where <math>\tau</math> is a constant (evaluated at 4.28 * 10<sup>17</sup> s) that is the reciprocal of the Hubble factor ''H''<sub>0</sub> in weak gravity.<ref>Evolutionistic astronomers might assume that this value gives the age of the universe; it does in fact give a value very close to the visible radius of the universe, measured in light-years. It probably does represent a value that an observer at the limits of the visible universe might measure for its age—because the Carmeli-Hartnett system ''also'' predicts tremendous time dilation at the center of the expansion.</ref> | where <math>\tau</math> is a constant (evaluated at 4.28 * 10<sup>17</sup> s) that is the reciprocal of the Hubble factor ''H''<sub>0</sub> in weak gravity.<ref>Evolutionistic astronomers might assume that this value gives the age of the universe; it does in fact give a value very close to the visible radius of the universe, measured in light-years. It probably does represent a value that an observer at the limits of the visible universe might measure for its age—because the Carmeli-Hartnett system ''also'' predicts tremendous time dilation at the center of the expansion.</ref> |