Lemaître–Tolman metric
In mathematical physics, the Lemaître–Tolman metric is the spherically symmetric dust solution of Einstein's field equations. It was first found by Georges Lemaître in 1933 and Richard Tolman in 1934 and later investigated by Hermann Bondi in 1947. This solution describes a spherical cloud of dust (finite or infinite) that is expanding or collapsing under gravity. It is also known as the Lemaître–Tolman–Bondi metric or the Tolman metric.
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Dust solutionGeorges LemaîtreHermann BondiIndex of physics articles (L)Inhomogeneous cosmologyLTBLTB dustLTB dustsLemaitre-Tolman-Bondi metricLemaitre-Tolman metricLemaitre–Tolman metricLemaîtreLemaître-Tolman-Bondi metricLemaître-Tolman metricLemaître coordinatesLemaître–Tolman–Bondi metricMetric tensor (general relativity)Richard C. TolmanTolman metric
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Lemaître–Tolman metric
In mathematical physics, the Lemaître–Tolman metric is the spherically symmetric dust solution of Einstein's field equations. It was first found by Georges Lemaître in 1933 and Richard Tolman in 1934 and later investigated by Hermann Bondi in 1947. This solution describes a spherical cloud of dust (finite or infinite) that is expanding or collapsing under gravity. It is also known as the Lemaître–Tolman–Bondi metric or the Tolman metric.
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In mathematical physics, the L ...... i metric or the Tolman metric.
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Lemaître–Tolman-metrik (även L ...... ant och , exempelvis konstant.
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托尔曼度规（英語：Tolman metric）是描述能量-动量张量为流体的场的度规，是时间的函数。数学表示为：
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In mathematical physics, the L ...... i metric or the Tolman metric.
@en
Lemaître–Tolman-metrik (även L ...... öljer med dammpartiklarna. där
@sv
托尔曼度规（英語：Tolman metric）是描述能量-动量张量为流体的场的度规，是时间的函数。数学表示为：
@zh
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Lemaître–Tolman metric
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Lemaître–Tolman-metrik
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托尔曼度规
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