Baldovin M, Caprini L, Vulpiani A
Dipartimento di Fisica, Università di Roma Sapienza, Piazzale Aldo Moro 5, 00185 Rome, Italy.
Scuola di Scienze e Tecnologie, Università di Camerino, via Madonna delle Carceri, 62032 Camerino, Italy.
Phys Rev E. 2021 Sep;104(3):L032101. doi: 10.1103/PhysRevE.104.L032101.
We introduce a general formulation of the fluctuation-dissipation relations (FDRs) holding also in far-from-equilibrium stochastic dynamics. A great advantage of this version of the FDR is that it does not require explicit knowledge of the stationary probability density function. Our formula applies to Markov stochastic systems with generic noise distributions: When the noise is additive and Gaussian, the relation reduces to those known in the literature; for multiplicative and non-Gaussian distributions (e.g., Cauchy noise) it provides exact results in agreement with numerical simulations. Our formula allows us to reproduce, in a suitable small-noise limit, the response functions of deterministic, strongly nonlinear dynamical models, even in the presence of chaotic behavior: This could have important practical applications in several contexts, including geophysics and climate. As a case of study, we consider the Lorenz '63 model, which is paradigmatic for the chaotic properties of deterministic dynamical systems.
我们引入了一种波动耗散关系(FDRs)的通用表述,它同样适用于远离平衡态的随机动力学。这种版本的FDR的一个巨大优势在于,它不需要明确知晓平稳概率密度函数。我们的公式适用于具有一般噪声分布的马尔可夫随机系统:当噪声是加性高斯噪声时,该关系简化为文献中已知的关系;对于乘性和非高斯分布(例如柯西噪声),它能给出与数值模拟结果相符的精确结果。我们的公式使我们能够在合适的小噪声极限下,重现确定性强非线性动力学模型的响应函数,即使存在混沌行为:这在包括地球物理学和气候学在内的多个领域可能具有重要的实际应用。作为一个研究案例,我们考虑洛伦兹'63模型,它是确定性动力系统混沌特性的典型代表。