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for the Dirichlet form associated to sticky Brownian motion. Denoting a_0=\frac{1}{2+\omega L} and b_0=\omega a_0 , for all s>0 we have

\int f^2\mathrm{d}\mu=a_0(f(0)^2+f(L)^2)+b_0\int_0^L f^2\mathrm{d}x, \le a_0(f(0)^2+f(L)^2)+b_0s\int_0^L(f')^2\mathrm{d}x+b_0\beta(s)\left(\int_0^L|f|\mathrm{d}x\right)^2, \le b_0s\int_0^L(f')^2\mathrm{d}x+b_0\max(b_0^{-2},a_0^{-1})\beta(s)\left(\int|f|\mathrm{d}\mu\right)^2.

Therefore the sticky Brownian satisfies a super Poincaré inequality. Then by [Wan00, Th. 5.1], it has an empty essential spectrum. Now, by [BGL14, Th. A.6.4], the resolvent is compact and thus the generator has discrete spectrum. \square

Corollary 19. Choosing T=m^{-1/2} , the transition semigroup of the RTP process is exponentially contractive in T -average with rate

\nu=\Omega\left(\frac{\omega}{1+(\omega L)^2}\right).

Note that the relaxation time corresponding to this decay rate is of the same order as the mixing time obtained in [GHM24]. It reveals the existence of two regimes controlled by the parameter \omega L . In the ballistic regime \omega L\ll 1 , velocity flips are rare, leading to a fast exploration of the position space \mathcal{S} and a comparatively slow exploration of the velocity space \mathcal{V} . This results in the scaling \nu\propto\omega . On the contrary, in the diffusive regime \omega L\gg 1 , the high frequency of velocity flips makes the exploration of \mathcal{V} faster than the exploration of \mathcal{S} . This leads to the scaling \nu\propto\omega^{-1}L^{-2} .

Proof. We begin by verifying Assumption (A). Recall that \mathrm{Dom}(\mathcal{L}_{C^0}) is a core of \mathcal{L} by Theorem 7. For all f\in\mathrm{Dom}(\mathcal{L}_{C^0}) we have \hat{\mathcal{L}}_v(f\circ\pi)=0 hence \hat{\mathcal{L}}_{\mathrm{tr}} is a lift of \mathcal{L} by Remark 8. Furthermore, for f\in\mathrm{Dom}(\mathcal{L}_{C^0}) one has

\hat{\mathcal{L}}_{\mathrm{tr}}^*(f\circ\pi)(x,v)=-v1_{\{0<x<L\}}f'(x)=-\hat{\mathcal{L}}_{\mathrm{tr}}(f\circ\pi)(x,v).

A straightforward computation yields

\int_\mathcal{V}\hat{\mathcal{L}}_vf(x,v)\mathrm{d}\kappa_x(v)=0\text{ for all }x\in\mathcal{S}\text{ and }f\in\mathrm{Dom}(\hat{\mathcal{L}}).

Finally, we prove \|f-\Pi_vf\|_{L^2(\hat{\mu})}^2\le\frac{1}{m_v}\mathcal{E}_v(f) with m_v=2 . Define the matrices

S=\begin{pmatrix} 1/4 & 0 & 0 \\ 0 & 1/2 & 0 \\ 0 & 0 & 1/4 \end{pmatrix},\quad Q=\begin{pmatrix} -2 & 2 & 0 \\ 1 & -2 & 1 \\ 0 & 2 & -2 \end{pmatrix},

as well as the scalar product \langle x,y\rangle_S=x^\top Sy and let \Pi be the orthogonal projection on the kernel of Q with respect to \langle\cdot,\cdot\rangle_S . The matrix Q is symmetric w.r.t. the scalar

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