A non-linear mathematical model for the X-ray variability classes of the microquasar GRS 1915+105 -- I: quiescent, spiking states and QPOs
E. Massaro, F. Capitanio, M. Feroci, T. Mineo, A. Ardito, P. Ricciardi

TL;DR
This paper introduces a non-linear differential equation model, adapted from the Hindmarsh-Rose model, that simulates the diverse X-ray variability patterns and QPOs of the microquasar GRS 1915+105 by adjusting a single input parameter.
Contribution
The study develops a unified differential equation framework that reproduces various variability classes and QPOs of GRS 1915+105 through parameter variation, providing new insights into its complex behavior.
Findings
Model reproduces multiple variability classes and QPOs
Transitions between stable and unstable states driven by a single parameter
Stability analysis of equilibrium points supports observed phenomena
Abstract
The microquasar GRS 1915+105 is known to exhibit a very variable X-ray emission on different time scales and patterns. We propose a system of two ordinary differential equations, adapted from the Hindmarsh-Rose model, with two dynamical variables x(t), y(t) and an input constant parameter J_0, to which we added a random white noise, whose solutions for the x(t) variable reproduce consistently the X-ray light curves of several variability classes as well as the development of low frequency Quasi-Periodic Oscillations (QPO). We show that changing only the value of J_0 the system moves from stable to unstable solutions and the resulting light curves reproduce those of the quiescent classes like phi and chi, the delta class and the spiking rho class. Moreover, we found that increasing the values of J_0 the system induces high frequency oscillations that evolve to QPO when it moves into…
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