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Second order statistics characterization of Hawkes processes and non-parametric estimation
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We show that the jumps correlation matrix of a multivariate Hawkes process is related to the Hawkes kernel matrix through a system of Wiener-Hopf integral equations. A Wiener-Hopf argument allows one to prove that this system (in which the kernel matrix is the unknown) possesses a unique causal solution and consequently that the second-order properties fully characterize a Hawkes process. The numerical inversion of this system of integral equations allows us to propose a fast and efficient method, which main principles were initially sketched in [Bacry and Muzy, 2013], to perform a non-parametric estimation of the Hawkes kernel matrix. In this paper, we perform a systematic study of this non-parametric estimation procedure in the general framework of marked Hawkes processes. We describe precisely this procedure step by step. We discuss the estimation error and explain how the values for the main parameters should be chosen. Various numerical examples are given in order to illustrate the broad possibilities of this estimation procedure ranging from 1-dimensional (power-law or non positive kernels) up to 3-dimensional (circular dependence) processes. A comparison to other non-parametric estimation procedures is made. Applications to high frequency trading events in financial markets and to earthquakes occurrence dynamics are finally considered.
Forward citations
Cited by 2 Pith papers
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Scaling Limit Theorems for Multivariate Hawkes Processes and Stochastic Volterra Equations with Measure Kernel
Asymptotically critical multivariate Hawkes processes converge to the unique weak solution of a stochastic Volterra equation with a measure kernel, characterized by an admissible pair (K, Φ).
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Mean-Field Limits for Nearly Unstable Hawkes Processes
Nearly unstable Hawkes processes rescale to affine stochastic Volterra diffusions, and mean-field Hawkes systems exhibit synchronization, conditional independence, or extinction depending on n(1-||phi^n||)^2.
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