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Título

First-passage distributions for the one-dimensional Fokker-Planck equation

AutorArtime Vila, Oriol CSIC; Khalil, Nagi CSIC ORCID ; Toral, Raúl CSIC ORCID ; San Miguel, Maxi CSIC ORCID
Fecha de publicaciónoct-2018
EditorAmerican Physical Society
CitaciónPhysical Review E 98(4): 042143 (2018)
ResumenWe present an analytical framework to study the first-passage (FP) and first-return (FR) distributions for the broad family of models described by the one-dimensional Fokker-Planck equation in finite domains, identifying general properties of these distributions for different classes of models. When in the Fokker-Planck equation the diffusion coefficient is positive (nonzero) and the drift term is bounded, as in the case of a Brownian walker, both distributions may exhibit a power-law decay with exponent −3/2 for intermediate times. We discuss how the influence of an absorbing state changes this exponent. The absorbing state is characterized by a vanishing diffusion coefficient and/or a diverging drift term. Remarkably, the exponent of the Brownian walker class of models is still found, as long as the departure and arrival regions are far enough from the absorbing state, but the range of times where the power law is observed narrows. Close enough to the absorbing point, though, a new exponent may appear. The particular value of the exponent depends on the behavior of the diffusion and the drift terms of the Fokker-Planck equation. We focus on the case of a diffusion term vanishing linearly at the absorbing point. In this case, the FP and FR distributions are similar to those of the voter model, characterized by a power law with exponent −2. As an illustration of the general theory, we compare it with exact analytical solutions and extensive numerical simulations of a two-parameter voterlike family models. We study the behavior of the FP and FR distributions by tuning the importance of the absorbing points throughout changes of the parameters. Finally, the possibility of inferring relevant information about the steady-sate probability distribution of a model from the FP and FR distributions is addressed.
Versión del editorhttps://doi.org/10.1103/PhysRevE.98.042143
URIhttp://hdl.handle.net/10261/188486
DOI10.1103/PhysRevE.98.042143
ISSN470-0045
E-ISSN2470-0053
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