First-passage area distribution and optimal fluctuations of fractional Brownian motion
arXiv:2310.14003 · doi:10.1103/PhysRevE.109.014146
Abstract
We study the probability distribution of the area swept under fractional Brownian motion (fB\ m) until its first passage time to the origin. The process starts at from a specified point . We show that obeys exact scaling relation where is the Hurst exponent characterizing the fBm, is the coefficient of fractional diffusion, and is a scaling function. The small- tail of has been recently predicted by Meerson and Oshanin [Phys. Rev. E 105, 064137 (2022)], who showed that it has an essential singularity at , the character of which depends on . Here we determine the large- tail of . It is a fat tail, in particular such that the average value of the first-passage area diverges for all . We also verify the predictions for both tails by performing simple-sampling as well as large-deviation Monte Carlo simulations. The verification includes measurements of up to probability densities as small as . We also perform direct observations of paths conditioned to the area . For the steep small- tail of the "optimal paths", i.e. the most probable trajectories of the fBm, dominate the statistics. Finally, we discuss extensions of theory to a more general first-passage functional of the fBm.
9 pages, 8 figures
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