Testing the growth rate in homogeneous and inhomogeneous interacting vacuum models
DOI10.1088/1475-7516/2023/06/009zbMath1528.83127arXiv2303.04793MaRDI QIDQ6173860
Unnamed Author, Humberto A. Borges, Cássio Pigozzo, Micol Benetti, Unnamed Author
Publication date: 13 July 2023
Published in: Journal of Cosmology and Astroparticle Physics (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/2303.04793
Relativistic cosmology (83F05) Diffraction, scattering (78A45) Quantum optics (81V80) Observational and experimental questions in relativity and gravitational theory (83B05) Geodesics in global differential geometry (53C22) Galactic and stellar structure (85A15) Approximation procedures, weak fields in general relativity and gravitational theory (83C25) Dark matter and dark energy (83C56)
Cites Work
- Unification of dark matter and dark energy: the inhomogeneous Chaplygin gas
- Density perturbations in a universe dominated by the Chaplygin gas
- Correction to: ``Dynamical system analysis of interacting models
- Cosmological constant -- the weight of the vacuum
- Inhomogeneous vacuum energy
- The cosmological constant and dark energy
- The angular size–redshift relation in power-law cosmologies
- Cosmological parameters from SDSS and WMAP
- Looking for interactions in the cosmological dark sector
- 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
- Chaplygin gas with non-adiabatic pressure perturbations
- Observational constraints on interacting vacuum energy with linear interactions
- An alternative to quintessence
- Non-adiabatic Chaplygin gas
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