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Inertia in Friedmann Universes with variable \(G\) and \(\varLambda\)
- 作者:J. Sultana ; D. Kazanas
- 关键词:Inertia ; Friedmann Universes ; Mach’s Principle
- 刊名:Astrophysics and Space Science
- 出版年:2015
- 出版时间:September 2015
- 年:2015
- 卷:359
- 期:1
- 全文大小:719 KB
- 参考文献:Abbussattar, Vishwakarma, R.G.: Class. Quantum Gravity 14, 945 (1997) ADS View Article
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D. Kazanas (2)
1. Department of Mathematics, Faculty of Science, University of Malta, Msida, MSD2080, Malta 2. Astrophysics Science Division, NASA/Goddard Space Flight Center Greenbelt, Maryland, 20771, USA
- 刊物类别:Physics and Astronomy
- 刊物主题:Physics
Astronomy
- 出版者:Springer Netherlands
- ISSN:1572-946X
文摘
In light of the recent interest in dynamical dark energy models based on a cosmology with varying gravitational and cosmological parameters \(G\) and \(\varLambda\), we present here a model of inertia in a type of Friedmann universe with \(G = G_{0}(A/A_{0})^{\sigma}\); \(A\) being the dimensionless scale factor, that was recently studied by Singh et al. (Astrophys. Space Sci. 345:213, 2013). The proposed Machian model of inertia utilizes the curved space generalization of Sciama’s law of inertial induction, which is based on the analogy between the retarded far fields of electrodynamics and those of gravitation, and expresses the total inertial force \(F= -ma\) on an accelerating mass \(m\) in terms of contributions from all matter in the observable Universe. We show that for a varying Friedmann model with \(\sigma=-3/2\), inertial induction alone can account for the total inertial force on the accelerating mass. We then compare this cosmological model with current observational constraints for the variation of \(G\).
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