Girsanov for Stochastic Differential Equations
The Girsanov theorem turns a drifted Brownian motion into a Brownian motion by tilting the probabilities, not the paths. This page runs the same tilt through equations. It turns solutions of one stochastic differential equation into solutions of another that differs by a drift, and then lets the mechanism loose on equations too rough for the existence theory to reach. One scope decision should be stated plainly. The exchange below keeps the noise additive. The coefficient in front of \(d\mathbf{w}\) is the identity, and the state and the noise share the dimension \(n\). A version with a state-dependent coefficient matrix exists, but transporting the stochastic integral itself across a change of measure requires knowing that the integral's construction is unchanged by an equivalent reweighting of probabilities, a fact that has not been built on this track. The additive-noise exchange closes by pathwise algebra alone, and it is exactly the form the weak-solution construction ahead puts to work.
Fix \(T \gt 0\), a point \(x \in \mathbb{R}^n\), and constants \(C\) and \(D\). Let \(b : \mathbb{R}^n \to \mathbb{R}^n\) be Lipschitz continuous with constant \(D\), and let \(X = X^x\) be the solution of
\[ dX_t = b(X_t)\, dt + d\mathbf{w}_t , \quad 0 \leq t \leq T , \quad X_0 = x , \]
provided by the existence and uniqueness theorem read in the systems convention recorded at the close of the existence pages. Let \(\boldsymbol{\gamma}(s, \omega)\) be progressively measurable with \(|\boldsymbol{\gamma}| \leq C\), and let \(\mathbf{Y}\) be a continuous adapted process satisfying, almost surely, simultaneously for every \(t \in [0, T]\),
\[ \mathbf{Y}_t = x + \int_0^t \bigl( \boldsymbol{\gamma}(s, \omega) + b(\mathbf{Y}_s) \bigr)\, ds + \mathbf{w}_t . \]
Let \(M\) be the exponential martingale of \(\boldsymbol{\gamma}\), let \(\mathbb{Q}\) be the measure of the Girsanov theorem applied to \(\boldsymbol{\gamma}\), and set \(\hat{\mathbf{w}}_t = \int_0^t \boldsymbol{\gamma}\, ds + \mathbf{w}_t\). Then:
(1) At every \(\omega\) where the displayed identity holds, and for every \(t \in [0, T]\), \(\mathbf{Y}_t = x + \int_0^t b(\mathbf{Y}_s)\, ds + \hat{\mathbf{w}}_t\).
(2) On the space \(\bigl( \Omega, \mathcal{F}_T^{(n)}, \mathbb{Q} \bigr)\) with the filtration \(\{\mathcal{F}_t^{(n)}\}\), the pair \((\mathbf{Y}, \hat{\mathbf{w}})\) is a weak solution of \(dX_t = b(X_t)\, dt + d\hat{\mathbf{w}}_t\) with initial law \(\delta_x\).
(3) The law of \(\mathbf{Y}\) under \(\mathbb{Q}\) coincides with the law of \(X^x\) under \(\mathbb{P}\), that is, their finite-dimensional distributions on \([0, T]\) agree.
Step 1 (Pathwise rearrangement).
Wherever the hypothesis identity holds,
\[ \mathbf{Y}_t - \int_0^t b(\mathbf{Y}_s)\, ds = x + \int_0^t \boldsymbol{\gamma}\, ds + \mathbf{w}_t = x + \hat{\mathbf{w}}_t , \]
which is (1). No measure has been mentioned yet. This is algebra of paths.
Step 2 (The new noise and its filtration).
The Girsanov theorem applied to \(\boldsymbol{\gamma}\) makes
\(\mathbb{Q}\) a probability measure with the same null sets as
\(\mathbb{P}\), and makes \(\hat{\mathbf{w}}\) an \(n\)-dimensional
Brownian motion relative to \(\{\mathcal{F}_t^{(n)}\}\) under
\(\mathbb{Q}\), with each increment
\(\hat{\mathbf{w}}_t - \hat{\mathbf{w}}_s\) independent of
\(\mathcal{F}_s^{(n)}\). The filtration contains every
\(\mathbb{P}\)-null set by construction, and every \(\mathbb{Q}\)-null
set is \(\mathbb{P}\)-null by the equivalence, so it contains every
\(\mathbb{Q}\)-null set. These are the two properties that the
enlargement lemma
supplies in the strong-solution setting, adaptedness over a filtration
holding all null sets and independence of increments from the running
past, now holding for \(\hat{\mathbf{w}}\) under \(\mathbb{Q}\).
