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If dark matter really lives up to it's name and truly is some form of matter, then wouldn't it feed black holes given extreme gravitational regime in a black hole?
Dark matter only interacts gravitationally, so it has trouble losing energy, so the cross-section for capture of dark matter by a black hole is much smaller than for normal matter. But yes, it can be swallowed by a black hole like anything else.ToddM4 said:If dark matter really lives up to it's name and truly is some form of matter, then wouldn't it feed black holes given extreme gravitational regime in a black hole?
It doesn't particularly accumulate, that's the point. To accumulate it needs some mechanism to dump kinetic energy, which ordinary matter does by collision. But dark matter is (near) collisionless, which is why it forms diffuse halos around galaxies.ToddM4 said:I presume it's difficult to test since dark matter doesn't emit light so we can't see it accruing near a black hole's horizon?
It's written on the label!Vanadium 50 said:If I have a black hole of mass M, how do I know how much of M was originally ordinary matter and how much was originally dark?
I don’t. As has been mentioned already, dark matter lacks a way to radiate away energy and clump. This makes it relatively less abundant in matter-dense regions.ToddM4 said:I imagine there would've been plenty of dark matter that was very nearly on a collision course with the black hole.
If you could account for its entire history and track every bit of normal matter that fell in, sure. But the thing is older than the Earth and we've only just started to get blurry pictures of it. The data isn't there and can't ever be.ToddM4 said:Is there a way to observe Sgt A*, calculate it's size based on normal matter and derive how much dark matter it has swallowed?
Black holes are small. Even Sagittarius A* is only about twenty million kilometres across, less than twice the size of the Sun. You have to hit within 1.5 times that to fall in. It's a really small target on a galactic scale.ToddM4 said:imagine there would've been plenty of dark matter that was very nearly on a collision course with the black hole.
A black hole has the same gravitational attraction as a star of the same mass. From that point of view, the concept of an "extreme gravitational regime" is a misconception. It's only when you within where the surface of the star would have been that the gravity keeps increasing - but you would have crashed into the original star at that point in any case.ToddM4 said:If dark matter really lives up to it's name and truly is some form of matter, then wouldn't it feed black holes given extreme gravitational regime in a black hole?
Darn. I was hoping it would lead to clarifications on the JWST observations of black holes in the early Universe and their sizes.Ibix said:If you could account for its entire history and track every bit of normal matter that fell in, sure. But the thing is older than the Earth and we've only just started to get blurry pictures of it. The data isn't there and can't ever be.
In principle you could track its growth, but I suspect the error bars around how much normal matter it swallows (even if we get vastly better images) would be much larger than the supposed dark matter infall.
My point precisely by saying "extreme gravitational regime" as in: past the event horizon.PeroK said:A black hole has the same gravitational attraction as a star of the same mass. From that point of view, the concept of an "extreme gravitational regime" is a misconception. It's only when you within where the surface of the star would have been that the gravity keeps increasing - but you would have crashed into the original star at that point in any case.
That's irrelevant for dark matter "feeding the black hole". The dark matter would have to be local to get sucked in.ToddM4 said:My point precisely by saying "extreme gravitational regime" as in: past the event horizon.
If the black hole is moving through space, and that space is filled with dark matter, won't dark matter going past the horizon be feeding the black hole?PeroK said:That's irrelevant for dark matter "feeding the black hole". The dark matter would have to be local to get sucked in.
Reference please. For light, the max impact parameter for the geodesic to end up inside the horizon is ##3\sqrt{3}R_S/2## if I don’t misremember. That’s about 2.6 times the Schwarzschild radius.Ibix said:You have to hit within 1.5 times that to fall in.
Yes it will, but there won’t be so much dark matter for it to matter significantly.ToddM4 said:If the black hole is moving through space, and that space is filled with dark matter, won't dark matter going past the horizon be feeding the black hole?
Won't this allow for study on how dark matter interacts in extreme gravitational regimes?Orodruin said:Yes it will, but there won’t be so much dark matter for it to matter significantly.
I was just going with the photon sphere. You seem to have done an actual calculation.Orodruin said:Reference please.
How so?ToddM4 said:Won't this allow for study on how dark matter interacts in extreme gravitational regimes?
If it interacts gravitationally different from visible matter it might give us clues into the nature of dark matter, no?PeroK said:How so?
Let me expand on that: if dark matter is throughout our galaxy, and thus our solar system, and, we produce black holes at LHC, couldn't we study their expected evaporation due to visible matter and measure the properties of dark matter if the evaporation rate is different from what we normally would expect just with visible matter?ToddM4 said:If it interacts gravitationally different from visible matter it might give us clues into the nature of dark matter, no?
