Dark matter, dark energy, and the Kerr metric?

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Discussion Overview

The discussion revolves around the concepts of dark matter and dark energy, particularly in relation to the Kerr metric and its implications for understanding the universe's structure and expansion. Participants explore the potential connections between these phenomena and question the adequacy of current models, such as Newtonian mechanics and MOND, in explaining observations at cosmic scales.

Discussion Character

  • Debate/contested
  • Exploratory
  • Technical explanation

Main Points Raised

  • Some participants express skepticism about the existence of dark matter and dark energy, questioning the validity of a universe composed of 95% unknown substances.
  • There are suggestions that the equations of motion may be incorrect, with references to alternative theories like MOND, though some find MOND arbitrary.
  • Participants propose the idea of a Kerr metric for spinning supermassive black holes potentially contributing to dark matter or dark energy effects, particularly with a varying cosmological constant.
  • Some argue that the Kerr metric describes local effects while the cosmological constant describes global effects, suggesting limited connection between the two.
  • Concerns are raised about the mass of black holes being insufficient to account for dark matter effects, with estimates indicating they comprise only about 2% of a galaxy's mass.
  • Frame dragging is discussed as a potential effect of rotating black holes, but some participants assert that it is a local effect and cannot account for dark matter on galactic scales.
  • There are conflicting views on whether frame dragging could have broader implications beyond local effects, with some participants questioning the assumptions behind these claims.
  • Neutrinos are mentioned as particles with properties similar to dark matter, but participants acknowledge that they do not fulfill the requirements for dark matter.

Areas of Agreement / Disagreement

Participants express multiple competing views regarding the nature and implications of dark matter and dark energy, with no consensus reached on the connections to the Kerr metric or the adequacy of current models.

Contextual Notes

Participants highlight limitations in understanding dark matter and dark energy, including the dependence on definitions and the unresolved nature of the mathematical implications of varying cosmological constants.

Imax
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I’m sorry, but I find dark matter and dark energy problematic. It’s hard to think of a Universe made up of about 95 % of stuff we have no idea about, except that maybe dark matter and dark energy have some properties.

So I’m thinking maybe there’s something wrong with the data, but I can’t see it. The Universe is expanding, and that expansion seems to be accelerating with time.

Maybe the equations of motion are wrong? Maybe Newtonian Mechanics is not the best way of be describing the Universe on a supper massive scale, something like MOND. But MOND doesn’t do it. It seems arbitrary with little insight.

So this is where I’m at. Almost every spiral galaxy has a supper massive black hole, weighing in at about a million to a billion times the mass of our sun. It’s about 10% the mass of a galaxy. The Schwarzschild radius for a super massive black hole is huge, something like the radius of our solar system. But, the average density over volume is low, not much different than the density of water.

Can some of that dark matter/dark energy come about from a Kerr metric for a spinning supper massive black hole, where Einstein’s cosmological constant is not zero? What could happen with a Kerr like metric, where the cosmological constant can vary? Is there a value which could keep galaxies together, at least for a short time?
 
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Imax said:
I’m sorry, but I find dark matter and dark energy problematic. It’s hard to think of a Universe made up of about 95 % of stuff we have no idea about, except that maybe dark matter and dark energy have some properties.
I suppose nobody is very happy about it.

Imax said:
Can some of that dark matter/dark energy come about from a Kerr metric for a spinning supper massive black hole, where Einstein’s cosmological constant is not zero?
Kerr metric describes gravity around rotating black hole where cosmological constant describes average "antigravity" of the whole universe.
So your statement does not make much sense, at least for me.
Dark matter problem is more about how gravity changes from place to place around galaxy then about some overall missing mass in galaxy. So again it does not make sense.

Imax said:
What could happen with a Kerr like metric, where the cosmological constant can vary? Is there a value which could keep galaxies together, at least for a short time?
Kerr metric describes local effects where cosmological constant describes global effect. There isn't too much connection between the two.

