Dark Matter

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In astronomy and cosmology, dark matter is hypothetical matter that is undetectable by its emitted radiation, 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 and dark energy could account for the vast majority of the mass in the observable universe. Dark matter is postulated to partially account for evidence of "missing mass" in the universe, including the rotational speeds of galaxies, orbital velocities of galaxies in clusters, gravitational lensing of background objects by galaxy clusters such as the Bullet Cluster, and the temperature distribution of hot gas in galaxies and clusters of galaxies. Dark matter is believed to play a central role in structure formation and galaxy evolution, and has measurable effects on the anisotropy of the cosmic microwave background.

Weitere Informationen

  • Allgemeine Informationen
    • GTIN 09786130214500
    • Editor Frederic P. Miller, Agnes F. Vandome, John McBrewster
    • Sprache Englisch
    • Genre Physik & Astronomie
    • Jahr 2009
    • EAN 9786130214500
    • Format Fachbuch
    • ISBN 978-613-0-21450-0
    • Titel Dark Matter
    • Untertitel Matter, Big Bang, Dark energy, Structure formation, Galaxy formation and evolution, Cosmic microwave background radiation, Fritz Zwicky, Virial theorem, Galaxy rotation curve
    • Herausgeber Alphascript Publishing
    • Anzahl Seiten 132

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