# Impact of the distribution of recovery rates on disease spreading in   complex networks

**Authors:** Guilherme Ferraz de Arruda, Giovanni Petri, Francisco A. Rodrigues,, and Yamir Moreno

arXiv: 1812.04734 · 2020-01-22

## TL;DR

This paper analyzes how heterogeneity in recovery rates influences epidemic spreading on complex networks, revealing shifts in critical thresholds and the interplay between network structure and dynamical parameters.

## Contribution

It introduces an analytical model incorporating arbitrary recovery rate distributions, highlighting their impact on epidemic thresholds and network behavior.

## Key findings

- Heterogeneous recovery rates significantly alter epidemic critical points.
- Power-law networks can mimic homogeneous behavior through recovery rate tuning.
- Recovery rate heterogeneity affects spreading localization properties.

## Abstract

We study a general epidemic model with arbitrary recovery rate distributions. This simple deviation from the standard setup is sufficient to prove that heterogeneity in the dynamical parameters can be as important as the more studied structural heterogeneity. Our analytical solution is able to predict the shift in the critical properties induced by heterogeneous recovery rates. Additionally, we show that the critical value of infectivity tends to be smaller than the one predicted by quenched mean-field approaches in the homogeneous case and that it can be linked to the variance of the recovery rates. We then illustrate the role of dynamical--structural correlations, which allow for a complete change in the critical behavior. We show that it is possible for a power-law network topology to behave similarly to a homogeneous structure by an appropriate tuning of its recovery rates, and vice versa. Finally, we show how heterogeneity in recovery rates affects the network localization properties of the spreading process.

## Full text

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## Figures

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## References

29 references — full list in the complete paper: https://tomesphere.com/paper/1812.04734/full.md

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Source: https://tomesphere.com/paper/1812.04734