Wiki card — concept node for
exp-families-stability.
Let \(\mathcal{P}_2(\mathbb{R}^d)\) denote probability measures with finite second moment, equipped with the quadratic Wasserstein distance \(W_2\). Define the free energy
\[ \mathcal{F}(\rho) \;:=\; \int_{\mathbb{R}^d} \rho\,\log\rho\, dx \;+\; \int V\, \rho\, dx, \]
for a potential \(V : \mathbb{R}^d \to \mathbb{R}\) (possibly \(V \equiv 0\)).
Theorem (Jordan–Kinderlehrer–Otto 1998). The Fokker–Planck equation \[ \partial_t \rho \;=\; \tfrac12 \Delta \rho \;+\; \nabla\cdot(\rho \nabla V) \] is the \(W_2\)-gradient flow of \(\mathcal{F}\): \[ \boxed{\;\rho^{n+1} \;=\; \arg\min_{\rho \in \mathcal{P}_2}\Bigl\{\tfrac{1}{2\tau} W_2^2(\rho, \rho^n) \;+\; \mathcal{F}(\rho)\Bigr\}\;} \tag{JKO} \] converges, as \(\tau \to 0\), to the Fokker–Planck solution.
In particular, for \(V \equiv 0\), the heat equation \(\partial_t \rho = \tfrac12 \Delta\rho\) is the \(W_2\)-gradient flow of (negative) differential entropy: \(\mathcal{F}(\rho) = \int \rho \log\rho\).
Restrict to \(\rho = \mathcal{N}(\mu, \sigma^2)\) on \(\mathbb{R}\). Then:
JKO with \(V = 0\): minimise \(\tfrac{1}{2\tau}\bigl((\mu - \mu_n)^2 + (\sigma - \sigma_n)^2\bigr) - \tfrac12 \log(2\pi e \sigma^2)\) over \((\mu, \sigma)\).
Critical-point conditions:
Continuous limit \(\tau \to 0\): \(\dot\mu = 0\), \(\dot\sigma = 1/\sigma\), i.e. \(\sigma^2(t) = \sigma^2(0) + 2 \cdot \tfrac{t}{2} = \sigma^2(0) + t\) (scaling by factor 2 absorbed into the \(\tfrac12\Delta\) convention; with the standard convention \(\partial_t \rho = \tfrac12 \partial_{xx}\rho\), \(\sigma^2(t) = \sigma^2(0) + t\)). ✓
Information-geometric takeaway. On the Gaussian submanifold, JKO reduces to a Euclidean gradient flow on \((\mu, \sigma)\), producing Q2's Riccati flow exactly. The submanifold is invariant, confirming Wheeler's reformulation: \(\mathcal{E}_{\mathrm{Gauss}}\) is a totally geodesic locus for the Wasserstein gradient flow of entropy.