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https://doi.org/10.1038%2Fs41558-020-00985-5
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https://dx.doi.org/10.1038/s41586-026-10893-x
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https://doi.org/10.1038%2Fhdy.2008.105
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https://doi.org/10.1038%2Fs41526-017-0015-y
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https://dx.doi.org/10.1038/s41586-026-10876-y
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https://dx.doi.org/10.1038/s41586-026-10912-x
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https://doi.org/10.1038%2Fs41598-018-32468-1
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https://dx.doi.org/10.1038/s41562-026-02568-4
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https://doi.org/10.1088%2F0264-9381%2F19%2F13%2F304
A cutoff at the Planck or electroweak scale leads to a cosmological constant which is, respectively, 10123 or 1055 times larger than the observed value, Λ/8πG ≃ 10−47 GeV4
https://doi.org/10.5194/GMD-19-2577-2026
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https://doi.org/10.5194/acp-22-10173-2022
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