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Everpresent $\Lambda$ is a cosmological scenario in which the observed cosmological "constant" $\Lambda$ fluctuates between positive and negative values with a vanishing mean, and with a magnitude comparable to the critical density at any epoch.
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A. J. Korn, F. Grundahl, O. Richard, P. S. Barklem, L. Mashonkina, R. Collet, N. Piskunov, and B. Gustafsson, A probable stellar solution to the cosmological lithium discrepancy
2006
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2007
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J. D. Barrow, A Strong Constraint on Ever-Present Lambda
2007
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J. A. Zuntz, The cosmic microwave background in a causal set universe
2008
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2010
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M. Pospelov and J. Pradler, Big Bang Nucleosynthesis as a Probe of New Physics
2010
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2015
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F. Melia and T. M. McClintock, Supermassive Black Holes in the Early Universe
2015
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2015
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2015
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2015
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2016
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2016
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2016
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W. L. Freedman, Correction: Cosmology at a crossroads
2017
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