TheoremComplete

Scott's Theorem: Measurable Cardinals and VLV \neq L

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

Theorem7.2Scott's Theorem

If there exists a measurable cardinal, then VLV \neq L. Equivalently, the axiom of constructibility V=LV = L implies there are no measurable cardinals.

Proof

Suppose κ\kappa is measurable and V=LV = L. Let UU be a κ\kappa-complete non-principal ultrafilter on κ\kappa, and form the ultrapower j:VM=Ult(V,U)j: V \to M = \mathrm{Ult}(V, U).

Since V=LV = L, we have M=LM = L as well (the ultrapower of LL is LL). The embedding j:LLj: L \to L is a non-trivial elementary embedding with critical point κ\kappa.

Now, in LL, the ordinal κ\kappa is definable as "the least measurable cardinal" (if one exists). By elementarity: j(κ)j(\kappa) is the least measurable cardinal in M=LM = L, so j(κ)=κj(\kappa) = \kappa. But j(κ)>κj(\kappa) > \kappa since κ\kappa is the critical point. Contradiction. \square


Significance

RemarkLarge Cardinals Transcend $L$

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.

Example$0^\sharp$ and the Constructible Universe

A related result: 00^\sharp (zero sharp) exists if and only if there is a non-trivial elementary embedding j:LLj: L \to L. The existence of 00^\sharp implies that LL is "thin" — every uncountable cardinal is inaccessible in LL — and provides an exact characterization of when the constructible universe is a proper subclass of VV.

RemarkInner Model Theory

Scott's theorem motivated the development of inner model theory, which constructs canonical models accommodating large cardinals. The models L[U]L[U] (for a measurable cardinal), KDJK^{DJ} (the Dodd-Jensen core model), and Mitchell's models for sequences of measures generalize LL to accommodate progressively stronger large cardinals while retaining fine structural properties.