High-low pressure domain wall for the classical Toda lattice

Dear Editor and Reviewers,

We thank you for critically reading our manuscript, and greatly appreciate your helpful comments and suggestions. We have addressed them as follows:

Response to reviewer 1: 1. Before equation 2.13 it might be useful to explicitly define the linear operator $W$. Such a detailed discussion of the non-interacting case has been removed. 2. In order to render the presentation more self-contained and for the sake of clarity, before equation 3.8, provide more details about the GHD equations. The Toda GHD is discussed at length in the recent literature. While trying to avoid duplication, we still added a few more explanations for better readability. 3. The singularity in the non-equilibrium behavior seems to be related to the existence of a critical pressure in equilibrium. Could you elaborate on this relationship? To more clearly state the main result of our contribution, we changed the title, rewrote the introduction, and correspondingly modified the last section. The critical pressure corresponds to a vanishing free volume (= stretch). 4. Is it possible to specify the parameter region for which this singularity appears? Is there any identifiable condition on $P_+$ and $P_-$ that ensures the appearance of the singularity? As far as I understand, the authors have studied only one point for which the singularity is present. The specific values of $P_+$ and $P_-$ are of no importance as long as $P_- < P_\mathrm{c} < P_+$. We have run more simulations for other parameters satisfying the condition. No qualitative change is observed.

Response to reviewer 2: - What is the self-similar solution of GHD? Something is said after eq. 2.14, but should be clearly stated in the paper. What is W in eq. (2.13)? I guess it is the Wigner function, but it is not defined. We now define explicitly the notion of self-similarity. The detailed discussion on the non-interacting case has been removed. So $W$ and Eqs. (2.13), (2.14) no longer appear. - As far as I understand the paragraph numerical method'' (page 8) is the algorithm for the equilibrium problem (the initial condition) and not for the GHD equation: I would specify it, since the section is calledGHD of the Toda lattice''. This is indeed a somewhat misleading formulation. We have expanded and improved our presentation, and also explicitly cover the calculations for GHD. In particular, we emphasize that starting from $n(v)$ allows to compute all the remaining functions of interest. For domain wall only the right/left asymptotics is thermal equilibrium, and the intermediate $n(v)$ has a pointwise jump, as illustrated in Fig. 2(a). - Simulations with molecular dynamics/hard rods are mentioned more than once, but not properly introduced. Our paper does not report on molecular dynamics. But it would be interesting to compare GHD predictions with molecular dynamics. We improved our explanations.

Response to reviewer 3: 1. Is there any physical picture or interpretation that can explain such a singularity? If it is so, I think it would important to explicitly mention it. To more clearly state the main result of our contribution, we changed the title, rewrote the introduction, and correspondingly modified last section. The singularity is linked to the vanishing of the free volume (= stretch). The physical picture of a bottleneck separating low and high pressure regime has been added in Section 5. 2. Which are the conditions for the development of such a singularity? Why was it not observed, for example, in Ref. [19]? The condition is to have a low-high pressure domain wall. In [19] only the case of low-low pressure domain wall is studied. 3. Since the natural output of the GHD equations is $n$ (which is linked to $\rho$ through Eq. (19)), and n is bounded, I do not see why $\nu^{-1}$ diverges. Can the authors comment more on how the singularity is developed in the equations? Is this feature due to the dressing? $\nu^{-1}$ diverges at some intermediate spatial location because the free volume vanishes. We hope that this feature is better explained in the revised version. 4. The singularity $1/|x|$ is not integrable, hence the number of particles contained in an interval encompassing such a singularity is infinite. However, on the initial state the particle density is finite, hence the singularity is developed through time evolution. How does it happen? Can the authors maybe provide a hydrodynamic description for it? I think that microscopic simulations of the classical model could further elucidate this point, but I understand it requires some extra work. Agreed. We reinvestigated the issue. In fact the physical density of particles has an inverse square root divergence, which is integrable. A molecular dynamics simulation is on the agenda. 5. In the conclusions, the authors comment that this singularity seems to be special for the Toda lattice. Can the authors speculate why is it so? What does make Toda special compared with other models? I understand this could be a difficult question, but if the authors have some further insight it would be important to share it. Good point. This is discussed now in Section 5. 6. In Eq. (3.8) $\rho$ and $\nu$ appear for the first time and the authors refer to the preexisting literature for their definition, but maybe some extra comments could make the paper more self-contained. For example, the authors explicitly mention $\rho$ to be the particle density, but do not say anything about $\nu$, which is defined only later in Eq. (3.16). Also, if $\nu^{-1}$ is defined as the integral of the particle density, I would expect it to be a positive quantity, while in Fig. 3.c $\nu$ passes through zero and changes sign. Could it be there is a typo in Eq. (3.16) and there is an absolute value missing? I think the absolute value is needed to be consistent with Ref. [17]. Moreover, I would ask the authors to provide an explicit definition of $\nu$ in their manuscript. We improved this part and added more explanations. In our terminology $\nu$ is the free volume (stretch). By definition, $\nu > 0$ in the low pressure regime and $\nu < 0$ in the high pressure regime. There is no typo in (3.16). $\nu\rho_\mathrm{p}\geq 0$ because it is the DOS of the Lax matrix. When $\nu$ changes from positive to negative values, $\rho_\mathrm{p}$ globally flips its sign, see Fig. 2 (b) in the current version. $\nu$ is now explicitly defined. The common notion of particle density refers to the spectral parameter or root density. This is distinct from the physical density of Toda particles. We tried to make this distinction clear. 7. Lastly, in the abstract it is written ...with a different choice of coordinates smooth behavior is recovered.'' and then, at the end of sectionOf course, the density really diverges, but when viewed in a different coordinate system the behavior is smooth.'' Both sentences sound a bit obscure: which is the coordinate system the authors are referring to? Can they further elaborate on this? Unfortunately these sentences are not so helpful and have been removed. The particle (fluid) picture is now explained in the new Section 5. The low and high pressure particles sit on top of each other in physical space and only cover a half-line. At the end-point of the half-line there is a ``bottleneck" at which the (positive) physical particle density diverges as an inverse square root.

With these changes, we hope that the revised version can be accepted for publication.

Best regards, Christian Mendl and Herbert Spohn

- changed the title to more clearly state the main result
- omitted Fig. 1 in the original manuscript and 1/|x| singularity discussion
- defined explicitly the notion of self-similarity in the introduction; added explanations of Toda GHD; removed detailed discussion of the non-interacting case, such that $W$ and Eqs. (2.13), (2.14) no longer appear
- extended the description of the numerical method, in particular the GHD simulations
- slightly revised the description and discussion of the domain wall problem in section 4
- included comparison of Toda with other models in revised concluding section 5
- physical picture of a bottleneck separating low and high pressure regime added in section 5