Inviting an author to review:
Find an author and click ‘Invite to review selected article’ near their name.
Search for authorsSearch for similar articles
10
views
0
recommends
+1 Recommend
0 collections
    0
    shares
      • Record: found
      • Abstract: found
      • Article: found
      Is Open Access

      Circular Kardar-Parisi-Zhang interfaces evolving out of the plane

      Preprint
      ,

      Read this article at

      Bookmark
          There is no author summary for this article yet. Authors can add summaries to their articles on ScienceOpen to make them more accessible to a non-specialist audience.

          Abstract

          Circular KPZ interfaces spreading radially in the plane have GUE Tracy-Widom (TW) height distribution (HD) and Airy\(_2\) spatial covariance, but what are their statistics if they evolve on the surface of a different background space, such as a bowl, a cup, or any surface of revolution? To give an answer to this, we report here extensive numerical analyses of several one-dimensional KPZ models on substrates whose size enlarges as \(\langle L(t) \rangle = L_0+\omega t^{\gamma}\), while their mean height \(\langle h \rangle\) increases as usual [\(\langle h \rangle\sim t\)]. We show that the competition between the \(L\) enlargement and the correlation length (\(\xi \simeq c t^{1/z}\)) plays a key role in the asymptotic statistics of the interfaces. While systems with \(\gamma>1/z\) have HDs given by GUE and the interface width increasing as \(w \sim t^{\beta}\), for \(\gamma<1/z\) the HDs are Gaussian, in a correlated regime where \(w \sim t^{\alpha \gamma}\). For the special case \(\gamma=1/z\), a continuous class of distributions exists, which interpolate between Gaussian (for small \(\omega/c\)) and GUE (for \(\omega/c \gg 1\)). Interestingly, the HD seems to agree with the Gaussian symplectic ensemble (GSE) TW distribution for \(\omega/c \approx 10\). Despite the GUE HDs for \(\gamma>1/z\), the spatial covariances present a strong dependence on the parameters \(\omega\) and \(\gamma\), agreeing with Airy\(_2\) only for \(\omega \gg 1\), for a given \(\gamma\), or when \(\gamma=1\), for a fixed \(\omega\). These results considerably generalize our knowledge on the 1D KPZ systems, unveiling the importance of the background space in their statistics.

          Related collections

          Most cited references1

          • Record: found
          • Abstract: found
          • Article: found
          Is Open Access

          Growing interfaces uncover universal fluctuations behind scale invariance

          Stochastic motion of a point – known as Brownian motion – has many successful applications in science, thanks to its scale invariance and consequent universal features such as Gaussian fluctuations. In contrast, the stochastic motion of a line, though it is also scale-invariant and arises in nature as various types of interface growth, is far less understood. The two major missing ingredients are: an experiment that allows a quantitative comparison with theory and an analytic solution of the Kardar-Parisi-Zhang (KPZ) equation, a prototypical equation for describing growing interfaces. Here we solve both problems, showing unprecedented universality beyond the scaling laws. We investigate growing interfaces of liquid-crystal turbulence and find not only universal scaling, but universal distributions of interface positions. They obey the largest-eigenvalue distributions of random matrices and depend on whether the interface is curved or flat, albeit universal in each case. Our exact solution of the KPZ equation provides theoretical explanations.
            Bookmark

            Author and article information

            Journal
            26 October 2018
            Article
            1810.11292
            467c72f3-bef9-43e5-b39d-68170472dd31

            http://arxiv.org/licenses/nonexclusive-distrib/1.0/

            History
            Custom metadata
            8 pages and 8 figures, including a Suppl. Material
            cond-mat.stat-mech

            Condensed matter
            Condensed matter

            Comments

            Comment on this article