Late-time cosmic acceleration from compactification

DOI10.1088/1361-6382/AB0804zbMath1476.83197arXiv1811.03660OpenAlexW3100436728WikidataQ64298248 ScholiaQ64298248MaRDI QIDQ5152939

Jorge G. Russo, Paul K. Townsend

Publication date: 28 September 2021

Published in: Classical and Quantum Gravity (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/1811.03660

zbMATH Keywords

compactificationcosmologyenergy conditionsno-go theorems

Mathematics Subject Classification ID

Relativistic cosmology (83F05) Geometrodynamics and the holographic principle (83E05) Einstein's equations (general structure, canonical formalism, Cauchy problems) (83C05) Classes of solutions; algebraically special solutions, metrics with symmetries for problems in general relativity and gravitational theory (83C20) Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.) (83C55) Kaluza-Klein and other higher-dimensional theories (83E15) Dimensional compactification in quantum field theory (81T33)

Related Items (10)

Out of the swampland with multifield quintessence? ⋮ Pixelated Dark Energy ⋮ Hidden sectors in string theory: kinetic mixings, fifth forces and quintessence ⋮ No asymptotic acceleration without higher-dimensional de Sitter vacua ⋮ Stringy multifield quintessence and the swampland ⋮ Universal accelerating cosmologies from 10d supergravity ⋮ String cosmology: from the early universe to today ⋮ Time-dependent compactification to De Sitter space: a no-go theorem ⋮ A dilaton-axion model for string cosmology ⋮ Hyperbolic field space and swampland conjecture for DBI scalar

Cites Work

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• de Sitter vacua in string theory
• M/string theory, S-branes and the accelerating universe
• Thoughts on tachyon cosmology
• A Study of Accelerating Cosmologies from Superstring/M Theories
• Cosmology as geodesic motion
• What if string theory has no de Sitter vacua?

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