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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%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%2Fhdy.2008.105
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https://dx.doi.org/10.1038/s41562-026-02568-4
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https://doi.org/10.1038%2Fs41598-018-32468-1
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https://doi.org/10.1088%2F0264-9381%2F19%2F13%2F304
Time varying models of dark energy can, to a certain extent, ameliorate the fine-tuning problem (faced by Λ), but do not resolve the puzzle of cosmic coincidence
https://doi.org/10.5194/GMD-19-2577-2026
The direct greenhouse effect of VOCs is generally minor due to either low abundance or weak absorption of infrared radiation, but they can exert larger indirect climate effects through their influence on key atmospheric processes
https://doi.org/10.5194/acp-22-10173-2022
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https://dx.doi.org/10.5067/DOCUM-AQR05
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https://doi.org/10.5120/ijca2017913207
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