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I investigate whether eternal inflation is possible when the inflaton originally travels upslope the scalar potential and inevitably reaches a turn-around point where its classical kinetic energy momentarily vanishes.
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Earlier work this paper cites.
A. D. Linde, Phys. Lett. B 175
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N. Arkani-Hamed, L. Motl, A. Nicolis and C. Vafa, JHEP 0706
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E. Dudas, N. Kitazawa and A. Sagnotti, Phys. Lett. B 694
2011
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L. Susskind, In *Carr, Bernard (ed.): Universe or multiverse?* 247-266 [hep-th/0302219]
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G. Obied, H. Ooguri, L. Spodyneiko and C. Vafa, arXiv:1806.08362 [hep-th]
Cited in the paper.
Y. Akrami, R. Kallosh, A. Linde and V. Vardanyan, arXiv:1808.09440 [hep-th]
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Cited in the paper.
H. Matsui and F. Takahashi, arXiv:1807.11938 [hep-th]
Cited in the paper.
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