Phantom dark energy nature of string-fluid cosmological models in \(f(Q) \)-gravity
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Publication:6204646
DOI10.1134/s0202289323040151OpenAlexW4388961580MaRDI QIDQ6204646
Publication date: 2 April 2024
Published in: Gravitation \& Cosmology (Search for Journal in Brave)
Full work available at URL: https://doi.org/10.1134/s0202289323040151
dark energyphantom fieldBianchi modelnonmetricity\(f(Q)\) gravityLocally Rotationally Symmetric spacetime
Relativistic cosmology (83F05) Relativistic gravitational theories other than Einstein's, including asymmetric field theories (83D05) Dark matter and dark energy (83C56)
Cites Work
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- Teleparallel gravity. An introduction
- LRS Bianchi type-I universe in Barber's second self creation theory
- Exact spatially homogeneous cosmologies
- Model-independent reconstruction of \(f(Q)\) non-metric gravity
- LRS Bianchi type II perfect fluid cosmological models in normal gauge for Lyra's manifold
- Some magnetized bulk viscous string cosmological models in general relativity
- A class of homogeneous cosmological models
- Massive String Cosmology in Bianchi Type III Space-Time with Electromagnetic Field
- PALATINI APPROACH TO MODIFIED GRAVITY: f(R) THEORIES AND BEYOND
- DYNAMICS OF DARK ENERGY
- INTRODUCTION TO MODIFIED GRAVITY AND GRAVITATIONAL ALTERNATIVE FOR DARK ENERGY
- Modified Gravity Models of Dark Energy
- Some Magnetized Bulk Viscous String Cosmological Models in Cylindrically Symmetric Inhomogeneous Universe with Variable Λ-Term
- Quantum electrodynamic formulation of the Josephson tunnelling theory
- Topology of cosmic domains and strings
- Anisotropy in Bianchi-type brane cosmologies
- Transit dark energy string cosmological models with perfect fluid in F(R,T)-gravity
- Viscous Bianchi type I universes in brane cosmology
- Anisotropic Bianchi Type-I Magnetized String Cosmological Models with Decaying Vacuum Energy Density Λ( t )
- The canonical frame of purified gravity
- Teleparallel Palatini theories
- 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
- LOCALLY ROTATIONALLY SYMMETRIC BIANCHI TYPE-I COSMOLOGICAL MODEL IN f(T) GRAVITY: FROM EARLY TO DARK ENERGY DOMINATED UNIVERSE
- Observational constraints in accelerated emergent f(Q) gravity model
- String models in Lyra geometry
- String cosmologies with a scalar field
- Dark energy nature of viscus universe in f(Q)-gravity with observational constraints
- Transit cosmological models in modified f(Q,T) gravity
- The models of transit cosmology along with observational constriction in f(Q,T) gravity
- Barrow holographic dark energy models in f(Q) symmetric teleparallel gravity with Lambert function distribution
- Cosmic evolution of holographic dark energy in f(Q,T) gravity
- Transit string dark energy models in f(Q) gravity
- Phantom dark energy nature of bulk-viscosity universe in modified f(Q)-gravity
- Tsallis holographic dark energy scenario in viscous f(Q) gravity with tachyon field
