Motion of a pair of gravitating bodies in dark energy presence: small deviations from Keplerian motion

Neishtadt, Anatoly; Bisnovatyi-Kogan, Gennady

Neishtadt_BK_two_body_4fin_a1.pdf (321.65 kB)

Motion of a pair of gravitating bodies in dark energy presence: small deviations from Keplerian motion

journal contribution

posted on 18.08.2020, 09:27 authored by Anatoly NeishtadtAnatoly Neishtadt, Gennady Bisnovatyi-Kogan

The problem of the motion of two gravitating bodies in the presence of dark energy (DE), considered as a perturbing factor, is investigated. In addition to the orbit precession frequency obtained in previous studies, the correction to the orbital motion frequency was calculated, and the oscillations of the semi-major axis and the eccentricity of the orbit caused by the influence of DE were studied.

Funding

Russian Foundation for Basic Research, project nos. 18-02-00619, 20-02-000455, and 20-52-12053

Leverhulme Trust, project no. RPG-2018-143

History

School

Science

Department

Mathematical Sciences

Published in

Astronomy Reports

Volume

64

Issue

9

Pages

731 - 737

Publisher

Springer Verlag

Version

AM (Accepted Manuscript)

Rights holder

Publisher statement

This is a post-peer-review, pre-copyedit version of an article published in Astronomy Reports. The final authenticated version is available online at: https://doi.org/10.1134/S1063772920100054

Acceptance date

30/05/2020

Publication date

2020-09-23

Copyright date

2020

Notes

The accepted version of this paper is written in Russian. A version of the accepted paper in English does not exist. The paper was accepted in Russian to the journal “Astronomicheskii Zhurnal” (“Астрономический журнал “). "Astronomy Reports” is the English translation of this journal. Translation was performed in the editorial house. The published version is in English.