ARWV Code User Manual

(2) Dep. of Physics; (3) Univ. of Turku; Finland); France; Italy; P. Chassonnery (1); R. Capuzzo-Dolcetta (2); Sapienza; S. Mikkola (3) ((1) ENS Paris-Saclay; Univ. of Rome

ARWV Code User Manual

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arxiv 1910.05202 v2 pith:ZY4BEQYO submitted 2019-10-11 astro-ph.IM

P. Chassonnery (1) , R. Capuzzo-Dolcetta (2) , S. Mikkola (3) ((1) ENS Paris-Saclay , France , (2) Dep. of Physics , Sapienza , Univ. of Rome , Italy

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(3) Univ. of Turku Finland)

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With this report we provide users of an easy manual to facilitate the proper download and use of a sophisticated, high precision, few-body code originally developed by S. Mikkola, and later largely improved and implemented to treat a variety of cases. The code download can be done via the link https://drive.google.com/file/d/16FkVVR4Tk8eKhKMju2vQ9rlWI4Mpv01W/view The use of the code is free upon proper citation. The work is in progress and users are invited to help the authors to improve both the code and the user handbook.

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Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. OpenAlex reports about 3 citations worldwide. Full citation record

Impact of a granular mass distribution on the orbit of S2 in the Galactic center
astro-ph.GA 2025-07 accept novelty 6.0 of 10

Granularity in the mass distribution around Sagittarius A* can perturb S2's orbit enough that the 2026 apocenter passage may reveal stellar-mass black holes, with simulated astrometric residuals exceeding GRAVITY's 30...

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