Abstract
The Casimir effect predicted in 1948 was not initially seen as relevant to cosmology. For a long time the cosmological constant and the quantum mechanics of the vacuum lived separate lives. The situation only changed in the late 1960s. Inspired by a brief revival of interest in cosmological models with a positive cosmological constant, in 1968 Yakov Zel’dovich pointed out the significance of the constant in the context of quantum field theory. He also formulated the first version of what would be known as the cosmological-constant problem. With Zel’dovich’s work two historical strands were finally joined: the quantum vacuum and the energy density related to the cosmological constant.
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Notes
- 1.
Indeed, the fate of the cosmological constant since 1917 has been remarkably chequered. According to a later review, “The cosmological constant \(\varLambda \) is an idea whose time has come ... and gone ... and come ... and so on” (Carroll et al. 1992, p. 536). And according to a still later review, “It has been alternately reviled and praised, and it has been counted out so many times, only to stage one comeback after another” (Earman 2001, p. 189).
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Kragh, H.S., Overduin, J.M. (2014). From Casimir to Zel’dovich. In: The Weight of the Vacuum. SpringerBriefs in Physics. Springer, Berlin, Heidelberg. https://doi.org/10.1007/978-3-642-55090-4_8
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