A Solar System Test of Mach's Principle with Gravimetric Data

dc.creatorUnzicker, Alexander
dc.creatorFabian, Karl
dc.date2006-10-07
dc.date.accessioned2026-07-07T07:27:57Z
dc.date.available2026-07-07T07:27:57Z
dc.descriptionWe present a new test for a possible Mach-Sciama dependence of the Gravitational constant G. According to Ernst Mach (1838-1916), the gravitational interaction depends on the distribution of masses in the universe. A corresponding hypothesis of Sciama (1953) on the gravitational constant, $c^2/G = \sum m_i/r_i$, can be tested since the elliptic earth orbit should then cause minute annual variations in G. The test is performed by analyzing the gravity signals of a network of superconducting gravimeters (SG) which reach a precision of $10^{-10} m/s^2$. After reducing the signal by modelling tidal, meteorologic and geophysical effects, no significant evidence for the above dependence is found.
dc.description8 pages, figures separate. To include figures, run pdflatex as described in the source. Paper with figures included can be obtained from http://www.alexander-unzicker.de/research.html
dc.identifierhttps://arxiv.org/abs/gr-qc/0610028
dc.identifierhttp://arxiv.org/abs/gr-qc/0610028
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/117562
dc.subjectGeneral Relativity and Quantum Cosmology
dc.subjectAstrophysics
dc.titleA Solar System Test of Mach's Principle with Gravimetric Data
dc.typetext

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