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Dark Matter's Profile Discovered?

pingbak writes "According to New Scientist, astronomers may have potentially discovered dark matter's EM profile (story). For the rest of us, this means astronomers may have just discovered all of the extra force holding the galaxy(-ies) together, which is not currently explainable though gravity and black holes at the center of universes alone. Since dark matter doesn't interact with ordinary matter, it's almost directly undetectable -- but now, physics and astronomy may just have had an awesome breakthrough. Nobel Prize material if it proves correct!"

7 of 83 comments (clear)

  1. Dark Matter Explaination? by Randolpho · · Score: 4, Interesting

    Um... perhaps I'm very much misinformed, which is entirely possible, but the article submission makes the claim that Dark Matter doesn't interact with regular matter.

    WTF? I thought the reason we're looking for Dark Matter is because the matter we *know* about doesn't add up to cause the gravetic interactions that we can observe. I thought Dark Matter was just matter we couldn't observe just yet, not some exotic "doesn't work the same as other matter" matter.

    Am I totally wrong here?

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    1. Re:Dark Matter Explaination? by CheshireCatCO · · Score: 5, Interesting

      They've looked pretty hard and carefully for normal, baryonic matter to cause the effects. So far, little has turned up.

      On the other hand, it's pretty clear at this point that dark matter in *some* form must exist. It's just a simple grasp of gravity coupled with some weird observations that lead to this conclusion. It is, in fact, very similar to the way Neptune was discovered. First, notice something odd about Uranus's orbit, then realize that another planet at position X could explain it. Just do it with galaxies and clusters, instead, and you start to suspect there's dark matter out there. Do some surveys and find that there doesn't appear to be enough brown dwarfs and black holes to make up the needed mass.

      To be honest, while I'm a planetary scientist and thus obligated to make fun of cosmologists, I don't find dark matter, even heretofore undiscovered particles, that hard to believe. Not only is the evidence pretty good, it isn't difficult to imagine that we've only scratched the surface of what is out there. You suggest that we're just finding "what's out there" (a claim with which I might quibble). So why is hard to believe that we haven't found all of the particles in the subatomic zoo? Especially given that the ones we seek are, by definition, difficult to find.

      And if you want "too convoluted to be natural", study quantum mechanics. It seems the universe doesn't care what we consider to be "natural", after all.

      (And now, a few quibbles: the SNP was only recently really clinched with lab data, but people had speculated about the solution, neutrino oscillations, for quite a while before hand. The same is true of a lot of what HST and others have told us in the past decade: usually, they're helping refine our models and confirm our best guesses as to what's out there. So it isn't like astronomers a decade ago would be shocked at what we've learned.)

  2. a little from column A, a little from... by bscott · · Score: 4, Interesting

    What they mean by "weakly interacting" is similar to how neutrinos are described - it doesn't have much of an electromagnetic impression, so it doesn't block light or smack into a detector in an earthbound observatory. Unlike neutrinos, it does posess a significant mass and is affected by gravity. And while that is "exotic", astrophysicists were only forced to consider this sort of thing when all previous efforts to explain some pretty obvious mis-matches in the numbers didn't work.

    Now I'll let someone else explain about "dark energy"...

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  3. Electronium? by 4of12 · · Score: 3, Interesting

    IANAHEP, but is there anypossibility that an electron and a positron could orbit one another with a reasonably long half-life?

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    1. Re:Electronium? by barawn · · Score: 4, Interesting

      Positronium.

      It has a half-life of 0.1 uS. It's a relatively standard physics problem at the graduate school level to ask what the binding energy of positronium is.

      If it ever comes up, it's (1/2) the binding energy of a hydrogen atom. The reasoning is simple - a positron and a proton have the same charge, but a positron and an electron have the same mass, so the "reduced mass factor" is 1/2, rather than 1. (M_p/(m_e+m_p) ~= 1) vs (M_e/(m_e+m_e) = 1/2).

  4. Neutrino's Big Cousin -- conclusions by pbhj · · Score: 3, Interesting

    In the conclusions they appear to be saying that some new interaction is happening due to ('mediated by') exchange of a light gauge boson (translation: low-energy force-carrying integer-spin-particle)

    Alternatively a new heavy fermion (neutrinos are fermionic, spin-1/2) mediates in the interaction: their words "could be responsible". So you might not be far off (if there second guess is correct).

    Start talking Nobel prizes when CERN/Fermilab find either of these particles.

    [... I've not done any particle physics for 5 years so this could be baloney.]

  5. Re:I don't get it by Royster · · Score: 3, Interesting

    There have been two leading candidates for dark matter: WIMPs and MACHOs. Each camp have had their proponents.

    WIMPS: Weakly Interacting Massive Particles. Neutrinos on steriods. Since they only interact through the weak and gravitational forces, they are by definintion dark in EM. But, we haven't found any in colliders.

    MACHOs: MAssive Cosmic Halo Objects. You're describing MACHOs. Ordinary, cold, dark matter. But there's probably too much of it to be this. It should have been swept up into stars.

    Frankly, I think that the energy levels detected will prove to be not what we're seeking here. It's too much of a coincidence that it is the e/e-bar annilation energy. OTOH, if there were a WILP which did have such a mass, we'd probably never see it thinking we were looking at e/e-bar reactions.

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