Step 3 (The solution clauses under \(\mathbb{Q}\)).
We verify clauses (S1) through (S4) of the
solution definition
for \(\mathbf{Y}\), coordinate by coordinate in the systems convention,
for the equation with drift \(b\) and unit noise coefficient, on the
space \(\bigl( \Omega, \mathcal{F}_T^{(n)}, \mathbb{Q} \bigr)\), with
initial value the constant \(x\), which is square integrable and
independent of everything.
(S1) Adaptedness and path continuity are properties of the maps \(\omega \mapsto \mathbf{Y}_\cdot(\omega)\) alone and do not see the change of measure.
(S3) For every \(\omega\), the map \(s \mapsto b(\mathbf{Y}_s)\) is continuous, being a composition of continuous maps, hence integrable on the compact \([0, T]\). The constant integrand \(1\) is measurable and adapted with \(\mathbb{E}_{\mathbb{Q}}\bigl[ \int_0^T 1\, ds \bigr] = T \lt \infty\), so it lies in \(\mathcal{V}(0, T)\) read over the \(\mathbb{Q}\)-space.
(S4) The constant integrand is an elementary process, and on elementary processes the integral is defined as the telescoping sum of increments, so \(\int_0^t d\hat{w}^{(i)}_s = \hat{w}^{(i)}_t\) for each coordinate. Clause (S4) is then Step 1's identity, which holds almost surely simultaneously for every \(t\).
(S2) Lipschitz continuity gives linear growth, \(|b(\mathbf{y})| \leq |b(\mathbf{0})| + D\, |\mathbf{y}|\). Fix \(\omega\) on the full event of Step 1 and write \(\hat{W}^* = \sum_{i=1}^{n} \sup_{s \leq T} |\hat{w}^{(i)}_s|\), so that \(|\hat{\mathbf{w}}_t| \leq \hat{W}^*\) for all \(t\). From (1),
\[ |\mathbf{Y}_t| \leq \bigl( |x| + |b(\mathbf{0})|\, T + \hat{W}^* \bigr) + D \int_0^t |\mathbf{Y}_s|\, ds , \]
and \(t \mapsto |\mathbf{Y}_t(\omega)|\) is continuous, hence measurable with finite integral over \([0, T]\), so Gronwall's inequality, applied path by path with the additive constant in parentheses and the multiplier \(D\), gives \(|\mathbf{Y}_t| \leq \bigl( |x| + |b(\mathbf{0})|\, T + \hat{W}^* \bigr)\, e^{D T}\). Squaring, integrating in time, and using \((u + v + z)^2 \leq 3 (u^2 + v^2 + z^2)\),
\[ \mathbb{E}_{\mathbb{Q}}\Bigl[ \int_0^T |\mathbf{Y}_t|^2\, dt \Bigr] \leq 3\, T\, e^{2 D T} \Bigl( |x|^2 + |b(\mathbf{0})|^2 T^2 + \mathbb{E}_{\mathbb{Q}}\bigl[ (\hat{W}^*)^2 \bigr] \Bigr) , \]
and it remains to bound the last expectation. Each coordinate \(\hat{w}^{(i)}\) is a \(\mathbb{Q}\)-martingale with respect to \(\{\mathcal{F}_t^{(n)}\}\). It is adapted, each \(\hat{w}^{(i)}_t\) is integrable because its \(\mathbb{Q}\)-law is that of a Brownian coordinate, and for \(s \leq t\) the increment is independent of \(\mathcal{F}_s^{(n)}\) by Step 2, so the independence collapse gives \(\mathbb{E}_{\mathbb{Q}}\bigl[ \hat{w}^{(i)}_t - \hat{w}^{(i)}_s \mid \mathcal{F}_s^{(n)} \bigr] = \mathbb{E}_{\mathbb{Q}}\bigl[ \hat{w}^{(i)}_t - \hat{w}^{(i)}_s \bigr] = 0\), the mean vanishing because the law of the increment is centered Gaussian. Paths are continuous, so Doob's martingale inequality with \(p = 4\), read on the space \(\bigl( \Omega, \mathcal{F}_T^{(n)}, \mathbb{Q} \bigr)\) and with the dyadic supremum agreeing with the full supremum along continuous paths, gives
