Relaxing the cosmological constant: a proof of concept

DOI10.1007/JHEP12(2016)022zbMath1390.83428arXiv1608.05715WikidataQ63354070 ScholiaQ63354070MaRDI QIDQ1636610

David Pirtskhalava, Paolo Creminelli, Andrei Khmelnitsky, Lasma Alberte, Enrico Trincherini

Publication date: 12 June 2018

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

Full work available at URL: https://arxiv.org/abs/1608.05715

zbMATH Keywords

classical theories of gravityglobal symmetrieseffective field theories

Mathematics Subject Classification ID

Relativistic cosmology (83F05)

Related Items (8)

Massless minimal quantum scalar field with an asymmetric self interaction in de Sitter spacetime ⋮ Self-tuning of the cosmological constant in brane-worlds with P(X,ϕ) ⋮ Inflation with 0 ≤ c _s ≤ 1 ⋮ Non-perturbative analysis for a massless minimal quantum scalar with V(ϕ) = λϕ ⁴/4! + βϕ ³/3! in the inflationary de Sitter spacetime ⋮ A small weak scale from a small cosmological constant ⋮ Robustness of the cosmological constant damping mechanism through matter eras ⋮ Superfluids and the cosmological constant problem ⋮ Reheating after relaxation of large cosmological constant

Cites Work

• Inflation from Minkowski space
• Starting the universe: stable violation of the null energy condition and non-standard cosmologies
• The big constant out, the small constant in
• Manifestly Local Theory of Vacuum Energy Sequestering
• Why the Cosmological Constant Is Small and Positive
• The cosmological constant problem
• \(k\)-inflation

This page was built for publication: Relaxing the cosmological constant: a proof of concept