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The Wall-Confined Free Energy: Norm Bound, Lower Bound, Weak-Star Compact Sublevel Sets and Displacement Monotonicity of the Score

The wall-confined free energy lives on laws with norm bound R, is bounded below, has weak-star compact sublevel sets on which it is lower semicontinuous, and has a score that is displacement monotone along optimal couplings.

Statement

In the setting of Noncommutative Laws, Couplings and the Wasserstein Distance: Standing Notation, let (D0,E0)(\mathcal{D}_{0},\mathcal{E}_{0}) be a free entropy penalty, let R>0R>0 be real, and let E:D→R\mathcal{E}:\mathcal{D}\to\mathbb{R}, on D=D0∩DR\mathcal{D}=\mathcal{D}_{0}\cap\mathcal{D}_{R} with DR\mathcal{D}_{R} the domain of the wall energy, be its wall-confined free energy with radius RR, with score domain DΞ\mathcal{D}_{\Xi} and score Ξ\Xi. The coupling pairings Jγ1\mathcal{J}^{1}_{\gamma} and Jγ2\mathcal{J}^{2}_{\gamma} are those of Marginal Isometries, Bounded Plans and Displacement Pairings for Noncommutative Laws §coupling-pairing, and weak-star convergence is that of Weak-Star Convergence of Noncommutative Laws §weak-star.

1. (Bounds) D⊆Σd,R\mathcal{D}\subseteq\Sigma_{d,R}, and there is a real ee with e≤E(λ)e\le\mathcal{E}(\lambda) for every λ∈D\lambda\in\mathcal{D}.

2. (Compact sublevel sets) Let cc be real and let (λm)m∈N(\lambda_{m})_{m\in\mathbb{N}} be a sequence in D\mathcal{D} with E(λm)≤c\mathcal{E}(\lambda_{m})\le c for every m∈Nm\in\mathbb{N}. Then there are a strictly increasing sequence (mi)i∈N(m_{i})_{i\in\mathbb{N}} of natural numbers and λ∈D\lambda\in\mathcal{D} such that (λmi)i∈N(\lambda_{m_{i}})_{i\in\mathbb{N}} converges weak-star to λ\lambda, the real sequence (E(λmi))i∈N(\mathcal{E}(\lambda_{m_{i}}))_{i\in\mathbb{N}} converges, and E(λ)≤lim⁡i→∞E(λmi)\mathcal{E}(\lambda)\le\lim_{i\to\infty}\mathcal{E}(\lambda_{m_{i}}).

3. (Monotone score) If μ,ν∈DΞ\mu,\nu\in\mathcal{D}_{\Xi} and γ∈Π(μ,ν)\gamma\in\Pi(\mu,\nu) is an optimal coupling, then

Jγ1(Ξ(μ))−Jγ2(Ξ(ν))≥0.\mathcal{J}^{1}_{\gamma}\bigl(\Xi(\mu)\bigr)-\mathcal{J}^{2}_{\gamma}\bigl(\Xi(\nu)\bigr)\ge0.

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