Dark energy beyond quintessence: constraints from the swampland

DOI10.1007/JHEP06(2019)070zbMath1416.83150arXiv1902.11014OpenAlexW3101209229WikidataQ127661595 ScholiaQ127661595MaRDI QIDQ2314928

Md. Wali Hossain, Suddhasattwa Brahma

Publication date: 30 July 2019

Published in: Journal of High Energy Physics (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/1902.11014

zbMATH Keywords

classical theories of gravitycosmology of theories beyond the SMeffective field theories

Mathematics Subject Classification ID

Relativistic cosmology (83F05) Model quantum field theories (81T10) Relativistic gravitational theories other than Einstein's, including asymmetric field theories (83D05)

Related Items (12)

Constraints on dark energy models from the Horndeski theory ⋮ Cosmic acceleration from string induced Galileons ⋮ Multi-field inflation in high-slope potentials ⋮ Out of the swampland with multifield quintessence? ⋮ Rescaled Einstein–Hilbert gravity: Inflation and the Swampland criteria ⋮ The Swampland: Introduction and Review ⋮ On the occurrence of finite-time singularities in swampland-related quintessence dark energy models ⋮ Reconstruction of quintessence field for the THDE with swampland correspondence in f(R,T) gravity ⋮ Compact objects and the swampland ⋮ Leaving the Swampland: non-geometric fluxes and the distance conjecture ⋮ Hyperbolic field space and swampland conjecture for DBI scalar ⋮ The stringy origins of Galileons and their novel limit

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