Magnitude-dependent epidemic-type aftershock sequences model for earthquakes

Ilaria Spassiani and Giovanni Sebastiani
Phys. Rev. E 93, 042134 – Published 26 April 2016

Abstract

We propose a version of the pure temporal epidemic type aftershock sequences (ETAS) model: the ETAS model with correlated magnitudes. As for the standard case, we assume the Gutenberg-Richter law to be the probability density for the magnitudes of the background events. Instead, the magnitude of the triggered shocks is assumed to be probabilistically dependent on that of the relative mother events. This probabilistic dependence is motivated by some recent works in the literature and by the results of a statistical analysis made on some seismic catalogs [Spassiani and Sebastiani, J. Geophys. Res. 121, 903 (2016)]. On the basis of the experimental evidences obtained in the latter paper for the real catalogs, we theoretically derive the probability density function for the magnitudes of the triggered shocks proposed in Spassiani and Sebastiani and there used for the analysis of two simulated catalogs. To this aim, we impose a fundamental condition: averaging over all the magnitudes of the mother events, we must obtain again the Gutenberg-Richter law. This ensures the validity of this law at any event's generation when ignoring past seismicity. The ETAS model with correlated magnitudes is then theoretically analyzed here. In particular, we use the tool of the probability generating function and the Palm theory, in order to derive an approximation of the probability of zero events in a small time interval and to interpret the results in terms of the interevent time between consecutive shocks, the latter being a very useful random variable in the assessment of seismic hazard.

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  • Received 6 February 2016
  • Revised 2 April 2016

DOI:https://doi.org/10.1103/PhysRevE.93.042134

©2016 American Physical Society

Physics Subject Headings (PhySH)

  1. Research Areas
Statistical Physics & Thermodynamics

Authors & Affiliations

Ilaria Spassiani1,* and Giovanni Sebastiani1,2,†

  • 1Department of Mathematics “Guido Castelnuovo”, Sapienza University of Rome, Rome, Italy
  • 2Istituto per le Applicazioni del Calcolo “M. Picone”, Consiglio Nazionale delle Ricerche, Rome, Italy

  • *spassianiilaria@gmail.com
  • sebastiani@mat.uniroma1.it

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Issue

Vol. 93, Iss. 4 — April 2016

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