Abstract
We study the stochastic six vertex model and prove that under weak asymmetry scaling (i.e., when the parameter \(\Delta \rightarrow 1^+\) so as to zoom into the ferroelectric/disordered phase critical point) its height function fluctuations converge to the solution to the Kardar–Parisi–Zhang (KPZ) equation. We also prove that the one-dimensional family of stochastic Gibbs states for the symmetric six vertex model converge under the same scaling to the stationary solution to the stochastic Burgers equation. Our proofs rely upon the Markov (self) duality of our model. The starting point is an exact microscopic Hopf–Cole transform for the stochastic six vertex model which follows from the model’s known one-particle Markov self-duality. Given this transform, the crucial step is to establish self-averaging for specific quadratic function of the transformed height function. We use the model’s two-particle self-duality to produce explicit expressions (as Bethe ansatz contour integrals) for conditional expectations from which we extract time-decorrelation and hence self-averaging in time. The crux of our Markov duality method is that the entire convergence result reduces to precise estimates on the one-particle and two-particle transition probabilities. Previous to our work, Markov dualities had only been used to prove convergence of particle systems to linear Gaussian SPDEs (e.g. the stochastic heat equation with additive noise).
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Notes
If there is no left-most particle, the dynamics can be still be defined with some care—see Sect. 2.1.
When \(|\Delta |<1\) the conical points in the phase diagram disappear and the two disordered phases merge. When \(\Delta <-1\) a new antiferroelectric phase emerges for H, V near zero. The associated Gibbs state is composed of diagonal bands of zig-zags made up only of the c-type vertices.
In fact, (1.12) only gives upper boundary of the lens. The other boundary comes from applying the diagonal symmetry of the symmetric model.
Recall, the symmetric 6V model only depends on (a, b, c) through two parameters b/a and c/a. Also, note that we have used bold symbols here for \({\mathbf {u}}\) and \(\varvec{\eta }\) since later in the text, \({\mathbf {u}}\) and \(\varvec{\eta }\) will be used for occupation variables. Even though the Baxter parameterizations is limited to this discussion, we prefer not to risk confusion here.
This indicator function is essentially the occupation variable \(\eta \) which is used later in the text, see (2.2). Note that the meaning of the coordinates in \(\eta \) and u are opposite.
We could have made the choice of parameter \(({\mathbf {u}}_\varepsilon ,\varvec{\eta }_\varepsilon )=(\frac{1}{2}\zeta {\sqrt{\varepsilon }},\frac{1}{2}{\sqrt{\varepsilon }})\) (without the lower order part in \({\mathbf {u}}_\varepsilon \)). This would lead to the parameter \(b_1\) which also depends on \(\varepsilon \), though the relation \(b_2/b_1 =e^{-{\sqrt{\varepsilon }}}\) would still hold. Our proof and result should still go through with extra notational complexity, though we do not pursue this direction here.
In terms of the \(\varepsilon \) and \(\zeta \), the (a, b, c) parameterization has a similar expansion of the form \(a=(1+\zeta )\tfrac{1}{2}\sqrt{\varepsilon }+{\mathcal {O}}(\varepsilon ^{-\frac{3}{2}})\), \(b=\zeta \tfrac{1}{2}\sqrt{\varepsilon }+{\mathcal {O}}(\varepsilon ^{-\frac{3}{2}})\), \(c=\tfrac{1}{2}\sqrt{\varepsilon }+{\mathcal {O}}(\varepsilon ^{-\frac{3}{2}})\).
Note that \(\eta (t,y)=\eta _{y}(\vec {x}(t))\). We distinguish the notation \(\eta (t,y)\) as a process and the notation \(\eta _{y}\) as a function on particle configurations \(\vec {x}\) merely for convenience.
The computation for \(\lambda \) simply boils down to a geometric series. The computation for \(\mu \) boils down to a sum of the form \(\sum _{n\ge 0} (n+1) (b_2\tau ^{-\rho })^n\); this multiplied by \((1-b_2 \tau ^{-\rho })\) again gives a geometric series.
For reference, see [Par18, Proposition 4.3] where existence, uniqueness and positivity in a more complicated case (i.e., with boundaries) are proved.
This is different from exponentiating the interpolated height function. Nevertheless, under the weak asymmetry scaling \( \tau =\exp (-{\sqrt{\varepsilon }}) \), it is straightforward to verify that the difference between these two interpolation schemes is negligible as \( \varepsilon \rightarrow 0. \)
Here \( \Gamma (t,\varepsilon )\) does not depend on \( \varepsilon \), but we keep this notation to be consistent throughout all cases.
This follows immediately from (1.29) by a simple tilting and centering.
