Stochastic eternal inflation is in the swampland
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Publication:2292447
DOI10.1007/JHEP11(2019)016zbMath1429.83105arXiv1904.10979WikidataQ126815927 ScholiaQ126815927MaRDI QIDQ2292447
Suddhasattwa Brahma, Sarah Shandera
Publication date: 3 February 2020
Published in: Journal of High Energy Physics (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/1904.10979
Relativistic cosmology (83F05) Model quantum field theories (81T10) String and superstring theories in gravitational theory (83E30) Applications of statistics to physics (62P35)
Related Items (17)
Self-organised localisation ⋮ Multi-field inflation in high-slope potentials ⋮ Eternal inflation in swampy landscapes ⋮ Topological eternal hilltop inflation and the swampland criteria ⋮ Multi-field inflation from single-field models ⋮ Swampland, trans-Planckian censorship and fine-tuning problem for inflation: tunnelling wavefunction to the rescue ⋮ Swampland constraints on no-boundary quantum cosmology ⋮ Quantum cosmology, eternal inflation, and swampland conjectures ⋮ Review of the no-boundary wave function ⋮ Role of trans-Planckian modes in cosmology ⋮ How a four-dimensional de Sitter solution remains outside the swampland ⋮ Four-dimensional de Sitter space is a Glauber-Sudarshan state in string theory ⋮ Implications of single field inflation in general cosmological scenarios on the nature of dark energy given the swampland conjectures ⋮ Crisis on infinite earths: short-lived De Sitter vacua in the string theory landscape ⋮ A tail of eternal inflation ⋮ Black hole production, eternal inflation, and information in quasi-de Sitter space ⋮ Conditions for (no) eternal inflation
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