The well-tempered cosmological constant: fugue in B♭

DOI10.1088/1475-7516/2020/12/037zbMath1484.83033arXiv2009.01723OpenAlexW3116487116MaRDI QIDQ5027100

Eric V. Linder, Stephen A. Appleby

Publication date: 3 February 2022

Published in: Journal of Cosmology and Astroparticle Physics (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/2009.01723

zbMATH Keywords

modified gravitydark energy theory

Mathematics Subject Classification ID

Quantum field theory on curved space or space-time backgrounds (81T20) Relativistic gravitational theories other than Einstein's, including asymmetric field theories (83D05) Exact solutions to problems in general relativity and gravitational theory (83C15) Minkowski geometries in nonlinear incidence geometry (51B20) Matrix models and tensor models for quantum field theory (81T32) Dark matter and dark energy (83C56)

Related Items (8)

A minimal self-tuning model to solve the cosmological constant problem ⋮ Well-tempered teleparallel Horndeski cosmology: a teleparallel variation to the cosmological constant problem ⋮ Tadpole cosmology: self tuning without degeneracy ⋮ Hi-COLA: fast, approximate simulations of structure formation in Horndeski gravity ⋮ Tadpole cosmology: Milne solution as a cosmological constant hideout ⋮ Well-tempered Minkowski solutions in teleparallel Horndeski theory ⋮ An expansion of well tempered gravity ⋮ Self-tuning kinetic gravity braiding: cosmological dynamics, shift symmetry, and the tadpole

Cites Work

• Categorizing different approaches to the cosmological constant problem
• Generalized G-Inflation: --Inflation with the Most General Second-Order Field Equations--
• Manifestly Local Theory of Vacuum Energy Sequestering
• The well-tempered cosmological constant
• Brane cosmology and the self-tuning of the cosmological constant
• The cosmological constant problem
• Well-tempered cosmology
• The cosmological constant

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