arXiv · 1104.1306
The Problem of Inertia in Friedmann Universes
Abstract
In this paper we study the origin of inertia in a curved spacetime, particularly the spatially flat, open and closed Friedmann universes. This is done using Sciama's law of inertial induction, which is based on Mach's principle, and expresses the analogy between the retarded far fields of electrodynamics and those of gravitation. After obtaining covariant expressions for electromagnetic fields due to an accelerating point charge in Friedmann models, we adopt Sciama's law to obtain the inertial force on an accelerating mass $m$ by integrating over the contributions from all the matter in the universe. The resulting inertial force has the form $F = -kma$, where $k < 1 $ depends on the choice of the cosmological parameters such as $Ω_{M}$, $Ω_Λ$, and $Ω_{R}$ and is also red-shift dependent.
Explore related subjects
Keep this discovery
Explore connections, maps & timelines
Joseph Sultana, Demosthenes Kazanas. 2011-04-07. The Problem of Inertia in Friedmann Universes. https://doi.org/10.1142/s0218271811019384
Cite the original work for its findings. Save a collection to share your selection of sources.