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Acknowledgements
The authors wish to thank J. Dubédat, P. di Francesco, and T. Spencer for discussions about the disordered phase of the 6V model, A. Aggarwal for discussions about his work on this subject, Y. Lin for careful reading of part of the manuscript and K. Ravishankar for helpful historical references about the role of dualities in SPDE limits. We also appreciate helpful comments from an anonymous referee. I. Corwin was partially supported by the NSF through DMS:1811143 and DMS:1664650, and the Packard Foundation through a Packard Fellowship for Science and Engineering. H. Shen is partially supported by the NSF through DMS:1712684. L-C. Tsai is partially supported by the NSF through DMS:1712575 and the Simons Foundation through a Junior Fellowship. Both I. Corwin and P. Ghosal collaborated on this project during the 2017 Park City Mathematics Institute, partially funded by the NSF through DMS:1441467.
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Appendix A. Quadratic variation in ASEP
Appendix A. Quadratic variation in ASEP
In this appendix we expand upon the brief discussion from Sects. 1.3 and 1.4 and explain how our Markov duality method can be applied to ASEP, which is a simpler limit of the stochastic 6V model. We will not carry out the necessary analysis, but rather just point to the main steps.
Recall that ASEP is an interacting particle system on \( {\mathbb {Z}}\), where particles inhabit sites index by \( {\mathbb {Z}}\) and jump left and right according to continuous-time exponential clocks with rates \( \ell > 0 \) and \( r> 0 \) subject to exclusion (jumps to occupied sites are suppressed). We will assume that \(\ell +r=1\) and set \(\tau := r/\ell \). The ASEP height function \( N_{ASEP }(t,x) \) has 1/0 slopes entering occupied/vacant sites as depicted in Fig. 6. For ASEP with near-stationary initial data of density \( \rho =\frac{1}{2} \) we define a variantFootnote 16 of the Hopf–Cole transform of \( N_{ASEP }(t,x) \) by
This solves the following microscopic SHE:
where \( \Delta f(x):= f(x+1)+f(x-1)-2f(x) \) denotes the discrete Laplacian, and, for each \( x\in {\mathbb {Z}}\), the process \( M(t,x) \), \( t\in {\mathbb {R}}_+ \), is a martingale.
Under weak asymmetry scaling, i.e., \( \tau =\tau _\varepsilon :=e^{-{\sqrt{\varepsilon }}} \) and \( (t,x)\mapsto (\varepsilon ^{-2}t,\varepsilon ^{-1}x) \), an informal scaling argument applied to (A.1) indicates that the equation should converge to the continuum SHE. Key to establishing this convergence is the identification of the limiting quadratic variation of \( M(t,x) \). Under weak asymmetry scaling, the optional quadratic variation of \( M(t,x) \) reads
where, following notations in Sect. 7, \( \mathcal {B}_\varepsilon (t,x) \) is a generic, uniformly bounded process, and
Referring to the r.h.s. of (A.2), we see that \( \varepsilon ^\frac{1}{2} \mathcal {B}_\varepsilon (t,x) \) is indeed negligible compared to the constant \( \frac{1}{4} \) factor. Key to identifying the limiting behavior is to argue that \( {\widetilde{F}}(t,x) \) is also negligible. With \( \nabla Z_{ASEP }(t,x) = (e^{-{\sqrt{\varepsilon }} \eta (t,x+1)}-1)Z_{ASEP }(t,x) \), we indeed have \( {\widetilde{F}}_\varepsilon (t,x) = \mathcal {B}_\varepsilon (t,x) Z_{ASEP }^2(t,x) \), i.e., pointwise bounded up to a multiplicative factor of \( Z_{ASEP }^2(t,x) \). On the other hand, it is conceivable that this term \( {\widetilde{F}}(t,x) \) does not tend to zero pointwise, i.e., \( {\widetilde{F}}(t,x) \not \rightarrow _\text {P} 0 \). The crux of the convergence result is to prove that this term converges to zero after time-averaging:
This is first achieved in [BG97] by showing the decay as t becomes large of the conditional expectation
where \( {\mathscr {F}}\) denotes the canonical filtration of ASEP. Roughly speaking, the estimate starts by using (A.1) to develop a sequence of inequality that bounds the conditional expectation. ‘Closing’ the series of inequality relies crucially on an identity [BG97, (A.6)] for the (semi)-discrete heat kernel. We do not know of a way to generalize this approach from [BG97] to the stochastic 6V model setting.
