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Studying tidal effects in planetary systems with Posidonius. A N-body simulator written in Rust.

Blanco-Cuaresma, Sergi; Bolmont, Emeline

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        <foaf:name>Blanco-Cuaresma, Sergi</foaf:name>
            <foaf:name>Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138, USA</foaf:name>
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        <foaf:name>Bolmont, Emeline</foaf:name>
            <foaf:name>Laboratoire AIM Paris-Saclay, CEA/DRF-CNRS-Univ. Paris Diderot - IRFU/SAp, Centre de Saclay, F- 91191 Gif-sur-Yvette Cedex, France</foaf:name>
    <dct:title>Studying tidal effects in planetary systems with Posidonius. A N-body simulator written in Rust.</dct:title>
    <dct:issued rdf:datatype="">2017</dct:issued>
    <dct:issued rdf:datatype="">2017-10-15</dct:issued>
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    <dct:description>&lt;p&gt;Planetary systems with several planets in compact orbital configurations such as TRAPPIST-1 are surely affected by tidal effects. Its study provides us with important insight about its evolution. We developed a second generation of a N-body code based on the tidal model used in Mercury-T, re-implementing and improving its functionalities using Rust as programming language (including a Python interface for easy use) and the WHFAST integrator. The new open source code ensures memory safety, reproducibility of numerical N-body experiments, it improves the spin integration compared to Mercury-T&amp;nbsp;and allows to take into account a new prescription for the dissipation of tidal inertial waves in the convective envelope of stars. Posidonius is also suitable for binary system simulations with evolving stars.&lt;/p&gt;</dct:description>
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