Scott's Theorem: Measurable Cardinals and
Scott's theorem (1961) demonstrates that measurable cardinals are incompatible with Gödel's constructible universe, providing one of the first connections between large cardinals and the structure of the set-theoretic universe.
Statement
If there exists a measurable cardinal, then . Equivalently, the axiom of constructibility implies there are no measurable cardinals.
Suppose is measurable and . Let be a -complete non-principal ultrafilter on , and form the ultrapower .
Since , we have as well (the ultrapower of is ). The embedding is a non-trivial elementary embedding with critical point .
Now, in , the ordinal is definable as "the least measurable cardinal" (if one exists). By elementarity: is the least measurable cardinal in , so . But since is the critical point. Contradiction.
Significance
Scott's theorem shows that the existence of a measurable cardinal is a genuinely "anti-constructibility" assumption. It implies that if large cardinals exist, then the set-theoretic universe must contain sets that are not constructible in Gödel's sense. This was one of the first indications that large cardinal axioms have profound structural consequences.
A related result: (zero sharp) exists if and only if there is a non-trivial elementary embedding . The existence of implies that is "thin" — every uncountable cardinal is inaccessible in — and provides an exact characterization of when the constructible universe is a proper subclass of .
Scott's theorem motivated the development of inner model theory, which constructs canonical models accommodating large cardinals. The models (for a measurable cardinal), (the Dodd-Jensen core model), and Mitchell's models for sequences of measures generalize to accommodate progressively stronger large cardinals while retaining fine structural properties.