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Quantum consistency suggests that any de Sitter patch that lasts a number of Hubble times that exceeds its Gibbons-Hawking entropy divided by the number of light particle species suffers an effect of quantum breaking.
1940
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G. Dvali, S. H. H. Tye, Brane inflation, Phys. Lett. B450 (1999) 72, arXiv:hep-ph/9812483; G. Dvali, Q. Shafi, S. Solganik, D-brane inflation, arXiv:hep-th/0105203
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L. Boubekeur, D. H. Lyth, Hilltop inflation, JCAP 0507 (2005) 010, arXiv:hep-ph/0502047
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A. D. Linde, Eternally Existing Self-reproducing Chaotic Inflationary Universe, Phys. Lett. B 175 (1986) 395. A. H. Guth, Eternal inflation and its implications, J. Phys. A40 (2007) 6811, arXiv:hep-th/0702178
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2014
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2018
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2018
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In [ 1 , 3 ] this bound was derived from quantum breaking due to a collective effect of purely graviton scattering. The relation ( 2
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G. Dvali, C. Gomez, On Exclusion of Positive Cosmological Constant, arXiv:1806.10877 [hep-th]
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D. Andriot, On the de Sitter swampland criterion, arXiv:1806.10999 [hep-th]
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S. K. Garg, C. Krishnan, Bounds on Slow Roll and the de Sitter Swampland, arXiv:1807.05193 [hep-th]
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A. Kehagias and A. Riotto, A note on Inflation and the Swampland, arXiv:1807.05445 [hep-th]
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2019
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