Put . Since the bracket is continuous finite variation, . The Itô formula applied to gives
Therefore
With the printed exponential formula, . The usual unit-initial-value stochastic exponential is ; the two coincide when , as in part (c).
For any strictly positive solution of this stochastic equation, its bracket is . Applying Itô to the logarithm, after localizing away from zero if necessary, gives
The same identity holds for , so is constant in time and is zero initially. Their continuous versions agree at all times on one full-probability event. Thus pathwise uniqueness for a multiplicative martingale equation gives
This is indistinguishability of stochastic processes, not just equality almost surely at each separately chosen time.
For and , the definition of the Radon-Nikodym derivative gives
The density is nonnegative and integrable; with the probability normalization used here its expectation is one. Hence
so is a martingale. When , the Itô formula under Wiener measure gives
The first term is a continuous local martingale, by localization on compact space-time sets. Since is a martingale, uniqueness of the continuous semimartingale decomposition makes identically. The integrand is continuous in time along every continuous path, so for every , outside one common null event.
For each fixed , has a Gaussian distribution with strictly positive density everywhere on . Since is continuous, almost surely implies for every real . Therefore
If the stated smoothness includes time zero, continuity extends the equation there. This is the backward heat equation. The full-support argument is needed to pass from an identity along Brownian paths to an equation at every spatial point.
Define . Positivity and smoothness of make continuous and bounded on compact space-time sets. Brownian paths remain in compact spatial sets on each finite horizon, so almost surely for every . Thus
is a well-defined continuous local martingale with . The backward heat equation from part (b) removes the drift in Itô's formula and yields
By the allowed fact and the uniqueness in part (a),
The finite-horizon form of the Girsanov theorem used here says: if is a continuous local martingale and its stochastic exponential is a strictly positive true martingale of mean one on , then under every continuous -local martingale becomes the -local martingale . Quadratic variation is unchanged by this locally equivalent change of measure.
All the assumptions hold. The integrand defining is locally square integrable as checked above; is strictly positive; and it is already a true martingale because it is the density process. On each finite horizon , so it is uniformly integrable on that horizon. There is no need to establish a separate Novikov condition, nor to assume equivalence on the infinite-time sigma-algebra.
Take . Its covariation with is . Hence is a continuous -local martingale starting at zero with . The Lévy characterization of Brownian motion makes it Brownian under . Since this argument holds on every finite horizon for the same process ,
This is the Brownian change of measure by a positive space-time harmonic function, a Doob h-transform with drift .

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