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B What's the deal with dark matter

  1. Dec 12, 2017 #41
    Possibly yet the frame drag of a rapidly spinning black hole could affect the orbit of a galaxy if the black hole is super massive in combination with an extreme magnetic field is present as well. ??
     
  2. Dec 12, 2017 #42
    If no consideration to a magnetic field that may be interacting with said frame drag. I admit it can be calculated based on current observational assumptions to be small and non pervasive however I’d like to add that we have yet to observe a black hole and to this point in time have only observered what could be explained as the result of a black hole. The inferences do get better but still no observations.
     
  3. Dec 12, 2017 #43

    ohwilleke

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    The latest measurements of magnetic fields around black holes show them to be surprisingly small. And, a supermassive black hole is a tiny fraction of the total mass of a galaxy, although it is fascinating how strictly corollated central supermassive black hole size and total galaxy size are empirically.
     
  4. Dec 12, 2017 #44

    Drakkith

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    What do you consider to be an "observation" of a black hole?
     
  5. Dec 28, 2017 #45

    Chronos

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    What we know is the universe is awash with regions of apparently empty space that behave as if occupied by large quantities of gravitating mass or pockets of the stress energy tensor. These regions tend to occur in the vicinity of large amounts of otherwise detectable mass, like galaxies and galactic clusters. Attempts to identify or detect constituent amounts of anything that may account for this phenomenon have been inconclusive. That pretty much sums what we can say with confidence about the current state of dark matter.
     
  6. Dec 28, 2017 #46

    ohwilleke

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    I would say we know quite a bit more than that. We have a lot of data about the inferred distribution and dynamics of dark matter if that is what it is, in relation to visible matter, which make it possible to rule out myriad models for it. We don't know just what is causing this phenomena, but we know pretty definitively that lots of possibilities that have been considered are not the answer.

    One of the really encouraging things about the search for the explanation of dark matter phenomena, unlike so many other unsolved problems in physics, is that we have rich data with regard to this one and both that data and our ability to analyze it are growing rapidly.

    This is very different from, for example, the search for experimental evidence of supersymmetry or other high energy "new physics" where we have nothing but a bunch of null results, anomalies that haven't panned out, and a huge area of the parameter space at high energies that it will be impossible as a practical matter to explore experimentally for decades or even ever.

    For example, observations by RAVE of Milky Way stars outside the plane in which most of the Milky Way's stars are found, can directly confirm or falsify lots of hypothetical solutions that otherwise reproduce the overall rotational dynamics of the Milky Way.

    Similarly, observations of colliding galaxies like the Bullet Cluster, similarly impose really meaningful constraints on models that can be cross checked against other similar colliding galaxy systems.

    The very systemic differences in this phenomena among galaxies that are of a particular type, and between different kinds of galaxies, and in galaxy clusters, all of which we have large data sets of, provide both overwhelming evidence that some kind of new physics or other is going on and constrains what the new physics can be.

    By dint of simple hard work and cumulative data collection by many independent investigators, this is one unsolved problem upon which we are making real progress on a regular basis, even if it doesn't always seem like that.
     
    Last edited: Dec 28, 2017
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