Success Stories 18|08
Efficient Product Development of Gears in Sun-Blinds
In astrophysics and cosmology, dark matter is a hypothetical form of matter that does not
emit or reflect enough electromagnetic radiation to be observed directly, but whose presence
can be inferred from gravitational effects on visible matter. According to present observations
of structures larger than galaxies, as well as Big
Bang cosmology, dark matter accounts for the
vast majority of mass in the observable universe.
Dark matter also plays a central role in structure
formation and galaxy evolution, and has
measurable effects on the anisotropy of the
cosmic microwave background. All these lines of
evidence suggest that galaxies, clusters of
galaxies, and the universe as a whole contain far
more matter than that which interacts with
electromagnetic radiation: the remainder is
called the "dark matter component. Determining
The Alpha Magnetic Spectrometer AMS.
the nature of this missing mass is one of the
most important problems in modern cosmology
and particle physics. > full story
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