The increments of Brownian motion are so jagged that the path has no derivative and no finite length, yet a different accumulated quantity, the sum of squared increments, is perfectly regular and equals the elapsed time. This quadratic variation is the reason a stochastic integral cannot be defined pathwise as a Riemann-Stieltjes integral and the reason the chain rule for Brownian functions carries a second-order correction. This post proves that Brownian motion has quadratic variation equal to time, building on the probability-space and independence results developed earlier [1], [2]. Throughout, is a standard Brownian motion and partitions of are with mesh .
#The quadratic variation of a path
The quadratic variation of a process over along a partition is . The process has quadratic variation when these sums converge to in (equivalently in probability) as the mesh tends to . For a deterministic path the convergence is pathwise, and for Brownian motion the limit holds along any mesh- sequence, with almost-sure convergence along sufficiently fast-shrinking sequences such as the dyadic ones.
For a continuously differentiable path the quadratic variation is zero. With on each increment obeys , so and
where is the (finite) total variation. The product vanishes because the mesh tends to while stays finite. A nonzero quadratic variation is therefore a signature of nonsmoothness, and Brownian motion has the simplest possible one.
#Brownian motion accumulates quadratic variation
For a standard Brownian motion and any partition of , the sum has and . Consequently in mean square as the mesh tends to , so .
Write , which by the increment law is and independent across . The second moment is , so by telescoping. For the variance, independence of the gives . A centred Gaussian of variance has fourth moment , read from the moment expansion of its characteristic function, so . Hence
which tends to as the mesh does. So in mean square, hence .
Along the dyadic partitions, where is cut into equal pieces, the convergence is almost sure, not merely in mean square.
For the dyadic partitions of , the quadratic-variation sums converge to almost surely.
With pieces each of length , the bound Equation (2) gives . By Chebyshev's inequality, , a convergent series in , so by the Borel-Cantelli lemma the event occurs only finitely often. Taking and intersecting the countably many resulting probability-one events gives almost surely.
#Infinite total variation
The roughness that produces a nonzero quadratic variation forbids a finite length.
Almost surely, Brownian motion has infinite total variation on every interval with .
Suppose the total variation were finite on a path. Along the dyadic partitions,
Let be the event that the path is continuous and the event from Corollary 3; both have probability one, so . Fix with finite total variation . Continuity on the compact is uniform, so the maximal increment over the dyadic partition tends to as , forcing by Equation (3). This contradicts , so for every , a set of probability one.
The infinite total variation is exactly why the stochastic integral cannot be built as a pathwise Stieltjes integral against , since that construction requires the integrator to have finite variation. The stochastic integral instead uses the finiteness of the quadratic variation, isometrically matching the second moment of the integral with an ordinary integral against .
#Covariation
Polarising the quadratic variation gives a bilinear pairing of two processes.
The covariation of and over is along partitions of vanishing mesh, equal to when the quadratic variations on the right exist.
For a second standard Brownian motion independent of the covariation is zero. Then has independent increments with , so its quadratic- variation sum has mean and variance , giving in . Since the algebraic identity and all three quadratic variations converge in over the same partitions, the cross sum has limit . The covariation of a Brownian motion with any continuous finite-variation process is likewise zero by the estimate Equation (3), so smooth drifts do not interact with Brownian noise at second order. These facts assemble into the multiplication rule , , . This bookkeeping drives Ito's formula, whose second-order term is exactly the quadratic variation that smooth calculus never sees.