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Cold Dark Matter

  1. Sep 17, 2007 #1
    Why does cold dark matter imply a bottom-up scenario of structure formation? and why does hot dark matter imply a top-down scenario of structure formation?

    is it simply because cold dark matter is slow moving (non-relativistic) and slow moving things are more likely to clump together to form larger things because they possess less energy and momentum? or is there more to it?

    thank you in advance!
     
    Last edited: Sep 17, 2007
  2. jcsd
  3. Sep 17, 2007 #2

    mathman

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    I can't answer your question specifically. However, the various studies of cold vs. warm are made using computer simulations of how the universe would evolve after the big bang and comparing to what is observed.
     
  4. Sep 17, 2007 #3

    hellfire

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    This is due to damping of density perturbations. For collisionless particles the most important damping effect is the free streaming damping. Free streaming damping means that the gravitation of the density perturbations of those particles cannot bind them below their free streaming length, and therefore density perturbations smaller than this length cannot form. The free streaming length is the lenght that those particles can travel until they become non-relativistic. Heavy dark matter particles like CDM particles are assumed to become non-relativistic very early, having thus a small free streaming length. This, in turn, means that density perturbations on small scales can be formed leading to a bottom-up scenario of structure formation.
     
    Last edited: Sep 17, 2007
  5. Sep 18, 2007 #4
    if anyone knows of any papers at any level that i can read to understand free stream damping and its relationship to cold/hot dark matter better, please post them here.

    thank you!
     
  6. Sep 18, 2007 #5

    hellfire

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  7. Sep 18, 2007 #6
    i will read those. thanks much!
     
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