First Friedmann equation with a cosmological constant (Q1543): Difference between revisions

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H^2 = \\frac{8\\pi G}{3}\\rho - \\frac{k c^2}{a^2} + \\frac{\\Lambda c^2}{3}
 
Property / LaTeX source: H^2 = \\frac{8\\pi G}{3}\\rho - \\frac{k c^2}{a^2} + \\frac{\\Lambda c^2}{3} / rank
Normal rank
 
Property / instance of
 
Property / instance of: mathematical expression / rank
 
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Property / LaTeX source
 
H^2 = \\frac{8\\pi G}{3}\\rho - \\frac{k c^2}{a^2} + \\frac{\\Lambda c^2}{3}
Property / LaTeX source: H^2 = \\frac{8\\pi G}{3}\\rho - \\frac{k c^2}{a^2} + \\frac{\\Lambda c^2}{3} / rank
 
Normal rank

Latest revision as of 14:02, 2 September 2026

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First Friedmann equation with a cosmological constant
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    H^2 = \\frac{8\\pi G}{3}\\rho - \\frac{k c^2}{a^2} + \\frac{\\Lambda c^2}{3}
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