Solar system effects in Schwarzschild--de Sitter spacetime

Abstract

The Schwarzschild--de Sitter space--time describes the gravitational field of a spherically symmetric mass in a universe with cosmological constant $\Lambda$. Based on this space--time we calculate Solar system effects like gravitational redshift, light deflection, gravitational time delay, Perihelion shift, geodetic or de Sitter precession, as well as the influence of $\Lambda$ on a Doppler measurement, used to determine the velocity of the Pioneer 10 and 11 spacecraft. For $\Lambda ={\Lambda }_0\sim 10^{-52}{\mathrm{m}}^{-2}$ the cosmological constant plays no role for all of these effects, while a value of $\Lambda \sim -10^{-37}{\mathrm{m}}^{-2}$, if hypothetically held responsible for the Pioneer anomaly, is not compatible with the Perihelion shift.

Published version

References in corpus (3)

• Two-body problem with the cosmological constant and observational constraints
• On the effects of the Dvali-Gabadadze-Porrati braneworld gravity on the orbital motion of a test particle
• General relativity and quintessence explain the Pioneer anomaly

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