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I dont know much about the research done on this dark matter... all I know
its elusive, there is indirect evidence of it, and its what holds galaxies together... is it possible that this dark matter could be like a white dwarf except completely cooled down so its one big chunk of 'metals'? This could be why we cant see them as they are not glowing at all, they would be the same temperature (or near enough) to space itself and thats why our infrared telescopes haven't seen them... (or have we seen things that aren't hot or bright?) however they would have to be substantially small, relatively, that they wouldn't be detected when they pass our line of sight... I'm thinking it would be fairly small stars with a short life span... just a thought... Niko |
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"Niko Holm" wrote in
: I dont know much about the research done on this dark matter... all I know its elusive, there is indirect evidence of it, and its what holds galaxies together... is it possible that this dark matter could be like a white dwarf except completely cooled down so its one big chunk of 'metals'? This could be why we cant see them as they are not glowing at all, they would be the same temperature (or near enough) to space itself and thats why our infrared telescopes haven't seen them... (or have we seen things that aren't hot or bright?) however they would have to be substantially small, relatively, that they wouldn't be detected when they pass our line of sight... I'm thinking it would be fairly small stars with a short life span... just a thought... You have identified one of the two leading candidates for dark matter. Burned out small stars (ones too small to have gone nova) are called black dwarves, and stars too small to ever have ignited are called brown dwarves. Both of these objects, as well as other planetoids, planets and icy bodies like comets, fall under the general category of MACHO's - Massively Compact Halo Objects. The other leading candidate is massive neutrinos, including both the muon and tau varieties. These are called WIMP's - Weakly Interacting Massive Particles. There is experimental evidence to support meaningful contributions from both of these categories. Brown dwarves were first observed a few years ago, indirectly by means of the way they bent the light of nearby stars when they passed near the line of sight between us and that star. And experimental evidence for a neutrino mass was observed just this last year, when the solar neutrino problem was solved, although there is currently still no good estimate for the neutrino's mass. But I hate the dumb names that physicists have given these two categories of sources for the mass. These guys have gotta do better than that. |
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On Mon, 12 Jan 2004 09:01:19 +0800, "Niko Holm"
wrote: I dont know much about the research done on this dark matter... all I know its elusive, there is indirect evidence of it, and its what holds galaxies together... is it possible that this dark matter could be like a white dwarf except completely cooled down so its one big chunk of 'metals'? This could be why we cant see them as they are not glowing at all, they would be the same temperature (or near enough) to space itself and thats why our infrared telescopes haven't seen them... (or have we seen things that aren't hot or bright?) however they would have to be substantially small, relatively, that they wouldn't be detected when they pass our line of sight... I'm thinking it would be fairly small stars with a short life span... just a thought... The proportion of Baryons (protons, neutrons, etc.) in the universe is more or less known, so it's known that a substaintial portion of the dark mass of the universe is not "normal" matter but some other "non-interacting" particles. However a portion of dark matter is normal, much of that is actually just so hot that it emits X-rays rather than visible light. -- Robb McLeod ) A bus station is where a bus stops. A train station is where a train stops. On my desk I have a work station... |
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"Niko Holm" wrote in message ...
I dont know much about the research done on this dark matter... all I know its elusive, there is indirect evidence of it, and its what holds galaxies together... is it possible that this dark matter could be like a white dwarf except completely cooled down so its one big chunk of 'metals'? This could be why we cant see them as they are not glowing at all [...] This is a reasonable question, and the main motivation behind OGLE and similar projects. These stare at distant galaxies, watching for the gravitational lensing that occurs when a large body (glowing or not) comes close to the line of sight between us and one of the stars in the distant galaxy. This effect depends only on gravity, and so could detect the stars you mention. So far, their results show that at most 20% or so of the dark matter can be in the form of star sized bodies (otherwise they would see more events than they do). Lou Scheffer |
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