\[ \mathbb{Q}\Bigl[ \sup_{s \leq T} |\hat{w}^{(i)}_s| \geq \lambda \Bigr] \leq \frac{1}{\lambda^4}\, \mathbb{E}_{\mathbb{Q}}\bigl[ (\hat{w}^{(i)}_T)^4 \bigr] = \frac{3 T^2}{\lambda^4} , \]
the fourth moment being that of a centered Gaussian with variance \(T\) by the law identification. Writing \(\varphi_T\) for its density, the relation \(z\, \varphi_T(z) = -T\, \varphi_T'(z)\) and one integration by parts give \(\mathbb{E}_{\mathbb{Q}}[(\hat{w}^{(i)}_T)^4] = 3\, T\, \mathbb{E}_{\mathbb{Q}}[(\hat{w}^{(i)}_T)^2] = 3\, T^2\). The layer-cake identity \(S^2 = \int_0^\infty 2 \lambda\, \mathbf{1}_{\{\lambda \lt S\}}\, d\lambda\) and Tonelli's theorem convert the tail bound into a moment bound. Splitting the integral at \(\lambda = (3 T^2)^{1/4}\), where the two estimates \(\mathbb{Q}[\cdot] \leq 1\) and the display cross, we obtain
\[ \mathbb{E}_{\mathbb{Q}}\Bigl[ \sup_{s \leq T} |\hat{w}^{(i)}_s|^2 \Bigr] = \int_0^\infty 2 \lambda\, \mathbb{Q}\Bigl[ \sup_{s \leq T} |\hat{w}^{(i)}_s| \gt \lambda \Bigr]\, d\lambda \leq \sqrt{3}\, T + \sqrt{3}\, T = 2 \sqrt{3}\, T . \]
Then \((\hat{W}^*)^2 \leq n \sum_i \sup_{s \leq T} |\hat{w}^{(i)}_s|^2\) by the Cauchy-Schwarz inequality on the defining sum, so \(\mathbb{E}_{\mathbb{Q}}[(\hat{W}^*)^2] \leq 2 \sqrt{3}\, n^2 T \lt \infty\), and (S2) holds. Together with Step 2, all clauses of the weak solution definition are met, with initial law \(\delta_x\). This proves (2).
Step 4 (Uniqueness in law).
The strong solution \(X^x\) on the original space, driven by
\(\mathbf{w}\) under \(\mathbb{P}\) over the enlarged filtration of a
constant start, is a solution of the same equation with the same initial
law \(\delta_x\). The coefficients satisfy (H1) and (H2). The constant
noise coefficient trivially, and the drift because Lipschitz continuity
supplies both the Lipschitz clause and, through
\(|b(\mathbf{y})| \leq |b(\mathbf{0})| + D |\mathbf{y}|\), linear
growth. The initial law \(\delta_x\) has finite second moment. The
uniqueness in law lemma,
read in the same systems convention, therefore applies to the pair of
solutions \((X^x, \mathbf{w})\) under \(\mathbb{P}\) and
\((\mathbf{Y}, \hat{\mathbf{w}})\) under \(\mathbb{Q}\). That lemma's
proof is a sketch whose single unproved step is the induction carrying
laws through the Picard iterates, and this page's reliance on it
inherits exactly that one point of trust and no other. The conclusion
is that the two solutions share their finite-dimensional distributions,
which is (3).
The theorem inverts the usual order of solving. Ordinarily an equation is given and a solution must be manufactured. Here a process is given, its equation is off by a drift, and a change of measure repairs the equation without touching the process. The construction that follows runs this inversion at full strength. It starts from a process so simple that it solves almost nothing, Brownian motion itself, and tilts the measure until it solves an equation whose coefficients are too rough for the existence theorem to reach.