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It has been suggested that low energy effective field theories should satisfy given conditions in order to be successfully embedded into string theory.
1902
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E. Palti, “The Swampland: Introduction and Review,” arXiv:1903.06239 [hep-th]
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F. Finelli and R. Brandenberger, “On the generation of a scale-invariant spectrum of adiabatic fluctuations in cosmological models with a contracting phase,” Phys. Rev. D 65
2002
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S. P. Patil and R. H. Brandenberger, “The Cosmology of massless string modes,” JCAP 0601
2003
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R. H. Brandenberger, “Lectures on the theory of cosmological perturbations,” Lect. Notes Phys. 646
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A. Nayeri, R. H. Brandenberger and C. Vafa, “Producing a scale-invariant spectrum of perturbations in a Hagedorn phase of string cosmology,” Phys. Rev. Lett. 97
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R. Bousso, B. Freivogel and I. S. Yang, “Eternal Inflation: The Inside Story,” Phys. Rev. D 74
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H. Ooguri and C. Vafa, “On the Geometry of the String Landscape and the Swampland,” Nucl. Phys. B 766
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N. Arkani-Hamed, L. Motl, A. Nicolis and C. Vafa, “The String landscape, black holes and gravity as the weakest force,” JHEP 0706
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2018
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H. Matsui and F. Takahashi, “Eternal Inflation and Swampland Conjectures,” Phys. Rev. D 99
2018
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2019
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2019
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