Beyond Fab Four

DOI10.1088/0264-9381/32/24/242001zbMath1331.83066arXiv1507.05942OpenAlexW3105817563MaRDI QIDQ2788968

Christos Charmousis, David Langlois, Ryo Saito, Eugeny Babichev

Publication date: 23 February 2016

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

Full work available at URL: https://arxiv.org/abs/1507.05942

zbMATH Keywords

scalar-tensor theorymodified gravityself tuning of cosmological constant

Mathematics Subject Classification ID

Geometrodynamics and the holographic principle (83E05) Applications of differential geometry to physics (53Z05) Einstein's equations (general structure, canonical formalism, Cauchy problems) (83C05) Relativistic gravitational theories other than Einstein's, including asymmetric field theories (83D05)

Related Items (9)

Disformally self-tuning gravity ⋮ Modeling dark sector in Horndeski gravity at first-order formalism ⋮ Tadpole cosmology: self tuning without degeneracy ⋮ Tadpole cosmology: Milne solution as a cosmological constant hideout ⋮ Strong gravitational lensing by DHOST black holes ⋮ Cosmological consequences and thermodynamics of modified gravity with extended nonminimal derivative couplings ⋮ Superfluids and the cosmological constant problem ⋮ Stellar pulsations in beyond Horndeski gravity theories ⋮ Asymptotically flat black holes in Horndeski theory and beyond

Cites Work

• Generalized G-Inflation: --Inflation with the Most General Second-Order Field Equations--
• A unifying description of dark energy
• A small cosmological constant from a large extra dimension
• General properties of the self-tuning domain wall approach to the cosmological constant problem

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