How big is a set? For a line segment the answer is its length; for a blob in the plane, its area. But what is the "length" of the rational numbers scattered along a line, or the total size of a fractal dust? Measure theory is the rigorous answer — a single, watertight framework for assigning a size to sets far too wild for ordinary geometry, and for building an integral that can handle them.
The prize is the Lebesgue integral, which succeeds where the school
(Riemann) integral fails: it integrates ferociously discontinuous functions, and its limit
theorems — swapping limits and integrals almost for free — are the engine of modern
One thread runs through everything here. Riemann chops up the x-axis; Lebesgue chops up the y-axis and then asks "how big is the set of x landing in this height band?" — a question of measure. So the whole subject is built in order: decide which sets are measurable (a σ-algebra), assign them sizes (a measure), and only then define the integral as a sum over height bands. Get the measure right and the integral, and its miraculous convergence theorems, follow.
This course moves in two stages.
We begin by breaking the school integral on purpose — meeting a function so jagged that Riemann simply gives up. That failure is exactly the doorway into measure theory.