Here we provide an alternative approach via duality. The Markov duality method also begins with bounding conditional expectations. However, instead of trying to close a sequence of inequalities, this method provides direct access to the conditional expectations. First, the expression \( {\widetilde{F}}_\varepsilon (t,x) \) is not convenient for our purpose. Use \( \nabla Z_{ASEP }(t,x) = (e^{-{\sqrt{\varepsilon }} (\eta ^+(t,x)-\frac{1}{2}) }-1)Z_{ASEP }(t,x) \) where \( \eta ^+(t,x) := \eta (t,x+1) \), and Taylor expand
where \( \mathcal {B}_\varepsilon (t,x)\) stands for a generic uniformly bounded process as in Sect. 7. We can then write \( {\widetilde{F}}_\varepsilon (t,x) = F_\varepsilon (t,x) + \varepsilon ^{1/2} \mathcal {B}_\varepsilon (t,x)Z_{ASEP }^2(t,x) \), where
where, following the notation in Sect. 7,
To see (A.6), we use (A.5) just as in the proof of Lemma 7.3 (for the stochastic 6V model):
In the last step, we replace \(Z_{ASEP }(t,x)\) with \(Z_{ASEP }(t,x\pm 1)\) costing error of order \(\varepsilon ^{1/2} \mathcal {B}_\varepsilon (t,x)Z_{ASEP }(t,x)\).
As mentioned in Sect. 1.4, ASEP enjoys self-duality via the functions Q and \( {\widetilde{Q}} \) defined therein. Specifically, the \( k=2 \) duality translates (after tilting and centering) into the following statement, in which we used the notation
Proposition A.1
For all \( x_1<x_2\in {\mathbb {Z}}\) and \( t,s\in [0,\infty ) \), we have
Proposition A.1 provides the necessary ingredients for expressing conditional expectations for the relevant quantities. Specifically, with \( {\widetilde{Z}}(t,x-1,x) \) being an linear combination the two observables in (A.7) and in (A.8) at \( (x_1,x_2)=(x-1,x) \) we have
Likewise, \( Z_{\nabla }(t,x,x-1) \) is the difference of \( Z_{ASEP }(t,x+1)Z_{ASEP }(t,x-1) \) and \( Z_{ASEP }(t,x)Z_{ASEP }(t,x-1) \). Taking the difference of (A.7) for \( (x_1,x_2) = (x+1,x-1) \) and for \( (x,x-1) \) gives
where \( \nabla _{x_1} \) denotes the discrete (forward) gradient acting on the variable \( x_1 \). Similarly,
From the perspective of duality, roughly speaking, the mechanism of decay in \( t\rightarrow \infty \) arises from the discrete gradient \( \nabla _{x_1} \). The semigroup \( {\mathbf {V}}_{ASEP }\) behaves similar to (two copies of) the heat kernel, so that \(\sum _{y_1<y_2}{\mathbf {V}}_{ASEP }\big ((y_1,y_2),(x_1,x_2);t\big ) = \mathcal O(1)\), and each gradient of \( {\mathbf {V}}_{ASEP }\) effectively produces a factor of \( t^{-1/2} \) for large t. Under the scaling \( \varepsilon ^{-2} \) of time, namely \( t^{-1/2}\approx \varepsilon ^1\), we expect to trade in \( \varepsilon ^{-1/2}\nabla \) for \( \varepsilon ^{-1/2}\varepsilon ^{1}=\varepsilon ^{1/2} \rightarrow 0 \). In other words, the key heuristic is that the l.h.s of (A.4) behaves as
Note that the identity (A.9) in its current form does not involve gradients of \( {\mathbf {V}}_{ASEP }\). This identity can, however, be rewritten via Taylor expansion and summation by parts in a form that exposes the decay in \( t\rightarrow \infty \). We do not perform this procedure here, and direct the readers to Lemma 7.5, where the exact same procedure in carried out for the stochastic 6V model. Specifically, the identity (7.28) therein holds with \( ({\mathbf {V}}_{ASEP },Z_{ASEP },{\mathbb {Z}}) \) in place of \( ({\mathbf {V}}_\varepsilon ,Z,\Xi (s)) \), and with \( s,t\in [0,\infty ) \) instead of \( {\mathbb {Z}}_{\ge 0} \).
Given the preceding discussion, the task for bounding conditional expectations boils down to estimating the semigroup \( {\mathbf {V}}_{ASEP }\) and its gradients. Thanks to Bethe ansatz, \( {\mathbf {V}}_{ASEP }\) permits an explicit, analyzable formula in terms double contour integrals. Under weak asymmetry scaling, we write \( {\mathbf {V}}_{ASEP }={\mathbf {V}}_{\varepsilon ,ASEP }\) and the formula reads
where \( \mathcal {C}_r \) is a counter-clockwise oriented, circular contour centered at origin, with a large enough radius r so as to include all poles of the integrand, and
This contour integral formula is amenable to steepest decent analysis. Careful analysis jointly in \( (x_1,x_2,y_1,y_2,t) \) should produce the relevant estimates on \( {\mathbf {V}}_{\varepsilon ,ASEP }\) and its gradient (the result and proof should be analogous to Proposition 6.1). We do not pursue this analysis here.
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Corwin, I., Ghosal, P., Shen, H. et al. Stochastic PDE Limit of the Six Vertex Model. Commun. Math. Phys. 375, 1945–2038 (2020). https://doi.org/10.1007/s00220-019-03678-z
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DOI: https://doi.org/10.1007/s00220-019-03678-z