The Friedmann–Lemaître–Robertson–Walker metric (FLRW; /ˈfriːdmən ləˈmɛtrə ... /) is a metric based on an exact solution of the Einstein field equations...
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derived by Alexander Friedmann in 1922 from Einstein's field equations of gravitation for the Friedmann–Lemaître–Robertson–Walker metric and a perfect fluid...
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the Hubble–Lemaître law. The lunar crater Lemaître Friedmann–Lemaître–Robertson–Walker metric Lemaître coordinates Hubble–Lemaître law Lemaître observers...
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called the Friedmann–Lemaître–Robertson–Walker metric, or FLRW, after Friedmann, Georges Lemaître, Howard P. Robertson and Arthur Geoffrey Walker, who worked...
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Expansion of the universe (redirect from Metric expansion)
cosmology. It can be modeled mathematically with the Friedmann–Lemaître–Robertson–Walker metric (FLRW), where it corresponds to an increase in the scale...
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cosmological principle and assumed by all models that use the Friedmann–Lemaître–Robertson–Walker metric, including the current version of the ΛCDM model, or is...
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In physics, the Lemaître–Tolman metric, also known as the Lemaître–Tolman–Bondi metric or the Tolman metric, is a Lorentzian metric based on an exact...
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evolution of the scale factor in the Friedmann–Lemaître–Robertson–Walker metric is obtained solving the Friedmann equations: a ( t ) ∝ t 1 / 2 . {\displaystyle...
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Alcubierre metric, de Sitter/anti-de Sitter metrics, Friedmann–Lemaître–Robertson–Walker metric, Isotropic coordinates, Lemaître–Tolman metric, Peres metric, Rindler...
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Lemaître: Lemaître (crater), an impact crater on the Moon 1565 Lemaître, a minor planet the Friedmann–Lemaître–Robertson–Walker metric the Lemaître metric...
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horizon.[citation needed] The model uses the Friedmann–Lemaître–Robertson–Walker metric, the Friedmann equations, and the cosmological equations of state...
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computed by the following formula (derived using the Friedmann–Lemaître–Robertson–Walker metric): χ = ∫ t e t c d t ′ a ( t ′ ) {\displaystyle \chi =\int...
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is often visualized as curved spacetime. The Friedmann–Lemaître–Robertson–Walker metric is a curved metric which forms the current foundation for the description...
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Borde–Guth–Vilenkin theorem (section For FLRW metric)
space-time with no appeal to homogeneity or isotropy. The Friedmann–Lemaître–Robertson–Walker metric is given by d s = d t 2 − a 2 ( t ) d x i d x i {\displaystyle...
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a Big Bounce, or a Big Crunch. Cosmological constant Friedmann–Lemaître–Robertson–Walker metric High-Z Supernova Search Team Lambda-CDM model List of...
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( t ) {\displaystyle a(t)} is the scale factor of the Friedmann–Lemaître–Robertson–Walker metric, and we have taken the Big Bang to be at t = 0 {\displaystyle...
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the cosmological principle is correct, is the Friedmann–Lemaître–Robertson–Walker metric the right metric to use for our universe? Are the observations...
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was emitted, we may first note that according to the Friedmann–Lemaître–Robertson–Walker metric, which is used to model the expanding universe, if we...
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Rosen's universe is zero in any universe compliant with a Friedmann–Lemaître–Robertson–Walker metric, and proposed a mechanism of inflation-driven generation...
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\sum _{j=1}^{D-1}p_{j}^{2}={\frac {1}{D-1}}\neq 1.} The Friedmann–Lemaître–Robertson–Walker metric employed in cosmology, by contrast, is able to expand...
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kinematics of the observable universe, dependent on the Friedmann–Lemaître–Robertson–Walker metric but independent of the temporal dependence of the scale...
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described as a cosmological model for a flat matter-only Friedmann–Lemaître–Robertson–Walker metric (FLRW) universe. In the model, Einstein and de Sitter...
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cosmological principle and assumed by all models that use the Friedmann–Lemaître–Robertson–Walker metric, including the current version of the ΛCDM model, or is...
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Killing tensor (section FLRW metric)
tensors not simply obtained from Killing vectors. The Friedmann–Lemaître–Robertson–Walker metric, widely used in cosmology, has spacelike Killing vectors...
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decomposition of the most general linearized perturbations of the Friedmann–Lemaître–Robertson–Walker metric into components according to their transformations under...
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part of background metrics for some cosmological models; for example, the three cases of the Friedmann–Lemaître–Robertson–Walker metric may be represented...
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by Arthur Geoffrey Walker in 1936, and is today widely known in the United States as the Robertson–Walker metric. One of Robertson's landmark papers, a...
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matter) density of a substance and its pressure. In the Friedmann–Lemaître–Robertson–Walker metric, it can be shown that a strong constant negative pressure...
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In Einstein's theory of general relativity, the Schwarzschild metric (also known as the Schwarzschild solution) is an exact solution to the Einstein field...
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without major pitfalls. In practice, some metrics, notably the Friedmann–Lemaître–Robertson–Walker metric that appears to govern the universe, do not...
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