Future deceleration due to backreaction in a Universe with multiple inhomogeneous domains
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Publication:6047817
DOI10.1088/1475-7516/2023/08/064arXiv2305.17616MaRDI QIDQ6047817
Unnamed Author, Shashank Shekhar Pandey, Archan S. Majumdar
Publication date: 13 September 2023
Published in: Journal of Cosmology and Astroparticle Physics (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/2305.17616
Relativistic cosmology (83F05) Observational and experimental questions in relativity and gravitational theory (83B05) Dark matter and dark energy (83C56)
Cites Work
- Effect of cosmic backreaction on the future evolution of an accelerating universe
- Isotropic space with discrete gravitational-field sources. On the theory of a nonhomogeneous isotropic universe
- Towards a theory of macroscopic gravity
- On average properties of inhomogeneous fluids in general relativity: Dust cosmologies
- Backreaction: directions of progress
- Can the acceleration of our universe be explained by the effects of inhomogeneities?
- Constraints on backreaction in dust universes
- Is there proof that backreaction of inhomogeneities is irrelevant in cosmology?
- Covariant coarse graining of inhomogeneous dust flow in general relativity
- THE EFFECT OF STRUCTURE FORMATION ON THE EXPANSION OF THE UNIVERSE
- Cosmological Solutions in Macroscopic Gravity
- Future evolution in a backreaction model and the analogous scalar field cosmology
- On the relationship between mean observations, spatial averages and the Dyer-Roeder approximation in Einstein-Straus models
- Another look at redshift drift and the backreaction conjecture
- Effect of inhomogeneities on the propagation of gravitational waves from binaries of compact objects
- Towards statistically homogeneous and isotropic perfect fluid universes with cosmic backreaction
- An adaptive Metropolis algorithm
- On average properties of inhomogeneous fluids in general relativity: Perfect fluid cosmologies
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