Condensation transition in large deviations of self-similar Gaussian processes with stochastic resetting

We study the fluctuations of the area A(t)=integral 0tx(tau)d tau x(tau) with Hurst exponent H > 0 (e.g., standard or fractional Brownian motion, or the random acceleration process) that stochastically resets to the origin at rate r. Typical fluctuations of A(t) scale as similar to t t and on this scale the distribution is Gaussian, as one would expect from the central limit theorem. Here our main focus is on atypically large fluctuations of A(t). In the long-time limit t -> infinity, we find that the full distribution of the area takes the form PrAt similar to exp-t alpha phi(">A/t beta alpha = 1/(2H + 2) and beta = (2H + 3)/(4H + 4) in the regime of moderately large fluctuations, and a different anomalous scaling form Pr(">At similar to exp-t psi(">A/t(">2H+3/2 <i in the regime of very large fluctuations. The associated rate functions phi(y) and psi(w) depend on H and are found exactly. Remarkably, phi(y) has a singularity that we interpret as a first-order dynamical condensation transition, while psi(w) exhibits a second-order dynamical phase transition above which the number of resetting events ceases to be extensive. The parabolic behavior of phi(y) around the origin y = 0 correctly describes the typical, Gaussian fluctuations of A(t). Despite these anomalous scalings, we find that all of the cumulants of the distribution Pr(">At <i grow linearly in time, ;c approximate to cnt <i , in the long-time limit. For the case of reset Brownian motion (corresponding to H = 1/2), we develop a recursive scheme to calculate the coefficients c (n) exactly and use it to calculate the first six nonvanishing cumulants.