Einstein–de Sitter universe
The Einstein–de Sitter universe is a model of the universe proposed by Albert Einstein and Willem de Sitter in 1932. On first learning of Edwin Hubble's discovery of a linear relation between the redshift of the galaxies and their distance, Einstein set the cosmological constant to zero in the Friedmann equations, resulting in a model of the expanding universe known as the Friedmann–Einstein universe. In 1932, Einstein and De Sitter proposed an even simpler cosmic model by assuming a vanishing spatial curvature as well as a vanishing cosmological constant. In modern parlance, the Einstein–de Sitter universe can be described as a cosmological model for a flat matter-only Friedmann–Lemaître–Robertson–Walker metric (FLRW) universe.
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Einstein–de Sitter universe
The Einstein–de Sitter universe is a model of the universe proposed by Albert Einstein and Willem de Sitter in 1932. On first learning of Edwin Hubble's discovery of a linear relation between the redshift of the galaxies and their distance, Einstein set the cosmological constant to zero in the Friedmann equations, resulting in a model of the expanding universe known as the Friedmann–Einstein universe. In 1932, Einstein and De Sitter proposed an even simpler cosmic model by assuming a vanishing spatial curvature as well as a vanishing cosmological constant. In modern parlance, the Einstein–de Sitter universe can be described as a cosmological model for a flat matter-only Friedmann–Lemaître–Robertson–Walker metric (FLRW) universe.
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En cosmologie, l'espace d'Eins ...... ryonique) et de matière noire.
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L'univers d'Einstein–de Sitter ...... a ha esdevingut més important.
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The Einstein–de Sitter univers ...... dark energy became important.
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Unter einem Friedmann-Modell o ...... der kosmologischen Konstante .
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23,729,510
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1,022,908,526
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En cosmologie, l'espace d'Eins ...... ryonique) et de matière noire.
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L'univers d'Einstein–de Sitter ...... Walker mètric (FLRW) homogeni.
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The Einstein–de Sitter univers ...... Walker metric (FLRW) universe.
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Unter einem Friedmann-Modell o ...... der kosmologischen Konstante .
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Einstein-De Sittermodel
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Einstein–de Sitter universe
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Espace d'Einstein-de Sitter
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Friedmann-Modell
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Univers d'Einstein–de Sitter
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