What is the current evidence for dark matter?

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The discussion focuses on the nature of dark matter, emphasizing its distinction from ordinary matter and its gravitational interactions. Participants reference the Planck mission's findings, which indicate that dark matter constitutes approximately 26.8% of the universe's mass-energy content. The leading theoretical candidate for dark matter is Weakly Interacting Massive Particles (WIMPs), although recent LUX experiments have reported negative results. The conversation also touches on gravitational lensing as evidence for dark matter's existence and its clustering behavior, particularly in relation to galaxies and intergalactic space.

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  • Understanding of gravitational lensing and its implications for dark matter.
  • Familiarity with the standard model of cosmology and its components.
  • Knowledge of particle physics, specifically regarding WIMPs and vacuum energy.
  • Awareness of the Planck mission's contributions to cosmology.
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  • Research the implications of the LUX experiment findings on dark matter theories.
  • Explore the role of dwarf spheroidal galaxies in dark matter detection.
  • Investigate alternative theories to dark matter, including modifications to gravity.
  • Study the effects of dark energy in conjunction with dark matter in cosmological models.
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Astronomers, physicists, and students of cosmology interested in the latest discussions and theories surrounding dark matter and its implications for the universe's structure and evolution.

  • #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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