it has something to do with the fact that momentum and energy commute and that for a bound particle in a potential well, each energy level is associated with a particular momentum level). The article I linked to in my last post has a decent-looking explanation, and you can also see that page 86 of this textbook says the same thing, as does p. 142 of this book, and this page.peter0302 said:The degeneracy pressure, I thought, was due to the strong and electrostatic forces, not a "pauli exclusion" force or a "quantum" force.
As matter enters a black hole, it is subjected to immense gravitational forces that cause it to be stretched and compressed until it reaches the singularity, the point of infinite density and zero volume. This process is known as spaghettification.
Once matter crosses the event horizon, the point of no return, it is impossible for it to escape a black hole. The intense gravity of the black hole prevents even light from escaping, hence the name "black" hole.
The intense gravitational forces inside a black hole will break down matter into its fundamental particles. However, the matter is not destroyed but instead continues to exist in a highly compressed state within the singularity.
According to Einstein's theory of relativity, time is affected by the presence of a massive object such as a black hole. As matter gets closer to a black hole, time appears to slow down for an outside observer, and ultimately stops at the event horizon.
It is currently impossible to observe what happens to matter inside a black hole, as the intense gravity and distortion of space and time make it impossible for any information to escape. However, scientists can study the effects of black holes on their surroundings and make predictions based on mathematical models.