Deflation of vacuum energy during inflation due to Bulk-Brane interaction
DOI10.1088/1475-7516/2020/10/050zbMath1494.83031arXiv2006.11517OpenAlexW3097194400MaRDI QIDQ5071001
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Publication date: 14 April 2022
Published in: Journal of Cosmology and Astroparticle Physics (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/2006.11517
Density estimation (62G07) String and superstring theories in gravitational theory (83E30) Geometrodynamics and the holographic principle (83E05) Kaluza-Klein and other higher-dimensional theories (83E15) Relativistic gravitational theories other than Einstein's, including asymmetric field theories (83D05) Galactic and stellar structure (85A15)
Cites Work
- Gravitational coupling and dynamical reduction of the cosmological constant
- Non-conventional cosmology from a brane universe
- Effect of the chameleon scalar field on brane cosmological evolution
- Cosmological constant -- the weight of the vacuum
- Cosmology of a Brane Radiating Gravitons into the Extra Dimension
- Mechanism for a decaying cosmological constant
- Cosmological constant in chameleon Brans–Dicke theory
- Brane cosmology with a non-minimally coupled bulk-scalar field
- Measurements of Ω and Λ from 42 High‐Redshift Supernovae
- Inflationary universe: A possible solution to the horizon and flatness problems
- The cosmological constant problem
- The cosmological constant
- Brane-world gravity
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