Photon dilemma for MOND-like dark matter

In summary, this paper discusses how superfluid dark matter in tension with weak gravitational lensing data may be problematic. The issue is roughly speaking this: if it's coupled to photons then it should scatter them but we don't see that, but if it's not then why are photons affected by its gravity like everything else? This affects the theory of modified gravity, which suggests that some kind of dark matter particle exists that has properties that reproduce MOND in some circumstances.
  • #1
mitchell porter
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TL;DR Summary
whether to couple or not
"Superfluid dark matter in tension with weak gravitational lensing data" (Mistele, McGaugh, Hossenfelder)

Regarding this paper, Sabine Hossenfelder tweets

It's about superfluid dark matter but highlights what I believe is a general problem of hybrid approaches.
The issue is roughly speaking this. You introduce a new field that reproduces modified gravity in some regime and CDM in some other regime. Question is, do you couple it to photons or not.
If you do couple it to photons you get a problem with reproducing observations from GW170817 that require photons to travel pretty much like gravitaitonal waves inside galaxies.
If you don't couple it to photons then kinematic measurements (inferred from the motion of stars and gas) will generically not match to lensing observations. Alas the data say they do.

One comment summarizes this as

"if it's coupled to photons then it should scatter them but we don't see that,
but if it's not then why are photons affected by its gravity like everything else"
 
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  • #2
does this affect modify gravity ?
 
  • #3
It is a dark matter particle hypothesis that has properties that reproduce MOND in some circumstances.
 
  • #4
Matter with a special kind of gravity that doesn't bend the path of light? Weird.
 
  • #5
What about bimetric theories, where different kinds of matter see different geometries?
 
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  • #6
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  • #7
Demystifier said:
What about bimetric theories, where different kinds of matter see different geometries?
I get the impression from Milgrom's paper arxiv:22209.10882 (linked above) that the two metrics are indeed intended to inhabit one spacetime. But I don't understand what the 2nd metric (Milgrom's "##\hat g_{\mu\nu}##") actually does in the geometry. He constructs 2 affine connections ##\Gamma^\lambda_{~\mu\nu}## and ##\hat \Gamma^\lambda_{~\mu\nu}##, then calls their difference $$C^\lambda_{~\mu\nu} ~:=~ \Gamma^\lambda_{~\mu\nu} ~-~ \hat \Gamma^\lambda_{~\mu\nu}$$ a "relative acceleration tensor" (see p3).
His footnote 4 at the bottom of p3 says:

Milgrom said:
The tensor ##C^\lambda_{~\mu\nu}## may be thought of as the "relative acceleration field", of ##g_{\mu\nu}## with respect to ##\hat g_{\mu\nu}##, in the sense that in a frame where ##\hat g_{\mu\nu}## is locally flat at some ##\hat x## [i.e., ##\hat \Gamma^\lambda_{~\mu\nu}(\hat x) = 0]##], we have ##d^2 x^\mu/d\tau^2 |_{\dot x} = -C^\lambda_{~\alpha\beta} \dot x^\alpha \dot x^\beta##, on a geodesic of ##g_{\mu\nu}## through ##\hat x##.
So (clearly?) the 2 metrics participate somehow in the same geometry (e.g., congruences of worldlines) on a base manifold.

This is (so far) not making much sense to me, but I'll keep reading... :oldfrown:
 
  • #8
strangerep said:
I get the impression from Milgrom's paper arxiv:22209.10882 (linked above) that the two metrics are indeed intended to inhabit one spacetime. But I don't understand what the 2nd metric (Milgrom's "##\hat g_{\mu\nu}##") actually does in the geometry. He constructs 2 affine connections ##\Gamma^\lambda_{~\mu\nu}## and ##\hat \Gamma^\lambda_{~\mu\nu}##, then calls their difference $$C^\lambda_{~\mu\nu} ~:=~ \Gamma^\lambda_{~\mu\nu} ~-~ \hat \Gamma^\lambda_{~\mu\nu}$$ a "relative acceleration tensor" (see p3).
His footnote 4 at the bottom of p3 says:

So (clearly?) the 2 metrics participate somehow in the same geometry (e.g., congruences of worldlines) on a base manifold.

This is (so far) not making much sense to me, but I'll keep reading... :oldfrown:
I am not sure what you call geometry here, and what exactly confuses you. The same manifold can have many metrics, that is not a problem. It is another question what they are for.
 
  • #9
martinbn said:
I am not sure what you call geometry here, and what exactly confuses you.
You picked up on that, huh? :oldsmile:

So,... do you feel that you understand Milgrom's paper well? If so, I'd appreciate a summary explanation of the bimetric MOND theory in your own words, since I've never found Milgrom to be good at explaining things clearly.

martinbn said:
The same manifold can have many metrics, that is not a problem. It is another question what they are for.
Indeed, the latter is what I'm struggling with, i.e., the correspondence between the math and the real-world physics.

Among other things, Milgrom says (1st para, p3) that the other metric ##\hat g_{\mu\nu}## couples to "twin matter", which is assumed not to interact directly with matter. So... "twin matter" is like "dark matter"??

Oh, but no, because... in footnote 10 on p13 he seems to contradict this when he says that, in the MOND regime, matter and twin-matter repel each other.
 
  • #10
Oh, no, you are far ahead. I gave up after the introduction. I was just curious if you had any mathematical objections.
 
