Cosmological scenario in κ(R,T) gravity
From MaRDI portal
Publication:6187555
DOI10.1142/S021988782250013XMaRDI QIDQ6187555
Anirudh Pradhan, Archana Dixit, R. Chaubey
Publication date: 31 January 2024
Published in: International Journal of Geometric Methods in Modern Physics (Search for Journal in Brave)
Relativistic cosmology (83F05) Relativistic gravitational theories other than Einstein's, including asymmetric field theories (83D05)
Cites Work
- Cosmological reconstruction and stability in \(f(R,T)\) gravity
- Holographic Ricci dark energy with constant bulk viscosity in \(f(R,T)\) gravity
- Generalization of the Einstein Theory
- A periodic varying deceleration parameter in f(R, T) gravity
- Statefinder diagnostic for modified Chaplygin gas cosmology in f(R,T) gravity with particle creation
- Various dark energy models for variables G and Λ in f(R, T) modified theory
- ON THE COSMOLOGICAL CONSTANT AND THE COSMIC COINCIDENCE PROBLEM
- Jerk, snap and the cosmological equation of state
- RECONSTRUCTION OF f(R, T) GRAVITY DESCRIBING MATTER DOMINATED AND ACCELERATED PHASES
- Cosmic jerk, snap and beyond
- IS GRAVITY AN INTRINSICALLY QUANTUM PHENOMENON? DYNAMICS OF GRAVITY FROM THE ENTROPY OF SPACE–TIME AND THE PRINCIPLE OF EQUIVALENCE
- 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
This page was built for publication: Cosmological scenario in κ(R,T) gravity