Open and closed world models in Kaluza-Klein-theory with variables G and \(\lambda\)
From MaRDI portal
Publication:481312
DOI10.1007/s10773-014-2142-5zbMath1305.83060OpenAlexW2131789412WikidataQ126111162 ScholiaQ126111162MaRDI QIDQ481312
Publication date: 12 December 2014
Published in: International Journal of Theoretical Physics (Search for Journal in Brave)
Full work available at URL: https://doi.org/10.1007/s10773-014-2142-5
Cites Work
- Kaluza-Klein cosmology with varying \(G\) and \(\Lambda \)
- Kaluza-Klein cosmology with modified holographic dark energy
- Kaluza-Klein type Robertson Walker cosmological model with dynamical cosmological term \(\Lambda\)
- Brane universes tested by supernovae Ia
- Why there is nothing rather than something: A theory of the cosmological constant
- Kaluza–Klein-type models of de Sitter and Poincaré gauge theories of gravity
- Scale-Covariant Theory of Gravitation and Astrophysical Applications
- The cosmological constant problem and quintessence
- Testing non-standard cosmological models with supernovae
- Can the Stephani model be an alternative to FRW accelerating models?
- Restricted uniform density and corresponding convergence methods
- Measurements of Ω and Λ from 42 High‐Redshift Supernovae
- Type Ia Supernova Discoveries atz> 1 from theHubble Space Telescope: Evidence for Past Deceleration and Constraints on Dark Energy Evolution
- The cosmological constant problem
- An alternative to quintessence
This page was built for publication: Open and closed world models in Kaluza-Klein-theory with variables G and \(\lambda\)