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- W90455257 abstract "Next to flat Minkowski space, the simplest solutions of general relativity are given by isotropic Friedmann–Lemaitre–Robertson–Walker (FLRW) universe models. Friedmann–Lemaitre–Robertson–Walker (FLRW) model Thanks to spatial isotropy, there is just a single parameter, the scale factor (a(hbox {t})) scale factor determining the spatial scale via the line element $$ {text{d}}s^2=-N(t)^2{text{d}}t^2+a(t)^2{text{d}}sigma_k^2 $$(2.1)with $$ {text{d}}sigma_k^2={frac{{text{d}}r^2}{1-kr^2}}+r^2({text{d}}vartheta^2+ sin^2vartheta{text{d}}varphi^2) .$$(2.2)" @default.
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- W90455257 date "2011-01-01" @default.
- W90455257 modified "2023-09-26" @default.
- W90455257 title "Cosmology and Quantum Theory" @default.
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- W90455257 doi "https://doi.org/10.1007/978-1-4419-8276-6_2" @default.
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