Abstract
“Let us take a particular cosmological model as a basis for studying what happens when the constants of nature are changed in value. In this way we shall generate not just a new range of models of our universe, but a range or ensemble of universes corresponding to the given cosmological model. An ensemble of universes, covering all values of the constants of nature, apparently contains only a very small subset of universes in which stars and planetary systems exist. This leads to the conclusion: the constants of nature have their observed value because our universe is perhaps the only universe in which they can be observed by intelligent life.”
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