cold dark matter การใช้

• "Mixed " dark matter is also called hot + cold dark matter.
• The rest is presumably mostly cold dark matter, unknown and so far undetectable.
• Predictions of the cold dark matter paradigm are in general agreement with astronomical observations.
• Many simulations simulate only cold dark matter, and thus include only the gravitational force.
• Fuzzy cold dark matter is a limit of scalar field dark matter without self-interaction.
• Dark matter, sometimes called " cold dark matter, " has been known for some time.
• The leading candidate for the dark matter until now, called cold dark matter, is simple.
• This model requires the presence of non-relativistic neutrinos or other cold dark matter, to work.
• Cold dark matter, moving slowly and clumping easily, would have produced too much galactic clustering.
• Yet there are still many questions that the cold dark matter model does not answer.
• This so-called cuspy halo problem is a persistent problem for the standard cold dark matter theory.
• But cold dark matter had some shortcomings.
• One is the world of cold dark matter; the other is the world of warm wet matter.
• This is the hypothetical cold dark matter.
• While the overall constraints are inconclusive, uncorrelated isocurvature cold dark matter modes are found to be unlikely.
• The remainder is believed to consist of 26.8 percent cold dark matter and 68.3 percent dark energy.
• The evidence for nonbaryonic cold dark matter is exceptionally flimsy, but it does seem to be entrenched.
• The most widely discussed models of nonbaryonic dark matter are based on the cold dark matter hypothesis.
• Relativistic dark matter is " hot dark matter " and nonrelativistic dark matter is " cold dark matter ".
• Simulations of a universe full of cold dark matter produce galaxy distributions that are roughly similar to what is observed.