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  • #11
martinbn said:
I was just curious if you had any mathematical objections.
I have none at this stage -- but I have not studied the gory detail in the depths. (If the physical correspondences are unclear/missing, I tend to lose interest.)
 
  • #12
I'm sure it's a common question, but wouldn't bimetric approaches have causality problems? It seems to me they would need to share the same null geodesics, else you could use the null geodesics of one metric to violate the causality of another. I guess the idea is you completely remove any interactions between the two species other than gravity, so the only way they communicate is by joint effects on each others' metrics, and each metric has its own null geodesics so causality is enforced. Is that the idea? If so, there could never be direct detection of dark matter, which probably means it will always seem like a speculative explanation. It would also seem to complicate unifying gravity with the other forces, because it seems like it really requires gravity as a metric effect but not as a force carrier, is that not so?
 
  • #13
Demystifier said:
What about bimetric theories, where different kinds of matter see different geometries?

Madeleine Birchfield said:
One of the authors of the paper, Stacy McGaugh, said on his blog that while he hasn't yet had time to read Milgrom's bimetric MOND paper, he hopes that some time in the future he could read Milgrom's paper

https://tritonstation.com/2023/03/06/ask-and-receive/

https://arxiv.org/abs/2208.10882

Update: Stacy McGaugh says that "My understanding is that photons do see the MOND effect in bimetric theories, so the same concern doesn’t apply."

https://tritonstation.com/2023/05/19/commentary-on-wide-binaries/comment-page-1/#comment-21286
 
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  • #14
There are a couple of threads on this. This is very interesting to arm chair viewers like my self.

This article today.

https://phys.org/news/2024-06-mond-dark-rotation-galaxies-stay.html

“Stacy McGaugh, professor and director of the Department of Astronomy in the College of Arts and Sciences,

said Mistele's findings, slated for publication in the Astrophysical Journal Letters, push traditional boundaries.”

Slated? Quite strong language.

Pre print here

https://arxiv.org/abs/2406.09685

@strangerep @Vanadium 50 and @ohwilleke have all been following this.
 
  • #15
pinball1970 said:
There are a couple of threads on this. This is very interesting to arm chair viewers like my self.

This article today.

https://phys.org/news/2024-06-mond-dark-rotation-galaxies-stay.html

“Stacy McGaugh, professor and director of the Department of Astronomy in the College of Arts and Sciences,

said Mistele's findings, slated for publication in the Astrophysical Journal Letters, push traditional boundaries.”

Slated? Quite strong language.

Pre print here

https://arxiv.org/abs/2406.09685

@strangerep @Vanadium 50 and @ohwilleke have all been following this.
I've blogged it. If true, the observation generically rules out almost all current dark matter particle theories. Sabine is impressed too.

I don't read anything into "slated" other than that someone was bored and grabbed a thesaurus.
 
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  • #16
pinball1970 said:
https://phys.org/news/2024-06-mond-dark-rotation-galaxies-stay.html

“Stacy McGaugh, professor and director of the Department of Astronomy in the College of Arts and Sciences,
said Mistele's findings, slated for publication in the Astrophysical Journal Letters, push traditional boundaries.”

Slated? Quite strong language.
It appears to have been published 20-Jun-2024 (open access).
 
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FAQ: Photon dilemma for MOND-like dark matter

What is the photon dilemma in the context of MOND-like dark matter?

The photon dilemma refers to the challenge of reconciling the behavior of photons in a framework where Modified Newtonian Dynamics (MOND) or MOND-like dark matter is proposed. In standard physics, photons are massless particles that travel at the speed of light. However, in MOND-like theories, the dynamics of gravity and light propagation can differ significantly from those predicted by General Relativity, leading to questions about how photons behave in regions of weak gravitational fields or accelerated frames.

How does MOND modify the traditional understanding of gravity?

MOND modifies the traditional understanding of gravity by introducing a new regime of gravitational interaction that becomes significant at low accelerations, which are typical in the outskirts of galaxies. Instead of following Newton's laws or General Relativity, MOND posits that the effective gravitational force experienced by an object is not linear with respect to the mass of the object, leading to different predictions for the motion of stars and gas in galaxies compared to classical theories.

What implications does the photon dilemma have for cosmology?

The photon dilemma has significant implications for cosmology, particularly in understanding the large-scale structure of the universe and the behavior of light from distant galaxies. If MOND-like theories alter the propagation of photons, this could affect our observations of cosmic microwave background radiation, gravitational lensing, and the distribution of dark matter, potentially leading to new insights or revisions of our current cosmological models.

Are there any observational tests that can distinguish MOND-like dark matter from conventional dark matter?

Yes, there are several observational tests that can help distinguish MOND-like dark matter from conventional dark matter. These include analyzing the rotation curves of galaxies, studying the dynamics of galaxy clusters, and examining the gravitational lensing effects around massive objects. Differences in predictions regarding the behavior of light and the distribution of mass can provide critical evidence for or against MOND-like theories.

What are the current challenges in resolving the photon dilemma?

The current challenges in resolving the photon dilemma include the lack of a comprehensive theoretical framework that unifies MOND-like modifications with the behavior of light, as well as the need for precise observational data to test these theories. Additionally, the complexity of gravitational interactions in different astrophysical contexts complicates the development of clear predictions that can be empirically validated, making it difficult to draw definitive conclusions.

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