Constraining spacetime torsion with LAGEOS
arXiv:1101.2791 · doi:10.1007/s10714-011-1226-2
Abstract
We compute the corrections to the orbital Lense-Thirring effect (or frame-dragging) in the presence of spacetime torsion. We derive the equations of motion of a test body in the gravitational field of a rotating axisymmetric massive body, using the parametrized framework of Mao, Tegmark, Guth and Cabi. We calculate the secular variations of the longitudes of the node and of the pericenter. We also show how the LAser GEOdynamics Satellites (LAGEOS) can be used to constrain torsion parameters. We report the experimental constraints obtained using both the nodes and perigee measurements of the orbital Lense-Thirring effect. This makes LAGEOS and Gravity Probe B (GPB) complementary frame-dragging and torsion experiments, since they constrain three different combinations of torsion parameters.
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- Effective interactions in Ricci-Based Gravity models below the non-metricity scale
- Constraints from orbital motions around the Earth of the environmental fifth-force hypothesis for the OPERA superluminal neutrino phenomenology
- Covariant Equations of Motion of Extended Bodies with Arbitrary Mass and Spin Multipoles
- Effect of TTC on Satellite Orbital Mechanics
- (3+1)-Formulation for Gravity with Torsion and Non-Metricity II: The Hypermomentum Equation
- Solar system dynamics in general relativity
- Interference effects and modified Born rule in the presence of torsion
- Is torsion needed in a theory of gravity? A reappraisal