Interacting ω(q) dark energy model with phase space analysis

DOI10.1142/S0217732321502229zbMath1489.83041OpenAlexW3205708380MaRDI QIDQ5067327

Shynaray Myrzakul, Koblandy Yerzhanov, Duman Kenzhalin, Martiros Khurshudyan

Publication date: 1 April 2022

Published in: Modern Physics Letters A (Search for Journal in Brave)

Full work available at URL: https://doi.org/10.1142/s0217732321502229

zbMATH Keywords

accelerated expansiondark energy

Mathematics Subject Classification ID

Geometrodynamics and the holographic principle (83E05) Phase-space methods including Wigner distributions, etc. applied to problems in quantum mechanics (81S30) Dark matter and dark energy (83C56)

Cites Work

• Dark energy cosmology: the equivalent description via different theoretical models and cosmography tests
• Inflationary universe in terms of a van der Waals viscous fluid
• Warm decaying dark matter and the hubble tension

This page was built for publication: Interacting ω(q) dark energy model with phase space analysis