If you assume uneven distribution of dark energy at galaxy scales maybe it can provide some interesting approaches to dark matter problem but it seems that you are asking about something different.
 
Imax said:
Can some of that dark matter/dark energy come about from a Kerr metric for a spinning supper massive black hole, where Einstein’s cosmological constant is not zero? What could happen with a Kerr like metric, where the cosmological constant can vary? Is there a value which could keep galaxies together, at least for a short time?
Black holes only make up at most about 2% of the mass of a galaxy. So no, they don't have anywhere close to enough mass to so dramatically change our equations. Furthermore, whatever the solution to Einstein's equations for a black hole in the presence of a cosmological constant, it must approach the result for a cosmological constant in the limit of large distances. So I don't see how your proposal is any different than just proposing a cosmological constant in the first place, which is the leading candidate for the solution to the accelerated expansion.

I don't see why so many people are so opposed to dark matter, though. I mean, we already know of particles that have many of the same properties required for dark matter: neutrinos. Neutrinos don't fit the bill, of course, but that doesn't mean that other, higher-energy particles that are too massive to have yet been detected in particle accelerators won't.
 
Imax said:
It’s hard to think of a Universe made up of about 95 % of stuff we have no idea about, except that maybe dark matter and dark energy have some properties.

Well that's a little egocentric of you!
 
'Dark' matter and 'dark' energy are unrelated. Cosmologists are fully aware of this fact. Attempting to connect the two is a symantics fallacy.
 
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zonde said:
Kerr metric describes gravity around rotating black hole where cosmological constant describes average "antigravity" of the whole universe.
Ok, the cosmological constant describes an average "antigravity" of the whole universe, dark energy. So, maybe dark energy can’t be described by a Kerr metric with a varying cosmological constant, but what about dark matter and the Kerr metric?

I see a black hole as having mass, but it also has rotation. That rotation will induce frame dragging. Can some dark matter come from frame dragging of a suppermassive black hole at the center of galaxies?
 
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Imax said:
Ok, the cosmological constant describes an average "antigravity" of the whole universe, dark energy. So, maybe dark energy can’t be described by a Kerr metric with a varying cosmological constant, but what about dark matter and the Kerr metric?
You do realize that a varying cosmological constant is a contradiction in terms, right?

Imax said:
I see a black hole as having mass, but it also has rotation. That rotation will induce frame dragging. Can some dark matter come from frame dragging of a suppermassive black hole at center of galaxies?
No, frame dragging is a local effect, and the masses of the black holes at the centers of galaxies are far, far too small to do anything of the sort.
 
What if frame dragging is not a local effect, but has an effect on galactic proportions?
 
Imax said:
I see a black hole as having mass, but it also has rotation. That rotation will induce frame dragging. Can some dark matter come from frame dragging of a suppermassive black hole at the center of galaxies?
Qualitatively it has the same effect. But of course if quantitatively it can not account for considerable part (or all) of dark matter effect it would not be very interesting.
 
  • #10
Imax said:
What if frame dragging is not a local effect, but has an effect on galactic proportions?
Again: mass is way too small. The black holes at the centers of galaxies max out at roughly 2% of the visible mass, while the dark matter is around ten times the mass of the stars (or more).
 
  • #11
Chalnoth said:
Again: mass is way too small. The black holes at the centers of galaxies max out at roughly 2% of the visible mass, while the dark matter is around ten times the mass of the stars (or more).


Thanks Chalnoth, for putting these two in perspective.

It would be great if we could get some actual dark matter in the lab to find out what it is made of. Doesnt homogeniety require that there is at least some dark matter here and everywhere?

Thinking about it I guess we don't really know what the matter in black holes is made of either now that it is compressed almost to a true singularity.
 
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  • #12
Think of a poll of water, with no motion. Add a spinning sphere. Eventually, with enough time, matter will begin to rotate, and that rotation will be independent of gravity.
 

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