Quantised Inertia: A Solution to Dark Matter and Galaxy Rotations

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Discussion Overview

The discussion centers on the concept of quantised inertia as a potential solution to dark matter and the observed rotation of galaxies. Participants explore the theoretical underpinnings of quantised inertia, its implications for galaxy dynamics, and its predictions regarding galaxy clusters and cosmic acceleration.

Discussion Character

  • Exploratory
  • Technical explanation
  • Debate/contested
  • Mathematical reasoning

Main Points Raised

  • Some participants highlight that quantised inertia, or MiHsC, claims to explain galaxy rotation without dark matter by predicting rotational acceleration based solely on visible baryonic matter.
  • Others argue that the model's validity hinges on its ability to match galaxy cluster data, which they feel is not adequately addressed in the original paper.
  • One participant questions the use of proper acceleration in the context of galaxy edges, suggesting that coordinate acceleration might be more appropriate.
  • There is a discussion about the definitions of the Hubble radius and the particle horizon, with some participants seeking clarification on their usage in the context of quantised inertia.
  • A participant raises a question about the significance of Unruh radiation in affecting the inertial mass of gravitationally bound objects, suggesting it may be dynamically equivalent to Hawking radiation.
  • Another participant challenges the claim that Unruh radiation can be considered dynamically equivalent to Hawking radiation, asking for references to support this assertion.
  • Concerns are raised regarding the strength of Unruh radiation at ordinary accelerations and its implications for the predictions made by quantised inertia.
  • Participants engage in a technical debate about the relationship between the Hubble radius and the cosmic event horizon, with differing interpretations of their significance in cosmological models.

Areas of Agreement / Disagreement

Participants express a range of views, with some supporting the potential of quantised inertia while others remain skeptical, particularly regarding its applicability to galaxy clusters and cosmic microwave background data. The discussion remains unresolved with multiple competing perspectives on the validity and implications of the model.

Contextual Notes

There are limitations in the discussion regarding the definitions of terms like proper acceleration, coordinate acceleration, Hubble radius, and particle horizon, which are not uniformly agreed upon. Additionally, the relationship between Unruh radiation and Hawking radiation is debated without consensus.

  • #31
timmdeeg said:
Could you kindly clarify?

"Blackbody radiation" is just another way of saying "thermal radiation at some temperature", where in the case of the Unruh effect the temperature depends on the proper acceleration of the observer.
 
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  • #32
Hopefully I got it. If you say "an inertial observer watching the process would describe it as radiation ..." this doesn't imply that he observes it. Correct? Otherwise it seems that Wikipedia is wrong.
 
  • #33
timmdeeg said:
If you say "an inertial observer watching the process would describe it as radiation ..." this doesn't imply that he observes it. Correct?

Wrong. The inertial observer does observe radiation--but he observes it being emitted by the accelerated detector, whereas the accelerated observer, moving along with the detector, observes it absorbing radiation (the Unruh radiation). In other words, the detector itself can't avoid changing the state of the quantum field when it detects radiation, and that state change is a "real" change, seen by all observers, though different observers will describe the change differently.

timmdeeg said:
Otherwise it seems that Wikipedia is wrong.

Yes. And this surprises you? :wink:

Basically, the Wikipedia article is ignoring the effect of the detector on the quantum field. Many informal descriptions of the Unruh effect do so as well. But that's not really correct. See above.
 
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  • #34
PeterDonis said:
Yes. And this surprises you? :wink:

Basically, the Wikipedia article is ignoring the effect of the detector on the quantum field. Many informal descriptions of the Unruh effect do so as well. But that's not really correct. See above.
Well, indeed, I had the impression that the inertial observer doesn't see any radiation for quite a wile, due to some sources. The more I'm thankful that you have clarified this matter!
 
  • #35
timmdeeg said:
Yes, I think this is the key point which was also mentioned by PeterDonis in #25.
No, I don't think so. PeterDonis was pointing out that proper acceleration is not, in fact, observer dependent.

I added to that that the proper acceleration for an object in free-fall is identically zero. Which means that the proper acceleration of all stars and galaxies is so close to zero that it can be considered negligible, thus there should be no noticeable Unruh radiation with which to cause the rotation curve effect suggested by McCulloch. He seems to have made the mistake of assuming the Newtonian acceleration would result in the Unruh effect, but this isn't the case.

It is perhaps interesting that using this as an effect leads to results that match observation better than MOND. But the model is probably a non-starter as the premise appears to be impossible. I figured there was such an explanation why this idea wouldn't work, as otherwise the model would probably have gained more traction among theorists. I just wasn't sure what that explanation was early in the discussion, and I think this is it.
 
  • #36
timmdeeg said:
Correct? Otherwise it seems that Wikipedia is wrong.

It's not wrong but it's a bit ambiguous. What is meant by "where an inertial observer would observe none" is merely "vacuum state". They don't attempt to reconcile the detection events on the accelerated detector with the vacuum state measured by the first. This is done, as was said, by realizing that according to the inertial observer the detector emits radiation and Unruh radiation makes sense. You can think of it as a quantum mechanical analogue of centrifugal force, which is something you have to include for consistency when writing Newton's laws in a noninertial frame.

That said, any phenomenon that you explain in a noninertial frame has to have a corresponding explanation in the inertial one, for consistency. There is no Rindler horizon for the inertial observer, so it can't impose any boundary conditions on the radiation (even if it made sense that horizons did this, and it doesn't). This is a serious problem.
 
  • #37
kimbyd said:
I added to that that the proper acceleration for an object in free-fall is identically zero. Which means that the proper acceleration of all stars and galaxies is so close to zero that it can be considered negligible, thus there should be no noticeable Unruh radiation with which to cause the rotation curve effect suggested by McCulloch.
Yes. As a layman I was confused by this approach. The observer dependence of Unruh radiation is a bit subtle as I realized here, but that it is due to proper acceleration isn't.
 
  • #38
LeandroMdO said:
It's not wrong but it's a bit ambiguous. What is meant by "where an inertial observer would observe none" is merely "vacuum state". They don't attempt to reconcile the detection events on the accelerated detector with the vacuum state measured by the first. This is done, as was said, by realizing that according to the inertial observer the detector emits radiation and Unruh radiation makes sense.
They should have mentioned the latter at least shortly. They didn't and I'm the best example what kind of misunderstanding it creates. :frown:
 

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