Dark energy without fine tuning

DOI10.1007/JHEP10(2019)044zbMath1427.83135arXiv1905.00045WikidataQ127090570 ScholiaQ127090570MaRDI QIDQ2283380

José Eliel Camargo-Molina, Tommi Markkanen, Pat Scott

Publication date: 2 January 2020

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

Full work available at URL: https://arxiv.org/abs/1905.00045

zbMATH Keywords

dark energyclassical theories of gravitycosmology of theories beyond the SM

Mathematics Subject Classification ID

Relativistic cosmology (83F05) Symmetry breaking in quantum theory (81R40) Relativistic gravitational theories other than Einstein's, including asymmetric field theories (83D05) Astrophysical cosmology (85A40) Dark matter and dark energy (83C56)

Related Items (1)

Quintessential α-attractor inflation: forecasts for Stage IV galaxy surveys

Cites Work

• Dark energy as a remnant of inflation and electroweak symmetry breaking
• Natural quintessence?
• The cosmological constant and dark energy
• DYNAMICS OF DARK ENERGY
• Measurements of Ω and Λ from 42 High‐Redshift Supernovae
• The confrontation between general relativity and experiment

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