Cosmology would take some giant steps forward if we could recreate a galaxy at the LHC and study it in the lab - dark matter and all. Sadly, all attempts even to detect dark matter in the lab have failed. That's why some are now skeptical of its existence!ToddM4 said:Let me expand on that: if dark matter is throughout our galaxy, and thus our solar system, and, we produce black holes at LHC, couldn't we study their expected evaporation due to visible matter and measure the properties of dark matter if the evaporation rate is different from what we normally would expect just with visible matter?
Sure, but we can create tiny black holes in collisions at the LHC and study how fast they evaporate. If dark matter is matter that succumbs to the gravitational field of a black hole, with our solar system going through the galaxy, which implies going through dark matter, shouldn't we be able to measure the influence of dark matter on the evaporation of the tiny black holes?PeroK said:Cosmology would take some giant steps forward if we could recreate a galaxy at the LHC and study it in the lab - dark matter and all. Sadly, all attempts even to detect dark matter in the lab have failed. That's why some are now skeptical of its existence!
How long have you been working on black hole evaporation at the LHC?ToddM4 said:Sure, but we can create tiny black holes in collisions at the LHC and study how fast they evaporate.
Well, ChatGPT clarifies this one as well.ToddM4 said:Nevermind, it seems we didn't detect microscopic black holes @ the LHC.
https://cms.cern/news/search-microscopic-black-hole-signatures-large-hadron-collider#:~:text=No experimental evidence for microscopic,models that postulate extra dimensions.
I wonder if cosmic rays which happen at higher energies than those LHC can produce create microscopic black holes and thus test dark matter via evaporation.
Theoretically, cosmic rays with extremely high energies, such as those in the exa-electronvolt range, could, under certain models, produce microscopic black holes when they interact with particles in the Earth's atmosphere. This idea is based on some speculative extensions of certain theories, like extra dimensions in string theory.
However, it's important to note that this is highly speculative and not confirmed by experimental evidence. The energies required for such processes are far beyond what current particle accelerators can achieve, making it challenging to test these theories directly. As of my last knowledge update in January 2022, there hasn't been any experimental confirmation of microscopic black hole production through cosmic ray interactions.
I had my students do it as homework at some point. I guess that means I did it too since I had to know the correct answer.Ibix said:You seem to have done an actual calculation.
please don’t use ChatGPT as a source of information regarding advanced physics subjects. It is very prone to sounding authorative when in reality it has no clue whatsoever.ToddM4 said:Well, ChatGPT clarifies this one as well.
Is not a valid reference here.ToddM4 said:ChatGPT
There are models where this leaves a cosmological imprint 1 2. I'm sure their authors would agree with you!ToddM4 said:Still, wouldn't it be cool to test dark matter via microscopic black hole evaporation?
The bulk of the theoretical and observational work being done on this question involves predictions regarding how the properties of neutron stars (which also involve extreme gravitational effects) would be different (their so called "equation of state") if they had captured significant dark matter, estimates of how much dark matter neutron stars should have absorbed, and efforts to determine if observationally neutron star properties are a better fit to the with dark matter mixed in hypothesis or the without dark matter mixed in hypothesis.ToddM4 said:If dark matter really lives up to it's name and truly is some form of matter, then wouldn't it feed black holes given extreme gravitational regime in a black hole?
Dark matter is a form of matter that does not emit, absorb, or reflect light, making it invisible to current electromagnetic observational instruments. Its presence is inferred from its gravitational effects on visible matter, such as stars and galaxies. It is thought to make up about 27% of the universe's mass-energy content.
Scientists detect dark matter indirectly through its gravitational effects on visible matter, radiation, and the large-scale structure of the universe. Observations such as the rotation curves of galaxies, gravitational lensing, and the cosmic microwave background provide evidence for the existence of dark matter.
Extreme gravitational regimes refer to environments where gravitational forces are extremely strong, such as near black holes, neutron stars, or during the early moments of the universe. These regimes provide unique conditions to test theories of gravity and fundamental physics.
Dark matter interacts with extreme gravitational regimes primarily through gravity. In regions with intense gravitational fields, such as near black holes, dark matter can be influenced by the strong curvature of spacetime. However, dark matter does not interact electromagnetically, so its behavior in these regimes can differ significantly from that of normal matter.
Several theories attempt to explain dark matter, including Weakly Interacting Massive Particles (WIMPs), axions, and sterile neutrinos. Each of these hypothetical particles has different properties and interactions. Additionally, some alternative theories, like Modified Newtonian Dynamics (MOND) and theories of modified gravity, propose changes to our understanding of gravity to account for the effects attributed to dark matter.