2018
DOI: 10.1140/epjc/s10052-018-5932-8
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Can the apparent expansion of the universe be attributed to an increasing vacuum refractive index ?

Abstract: H.A. Wilson, then R.H. Dicke, proposed to describe gravitation by a spatial change of the refractive index of the vacuum around a gravitational mass. Dicke extended this formalism in order to describe the apparent expansion of the universe by a cosmological time dependence of the global vacuum index. In this paper, we develop Dicke's formalism. The metric expansion in standard cosmology (the timedependent scale factor of the Friedmann-Lemaître curved spacetime metric) is replaced by a flat and static Euclidean… Show more

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Cited by 10 publications
(7 citation statements)
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“…With a few exceptions (e.g. [24,26,27,28]), it is widely agreed that gravitationally bound objects do not expand cosmologically. On the other hand, despite the redshift of the Virgo cluster, i.e.…”
Section: The Lower Limit Of Cosmological Expansion or Scale Driftmentioning
confidence: 99%
“…With a few exceptions (e.g. [24,26,27,28]), it is widely agreed that gravitationally bound objects do not expand cosmologically. On the other hand, despite the redshift of the Virgo cluster, i.e.…”
Section: The Lower Limit Of Cosmological Expansion or Scale Driftmentioning
confidence: 99%
“…Assuming that the paired-photon strings or filaments form the fabric of space, their density gradients are gravitational fields [93][94][95][96][97]. Since the substance of space seeks thermodynamic balance in the least time, the bodies move coupled to the moving vacuum along the least-time paths, i.e., geodesics.…”
Section: The Gravitonmentioning
confidence: 99%
“…With a few exceptions (e.g. [24]), it is widely agreed that gravitationally bound objects do not expand cosmologically. On the other hand, despite the redshift of the Virgo cluster, the so-called Virgo infall exists [4].…”
Section: The Lower Limit Of Cosmological Expansion or Scale Driftmentioning
confidence: 99%