[Home]History of Dark matter

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Revision 24 . . (edit) December 18, 2001 7:33 am by Taw [format fix]
Revision 23 . . December 18, 2001 7:30 am by (logged).126.156.xxx
Revision 22 . . December 18, 2001 7:28 am by (logged).126.156.xxx
Revision 21 . . December 18, 2001 7:27 am by (logged).126.156.xxx [copyedit]
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Revision 19 . . December 18, 2001 7:25 am by (logged).126.156.xxx [Latest developements]
Revision 18 . . November 21, 2001 3:26 am by Chenyu
Revision 17 . . November 21, 2001 3:22 am by Chenyu
Revision 16 . . (edit) November 19, 2001 2:01 am by Derek Ross [spelling]
  

Difference (from prior major revision) (minor diff, author diff)

Changed: 9,10c9,14
Since it cannot be detected via optical means, the composition of dark matter remains speculative. Large masses like galaxy-sized black holes can be ruled out on the basis of lensing data. Possibilities involving normal baryonic matter include [brown dwarf]?s or perhaps small, dense chunks of heavy elements. The
possible amount of baryonic dark matter is, however, restricted by [big bang nucleosynthesis]?. At present, though, the most common view is that dark matter is made of elementary particles other than the usual electrons, protons, and neutrons, such as neutrinos, axion?s, or WIMPs.
Since it cannot be detected via optical means, the composition of dark matter remains speculative. Large masses like galaxy-sized black holes can be ruled out on the basis of lensing data. Possibilities involving normal baryonic matter include [brown dwarfs]? or perhaps small, dense chunks of heavy elements. The
possible amount of baryonic dark matter is, however, restricted by [big bang nucleosynthesis]?. At present, though, the most common view is that dark matter is made of elementary particles other than the usual
electrons, protons, and neutrons, such as neutrinos, axions?, or WIMPs.

alternative explanations




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