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CAN SOLAR SYSTEM OBSERVATIONS TELL US SOMETHING ABOUT THE COSMOLOGICAL CONSTANT?

2005/11/30 by Lorenzo Iorio, LORENZO IORIO · 2 citations
Physics and Astronomy · #Astronomy and Astrophysical Research #Cosmology and Gravitation Theories #Relativity and Gravitational Theory #astro-ph #gr-qc #hep-ph

paper · pdf · doi:10.1142/s021827180600819x

published as Int.J.Mod.Phys. D15 (2006) 473-476 · Latex2e, 4 pages, 2 table, no figures, 11 references. Table 2 added, typos in the units of Lambda corrected

arxiv created 2005/12/01 · openalex publication_date 2006/04/01 · arxiv updated 2009/12/01 · openalex created_date 2016/06/24 · openalex updated_date 2026/07/28

Abstract

In this note, we show that the latest determinations of the residual perihelion advances [Formula: see text] of the inner planets of the Solar System, obtained by accounting for almost all known Newtonian and post-Newtonian orbital effects, yield only very broad constraints on the cosmological constant Λ. Indeed, from, e.g., [Formula: see text] arcseconds per century for Mercury, one gets -2 × 10 -34 km -2 < Λ < 4 × 10 -35 km -2 . The currently accepted value for Λ, obtained from many independent cosmological and large-scale measurements, amounts to almost 10 -46 km -2 .

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