Andrade rheology in time-domain. Application to Enceladus' dissipation of energy due to forced libration
Yeva Gevorgyan, Gwena\"el Bou\'e, Clodoaldo Ragazzo, Lucas S. Ruiz,, Alexandre C. M. Correia

TL;DR
This paper introduces a time-domain implementation of Andrade rheology for simulating deformable bodies, applied to analyze Enceladus' libration and tidal heating, accommodating complex motions and providing new analytical and numerical insights.
Contribution
It presents a novel time-domain approach to Andrade rheology applicable to three-dimensional simulations, enabling analysis of complex orbital and librational behaviors.
Findings
Estimated core libration amplitude is 0.6% of the shell's.
Reproduced observed 10 GW tidal heat with viscosity of 0.17×10^14 Pa·s.
Provided an analytic formula for libration amplitude including rheological correction.
Abstract
The main purpose of this work is to present a time-domain implementation of the Andrade rheology, instead of the traditional expansion in terms of a Fourier series of the tidal potential. This approach can be used in any fully three dimensional numerical simulation of the dynamics of a system of many deformable bodies. In particular, it allows large eccentricities, large mutual inclinations, and it is not limited to quasi-periodic perturbations. It can take into account an extended class of perturbations, such as chaotic motions, transient events, and resonant librations. The results are presented by means of a concrete application: the analysis of the libration of Enceladus. This is done by means of both analytic formulas in the frequency domain and direct numerical simulations. We do not a priori assume that Enceladus has a triaxial shape, the eventual triaxiality is a consequence…
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