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Hot Dark Matter
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GKHP79COLFF
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Geliefert zwischen Mi., 26.11.2025 und Do., 27.11.2025
Details
Hot dark matter is a hypothetical form of dark matter which consists of particles that travel with ultrarelativistic velocities. The best candidate for the identity of hot dark matter is the neutrino. Neutrinos have very small masses, and do not partake in two of the four fundamental forces, the electromagnetic interaction and the strong interaction. They do interact by the weak interaction, and gravity, but due to the feeble strength of these forces, they are difficult to detect. A number of projects, such as the Super-Kamiokande neutrino observatory, in Gifu, Japan are currently studying these neutrinos.Dark matter is matter that cannot be detected by electromagnetic radiation, hence dark. It is postulated to exist to explain how clusters and superclusters of galaxies formed after the big bang. Data from galaxy rotation curves indicate that around 90% of the mass of a galaxy cannot be seen. It can only be detected by its gravitational effect.Hot dark matter cannot explain how individual galaxies formed from the big bang.
Weitere Informationen
- Allgemeine Informationen
- GTIN 09786130726706
- Editor Frederic P. Miller, Agnes F. Vandome, John McBrewster
- Genre Physik & Astronomie
- EAN 9786130726706
- Format Fachbuch
- Titel Hot Dark Matter
- Herausgeber Alphascript Publishing
- Anzahl Seiten 68
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