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| | Scale factor (Universe) - Wikipedia, the free encyclopedia |
 | | The evolution of the scale factor is a dynamical question, determined by the equations of general relativity, which are presented in the case of a locally isotropic, locally homogeneous universe by the Friedmann equations. |
 | | The scale factor, parameter of Friedmann-Lemaître-Robertson-Walker model, is a function of time which represents the relative expansion of the universe. |
 | | The scale factor could, in principle, have units of length or be dimensionless. |
| en.wikipedia.org /wiki/Scale_factor_(Universe) (192 words) |
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