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Solar system effects in Schwarzschild--de Sitter spacetime

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arxiv gr-qc/0602002 v2 pith:WVMCH7CW submitted 2006-02-01 gr-qc

classification gr-qc
keywords lambdaeffectsgravitationalsitterconstantcosmologicalperihelionpioneer
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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 $\Lambda=\Lambda_0 \sim 10^{-52} {\rm m}^{-2}$ the cosmological constant plays no role for all of these effects, while a value of $\Lambda \sim - 10^{-37} {\rm m}^{-2}$, if hypothetically held responsible for the Pioneer anomaly, is not compatible with the Perihelion shift.

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Cited by 2 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. Gravitational lensing time delay beyond the Shapiro/geometry split

    astro-ph.CO 2026-05 unverdicted novelty 7.0 of 10

    Derivation from Schwarzschild-de Sitter null geodesics recovers the standard time-delay split as the leading small-angle term, with the first correction intrinsic to the Schwarzschild metric and adding no new cosmolog...

  2. Observational Tests of Regular Black Holes with Scalar Hair and their Stability

    gr-qc 2025-10 unverdicted novelty 5.0 of 10

    Regular black holes with phantom scalar hair are constrained by Solar System and EHT observations, with exact relations linking photon sphere Lyapunov exponent to shadow size and impact parameter.

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