Periapsis precession in general stationary and axisymmetric spacetimes

Abstract This work studies the periapsis shift in the equatorial plane of arbitrary stationary and axisymmetric spacetimes. Two perturbative methods are systematically developed. The first works for small eccentricity but very general orbit size and the second, which is post-Newtonian and includes t...

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Main Authors: Jinhong He, Shaofei Xu, Junji Jia
Format: Article
Language:English
Published: SpringerOpen 2024-12-01
Series:European Physical Journal C: Particles and Fields
Online Access:https://doi.org/10.1140/epjc/s10052-024-13680-y
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author Jinhong He
Shaofei Xu
Junji Jia
author_facet Jinhong He
Shaofei Xu
Junji Jia
author_sort Jinhong He
collection DOAJ
description Abstract This work studies the periapsis shift in the equatorial plane of arbitrary stationary and axisymmetric spacetimes. Two perturbative methods are systematically developed. The first works for small eccentricity but very general orbit size and the second, which is post-Newtonian and includes two variants, is more accurate for orbits of large size but allows general eccentricity. Results from these methods are shown to be equivalent under small eccentricity and large size limits. The periapsis shift of Kerr–Newman, Kerr–Sen and Kerr–Taub-NUT spacetimes is computed to high orders. The electric charge and NUT charge are shown to contribute to the leading order but with opposite signs. The frame-dragging term and high-order effect of spacetime spin are given. The electric and NUT charges of the Earth, Sun and Sgr A* are constrained using the Mercury, satellite and S2 precession data. Periapsis shifts of other spacetimes are obtained too.
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issn 1434-6052
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spelling doaj-art-7135df88866044168f4848473d668f612025-02-02T12:38:41ZengSpringerOpenEuropean Physical Journal C: Particles and Fields1434-60522024-12-01841212310.1140/epjc/s10052-024-13680-yPeriapsis precession in general stationary and axisymmetric spacetimesJinhong He0Shaofei Xu1Junji Jia2Department of Astronomy, School of Physics and Technology, Wuhan UniversitySchool of Physics and Technology, Wuhan UniversityDepartment of Astronomy and MOE Key Laboratory of Artificial Micro- and Nano-structures, School of Physics and Technology, Wuhan UniversityAbstract This work studies the periapsis shift in the equatorial plane of arbitrary stationary and axisymmetric spacetimes. Two perturbative methods are systematically developed. The first works for small eccentricity but very general orbit size and the second, which is post-Newtonian and includes two variants, is more accurate for orbits of large size but allows general eccentricity. Results from these methods are shown to be equivalent under small eccentricity and large size limits. The periapsis shift of Kerr–Newman, Kerr–Sen and Kerr–Taub-NUT spacetimes is computed to high orders. The electric charge and NUT charge are shown to contribute to the leading order but with opposite signs. The frame-dragging term and high-order effect of spacetime spin are given. The electric and NUT charges of the Earth, Sun and Sgr A* are constrained using the Mercury, satellite and S2 precession data. Periapsis shifts of other spacetimes are obtained too.https://doi.org/10.1140/epjc/s10052-024-13680-y
spellingShingle Jinhong He
Shaofei Xu
Junji Jia
Periapsis precession in general stationary and axisymmetric spacetimes
European Physical Journal C: Particles and Fields
title Periapsis precession in general stationary and axisymmetric spacetimes
title_full Periapsis precession in general stationary and axisymmetric spacetimes
title_fullStr Periapsis precession in general stationary and axisymmetric spacetimes
title_full_unstemmed Periapsis precession in general stationary and axisymmetric spacetimes
title_short Periapsis precession in general stationary and axisymmetric spacetimes
title_sort periapsis precession in general stationary and axisymmetric spacetimes
url https://doi.org/10.1140/epjc/s10052-024-13680-y
work_keys_str_mv AT jinhonghe periapsisprecessioningeneralstationaryandaxisymmetricspacetimes
AT shaofeixu periapsisprecessioningeneralstationaryandaxisymmetricspacetimes
AT junjijia periapsisprecessioningeneralstationaryandaxisymmetricspacetimes