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19962026
most citedThe IAU 2000 resolutions for astrometry, celestial mechanics and metrology in the relativistic framework: explanatory supplement

391 citations · 649 across the 22 of their papers we have counts for

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12 papers · 1 filter

gr-qc2026

Gravitational waves and small-field astrometry

Robin Geyer, Sven Zschocke, Michael Soffel +3

Astrometric observations can, in principle, be used to detect gravitational waves. In this paper we give a practical overview of the gravitational wave effects which can be expecte…

gr-qc2023★ 10 cited

Reference frames in General Relativity and the galactic rotation curves

L. Filipe O. Costa, José Natário, F. Frutos-Alfaro +1

The physical interpretation of the exact solutions of the Einstein field equations is, in general, a challenging task, part of the difficulties lying in the significance of the coo…

gr-qc2016★ 26 cited

On Relativistic Multipole Moments of Stationary Spacetimes

Francisco Frutos-Alfaro, Michael Soffel

Among the known exact solutions of Einstein vacuum field equations the Manko-Novikov and the Quevedo-Mashhoon metrics might be suitable ones for the description of the exterior gra…

gr-qc2015★ 7 cited

On the Post-linear Quadrupole-Quadrupole Metric

Francisco Frutos-Alfaro, Michael Soffel

The Hartle-Thorne metric defines a reliable spacetime for most astrophysical purposes, for instance for the simulation of slowly rotating stars. Solving the Einstein field equation…

gr-qc2015★ 11 cited

Effects on satellite orbits in the gravitational field of an axisymmetric central body with a mass monopole and arbitrary spin multipole moments

J. Meichsner, M. H. Soffel

Perturbations of satellite orbits in the gravitational field of a body with a mass monopole and arbitrary spin multipole moments are considered for an axisymmetric and stationary s…

gr-qc2014★ 17 cited

The gravitational time delay in the field of a slowly moving body with arbitrary multipoles

Michael H. Soffel, Wen-Biao Han

We calculate the time delay of light in the gravitational field of a slowly moving body with arbitrary multipoles (mass and spin multipole moments) by the Time-Transfer-Function (T…

gr-qc2014★ 6 cited

The post-linear Schwarzschild solution in harmonic coordinates: elimination of structure-dependent terms

Sergei Klioner, Michael Soffel

The paper deals with a special kind of problems that appear in solutions of Einstein's field equations for extended bodies: many structure-dependent terms appear in intermediate ca…

gr-qc2013★ 1 cited

Towards sub-microarcsecond models for relativistic astrometry

S. Zschocke, S. A. Klioner, M. H. Soffel

Astrometric space missions like Gaia have stimulated a rapid advance in the field of relativistic astrometry. Present investigations in that field aim at accuracies significantly l…

gr-qc2005★ 13 cited

General-relativistic perturbation equations for the dynamics of elastic deformable astronomical bodies expanded in terms of generalized spherical harmonics

Chongming Xu, Xuejun Wu, Michael Soffel

In our previous paper, based on the Carter & Quintana framework and the Damour-Soffel-Xu scheme, we deduced a complete and closed set of post-Newtonian dynamical equations for elas…

gr-qc2003★ 17 cited

Relativistic theory of elastic deformable astronomical bodies: perturbation equations in rotating spherical coordinates and junction conditions

Chongming Xu, Xuejun Wu, Michael Soffel +1

In this paper, the dynamical equations and junction conditions at the interface between adjacent layers of different elastic properties for an elastic deformable astronomical body…

gr-qc1999★ 47 cited

Relativistic Celestial Mechanics with PPN Parameters

Sergei A. Klioner, Michael H. Soffel

Starting from the global parametrized post-Newtonian (PPN) reference system with two PPN parameters and we consider a space-bounded subsystem of matter and construct a loca…

gr-qc1998★ 6 cited

Nordtvedt effect in rotational motion

Sergei A. Klioner, Michael Soffel

Rotational motion of extended celestial bodies is discussed in the framework of the Parametrized Post-Newtonian (PPN) formalism with the two parameters and . A local PPN ref…