What is the current evidence for dark matter?

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Discussion Overview

The discussion revolves around the nature of dark matter, exploring various hypotheses regarding its composition and interaction with gravity. Participants examine whether dark matter could be related to particles within protons and neutrons, the implications of vacuum energy, and the evidence supporting dark matter's existence through gravitational lensing and other observations. The scope includes theoretical considerations, speculative ideas, and references to current research.

Discussion Character

  • Exploratory
  • Debate/contested
  • Technical explanation
  • Conceptual clarification

Main Points Raised

  • Some participants propose that dark matter could be particles that pop in and out of existence within protons and neutrons, questioning the nature of these particles.
  • Others argue that such particles are already accounted for as binding energy and mass, and that the concept of vacuum energy relates to dark energy rather than dark matter.
  • A participant mentions that dark matter's distribution is derived from gravitational lensing observations and the movement of stars in galaxies, suggesting it exists where ordinary matter is sparse.
  • There is mention of WIMPs (Weakly Interacting Massive Particles) as the leading theory for dark matter, with references to negative results from the LUX experiment.
  • Some participants speculate that dark matter might not be matter at all, but rather a force interacting with gravity, though this idea is challenged as unsupportable personal speculation.
  • Discussion includes the nature of gravity, with some participants asserting that gravity is not a particle and questioning how dark matter interacts gravitationally if it is not matter.
  • Concerns are raised about the possibility of dark matter being a modification of gravity or an undiscovered force, with references to existing theories and evidence supporting dark matter's existence.
  • A participant seeks clarification on whether dark matter is clumped around galaxies or distributed in intergalactic space, suggesting implications for unaccounted mass in the universe.

Areas of Agreement / Disagreement

Participants express multiple competing views regarding the nature of dark matter, with no consensus reached on its composition or the validity of various hypotheses. Some ideas are challenged as speculative, while others are supported by references to current research.

Contextual Notes

Limitations include unresolved assumptions about the nature of dark matter and the definitions of terms like "force" and "matter." The discussion reflects ongoing debates in the field without definitive conclusions.

  • #31
Discussion from the MoND guy.
http://www.astro.umd.edu/~ssm/mond/moti_bullet.html
We have known for some fifteen years now that MOND does not fully explain away the mass discrepancy in galaxy clusters. (See e.g. the 1999 paper by Sanders: http://xxx.lanl.gov/abs/astro-ph/9807023, but there have been quite a few others discussing this before and after, starting from 1988). Even after correcting with MOND you still need in the cluster some yet undetected matter in roughly the same amount as that of the visible matter. Call it dark matter if you wish, but we think it is simply some standard matter in some form that has not been detected.
 
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  • #32
kye said:
Is the collision separation phenomenon 100% proof of dark matter? if so, why is that some scientists still doubt their existence.. even astrophysicists... and they even have data that suggest it is opposite to dark matter predictions. see:

http://www.sciencedaily.com/releases/2009/05/090505061949.htm

any familiar with what they are talking about?
There's no such thing as 100% proof. But it is compelling evidence that makes MOND-type theories hard to support. The CMB is even more compelling evidence, but that's a little bit more difficult to wrap your head around as to precisely why.

kye said:
Here's more recent the suggest MOND is more appropriate.. so how does it still support dark matter?

http://www.sciencedaily.com/releases/2011/02/110223092406.htm
The claim here still requires a form of dark matter to fit the data. In this case, they use an undetected heavy species of neutrino in the fit (we know the three neutrinos we know about can't have that much mass). So they have a much more complicated model than just having dark matter: they've got both dark matter and modified gravity. Occam's Razor suggests that this is rather unlikely.
 

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