Domain wall and holographic dark energy in \(f(Q)\) theory of gravity
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Publication:6601428
DOI10.1142/S0219887824400334zbMATH Open1547.83126MaRDI QIDQ6601428
S. P. Hatkar, D. P. Tadas, S. D. Katore
Publication date: 10 September 2024
Published in: International Journal of Geometric Methods in Modern Physics (Search for Journal in Brave)
Relativistic cosmology (83F05) Geometrodynamics and the holographic principle (83E05) Relativistic gravitational theories other than Einstein's, including asymmetric field theories (83D05)
Cites Work
- Dark energy models in \(f(R,T)\) theory with variable deceleration parameter
- Cosmological models with linearly varying deceleration parameter
- Modified Gauss-Bonnet theory as gravitational alternative for dark energy
- \(f(R)\) theories
- Holographic dark energy density
- Domain walls in \(f(R,T)\) theory of gravitation
- Transit cosmological models with domain walls in \(f(R,T)\) gravity
- Model-independent reconstruction of \(f(Q)\) non-metric gravity
- First evidence that non-metricity \(f(Q)\) gravity could challenge \(\Lambda\)CDM
- Cosmological parameters from SDSS and WMAP
- RECONSTRUCTION OF f(R, T) GRAVITY DESCRIBING MATTER DOMINATED AND ACCELERATED PHASES
- Domain wall cosmological models with deceleration parameter in modified theory of gravitation
- Dark energy nature of viscus universe in f(Q)-gravity with observational constraints
- Transit string dark energy models in f(Q) gravity
- Tsallis holographic dark energy scenario in viscous f(Q) gravity with tachyon field
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