A MODEL OF 1PN QUASI-RIGID BODY FOR ROTATION OF CELESTIAL BODIES-Reference-Cited by-同舟云学术

A MODEL OF 1PN QUASI-RIGID BODY FOR ROTATION OF CELESTIAL BODIES

Published:2003-05 Issue:05 Volume:12 Page:811-824
ISSN:0218-2718
Container-title:International Journal of Modern Physics D
language:en
Short-container-title:Int. J. Mod. Phys. D

Author:

TAO JIN-HE¹²,XU CHONG-MING³

Affiliation:

1. Purple Mountain Observatory, The Chinese Academy of Sciences, Nanjing, 210008, P. R. China

2. National Astronomical Observatories, The Chinese Academy of Sciences, Nanjing, 210008, P. R. China

3. Department of Physics, Nanjing Normal University, Nanjing, 210097, P. R. China

Abstract

Applying the Damour–Soffel–Xu framework of general-relativistic celestial mechanics, the theory of relativistic rigid body presented by Thorne and Gürsel is extended and developed in this paper. We successfully construct a quasi-rigid body model in the full post-Newtonian framework for the first time. This model has some simple properties in a similar way to the Newtonian rigid body, and it could be applied in geodynamics and astronomy, for example, to solve problems on rotation or precession of celestial bodies when relativistic effects are not negligible.

Publisher

World Scientific Pub Co Pte Lt

Subject

Space and Planetary Science,Astronomy and Astrophysics,Mathematical Physics

Link

https://www.worldscientific.com/doi/pdf/10.1142/S0218271803003311

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