Cosmic acceleration: the second Friedmann equation (Q1544): Difference between revisions
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| Property / instance of: mathematical expression / rank | |||
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| Property / LaTeX source: \\frac{\\ddot a}{a} = -\\frac{4\\pi G}{3}\\left(\\rho + \\frac{3p}{c^2}\\right) + \\frac{\\Lambda c^2}{3} / rank | |||
| Property / instance of | |||
| Property / instance of: mathematical expression / rank | |||
Normal rank | |||
| Property / LaTeX source | |||
\\frac{\\ddot a}{a} = -\\frac{4\\pi G}{3}\\left(\\rho + \\frac{3p}{c^2}\\right) + \\frac{\\Lambda c^2}{3} | |||
| Property / LaTeX source: \\frac{\\ddot a}{a} = -\\frac{4\\pi G}{3}\\left(\\rho + \\frac{3p}{c^2}\\right) + \\frac{\\Lambda c^2}{3} / rank | |||
Normal rank | |||
Latest revision as of 14:02, 2 September 2026
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| Language | Label | Description | Also known as |
|---|---|---|---|
| English | Cosmic acceleration: the second Friedmann equation |
No description defined |
Statements
\\frac{\\ddot a}{a} = -\\frac{4\\pi G}{3}\\left(\\rho + \\frac{3p}{c^2}\\right) + \\frac{\\Lambda c^2}{3}
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