A direct <i>N</i>-body integrator for modelling the chaotic, tidal dynamics of multibody extrasolar systems: <tt>TIDYMESS</tt>

نویسندگان

چکیده

Tidal dissipation plays an important role in the dynamical evolution of moons, planets, stars and compact remnants. The interesting complexity originates from interplay between internal structure external tidal forcing. Recent upcoming observing missions exoplanets Galaxy help to provide constraints on physics dissipation. It is timely develop new N-body codes, which allow for experimentation with various models numerical implementations. We present open-source code TIDYMESS, stands ``TIdal DYnamics Multi-body ExtraSolar Systems''. This implements a creep deformation law bodies, parametrized by their fluid Love numbers relaxation times. Due centrifugal deformations, we approximate general shape body be ellipsoid. calculate associated gravitational field quadruple order, derive accelerations torques. equations motion orbits, spins deformations are integrated directly using fourth-order integration method based symplectic composition. implement novel allows time step solely dependent not spin periods or feature greatly speeds up calculations, while also improving consistency when comparing different regimes. demonstrate capabilities performance particularly niche regime parameter space where orbits chaotic tides become non-linear.

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ژورنال

عنوان ژورنال: Monthly Notices of the Royal Astronomical Society

سال: 2023

ISSN: ['0035-8711', '1365-8711', '1365-2966']

DOI: https://doi.org/10.1093/mnras/stad1133