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I propose an observationally and theoretically consistent resolution of the cosmological constant problem: $\Lambda$ is a counterterm -- with a running coupling -- that balances the monopole celestial sky average of the kinetic energy of expansion of inhomogeneously distributed `small' cosmic voids.
1912
Earlier work this paper cites.
S. Weinberg, “The cosmological constant problem,” Rev. Mod. Phys. 61
1989
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T. Buchert, “On average properties of inhomogeneous fluids in general relativity I: Dust cosmologies”, Gen. Rel. Grav. 32
2001
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F. Hoyle and M. S. Vogeley, “Voids in the PCSZ survey and the updated Zwicky catalog,” Astrophys. J. 566
2004
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A. Ishibashi and R. M. Wald, “Can the acceleration of our universe be explained by the effects of inhomogeneities?,” Class. Quant. Grav. 23
2006
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D. L. Wiltshire, “Cosmic clocks, cosmic variance and cosmic averages,” New J. Phys. 9
2007
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D. L. Wiltshire, “Exact solution to the averaging problem in cosmology,” Phys. Rev. Lett. 99
2007
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D. L. Wiltshire, “Gravitational energy and cosmic acceleration,” Int. J. Mod. Phys. D 17
2007
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2008
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2008
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D. L. Wiltshire, “Average observational quantities in the timescape cosmology,” Phys. Rev. D 80
2009
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2009
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D. Sapone, E. Majerotto and S. Nesseris, Phys. Rev. D 90
2014
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2012
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2023
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