Cosmic dynamics beyond Einstein theory: mathematical analysis with \(f(R, T)\) gravity
From MaRDI portal
Publication:6538428
DOI10.1007/S10773-024-05553-7zbMATH Open1540.831MaRDI QIDQ6538428
Rajiv Kumar Mishra, Navya Jain
Publication date: 14 May 2024
Published in: International Journal of Theoretical Physics (Search for Journal in Brave)
energy conditionsdeceleration parameter\(f(R, T)\) theoryenergy-momentum tensor Friedmann-Lemaître-Robertson-Walker spacetime
Relativistic cosmology (83F05) 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
- A relation between distance and radial velocity among extra-galactic nebulae.
- Constraining \(f(R,T)\) gravity from the dark energy density parameter \(\Omega_{\Lambda} \)
- The cosmological constant and dark energy
- CERTAIN COSMOLOGICAL MODELS WITH VARIATION OF HUBBLE PARAMETER
Related Items (1)
Dynamics of some compact structures and moment of inertia in \(f(\mathcal{R}, \mathcal{T})\) gravity
This page was built for publication: Cosmic dynamics beyond Einstein theory: mathematical analysis with \(f(R, T)\) gravity
Report a bug (only for logged in users!)Click here to report a bug for this page (MaRDI item Q6538428)
