Phantom dark energy nature of bulk-viscosity universe in modified f(Q)-gravity

DOI10.1142/S0219887822501985zbMath1530.83007OpenAlexW4284972849WikidataQ114072255 ScholiaQ114072255MaRDI QIDQ6188604

Dinesh Chandra Maurya, Archana Dixit, Anirudh Pradhan

Publication date: 7 February 2024

Published in: International Journal of Geometric Methods in Modern Physics (Search for Journal in Brave)

Full work available at URL: https://doi.org/10.1142/s0219887822501985

zbMATH Keywords

observational constraintbulk-viscosityLRS Bianchi type-I universemodified \(f(Q)\)-gravitytransit phase expansion

Mathematics Subject Classification ID

Relativistic cosmology (83F05) Relativistic gravitational theories other than Einstein's, including asymmetric field theories (83D05) Exact solutions to problems in general relativity and gravitational theory (83C15)

Related Items (2)

Phantom dark energy nature of string-fluid cosmological models in \(f(Q) \)-gravity ⋮ Observational constraints in accelerated emergent f(Q) gravity model

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