Late-time acceleration by a residual cosmological constant from sequestering vacuum energy in ultimate collapsed structures

DOI10.1088/1475-7516/2019/09/065OpenAlexW2803711682MaRDI QIDQ5861866

Lucas Lombriser

Publication date: 2 March 2022

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

Full work available at URL: https://arxiv.org/abs/1805.05918

zbMATH Keywords

dark energy theorygalaxy clusters

Mathematics Subject Classification ID

Relativity and gravitational theory (83-XX)

Related Items (5)

Well-tempered teleparallel Horndeski cosmology: a teleparallel variation to the cosmological constant problem ⋮ Limitations on Standard Sirens tests of gravity from screening ⋮ About the measure of the bare cosmological constant ⋮ Exploring the self-tuning of the cosmological constant from Planck mass variation ⋮ Self-tuning kinetic gravity braiding: cosmological dynamics, shift symmetry, and the tadpole

Cites Work

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• Challenges to self-acceleration in modified gravity from gravitational waves and large-scale structure
• Manifestly Local Theory of Vacuum Energy Sequestering
• The well-tempered cosmological constant
• Measurements of Ω and Λ from 42 High‐Redshift Supernovae
• The cosmological constant problem

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