Write the stochastic differential equation in integral form and replace the unknown integrand by the preceding Picard iterate. With the deterministic initial vector , the recursion is
Each iterate is a continuous adapted process. The Itô isometry inductively gives its square integrability on every bounded time interval, so all these Itô integrals are well defined.
Use for the dummy integration variable in the printed integral. The Itô isometry gives
The assumed second-moment bound also proves the integrability needed to apply the Itô isometry. The extra time integration is the source of the factorial improvement.
Set , where the norms are operator norms, and . Independence of the Brownian coordinates and the vector Itô isometry give
Induction, as in part (b), yields the Factorial Picard estimate for a linear stochastic differential equation
For , the triangle inequality in therefore bounds any tail of the iterates by the corresponding tail of
This numerical series converges by the ratio test: successive terms have ratio . Thus the iterates are Cauchy in , uniformly in the deterministic time parameter on each bounded interval. Completeness of Lp spaces gives a limit . Once its continuous adapted version is chosen in part (d), the Itô isometry permits passage to the limit in the integral equation: the squared norm of each integral difference is bounded by . Consequently the Picard limit solves the stochastic differential equation.
For every , is a continuous square-integrable vector martingale. Its norm is a submartingale, so the Doob L2 maximal inequality and the estimate from part (c) give
The Cauchy-Schwarz inequality now shows
By Tonelli's theorem, the random sum of these suprema is finite almost surely. Therefore the telescoping series converges absolutely and uniformly on outside one null event. Its limit is continuous and agrees at each fixed time with the limit from part (c). Taking the intersection of the probability-one events for integer provides a single version on the whole half-line. Hence
This also gives the requested pointwise almost-sure convergence of the full sequence.
Standard Brownian motion is centered, so . If , write ; the final increment is independent of and has mean zero. Thus
This is the Brownian covariance kernel. Together with joint Gaussianity and continuous paths, it gives the Gaussian-process characterization of Brownian motion.
For positive times the transformed process is centered and jointly Gaussian, and
Its paths are continuous away from zero. To verify continuity at zero, we need almost surely as . The strong law of large numbers applied to the independent increments gives . On the unit interval after , the Doob L2 maximal inequality gives
The Borel-Cantelli first lemma, first for each positive rational , shows that these between-integer fluctuations divided by tend to zero. Hence for all real , and as .
The Gaussian-process characterization of Brownian motion now proves is standard Brownian motion, with respect to its natural filtration. This is time inversion of Brownian motion; the transformed process need not be adapted to the original forward filtration.
The Itô formula for gives
The stochastic integral has expectation zero: its square integrability on a finite horizon follows from the finite sixth moments of a normal distribution. Since , integration and expectation yield
Put and . In the two-variable Itô formula, has finite variation, while the only nonzero quadratic term is . Therefore
This proves the stochastic exponential solves the equation. Its initial value is ; no normalization was stipulated.
The resulting process is initially a continuous local martingale. Since and ,
A bounded local martingale is a true martingale: apply the martingale identity to a localizing sequence and use dominated convergence in conditional expectations. The deterministic bound works on every finite horizon, proving is a martingale on every . The bound on also gives a positive deterministic lower bound , although the upper bound already proves the martingale assertion.

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