Phenomenological dark energy model with hybrid dynamic cosmological constant
From MaRDI portal
Publication:5023556
DOI10.1088/1361-6382/AC35EDzbMath1484.83031arXiv2202.01209OpenAlexW3209994500WikidataQ112108308 ScholiaQ112108308MaRDI QIDQ5023556
Publication date: 24 January 2022
Published in: Classical and Quantum Gravity (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/2202.01209
Relativistic cosmology (83F05) Geometrodynamics and the holographic principle (83E05) Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.) (83C55) Dusty-gas two-phase flows (76T15) Dark matter and dark energy (83C56)
Uses Software
Cites Work
- Unnamed Item
- Gravitationally induced particle production and its impact on structure formation
- Scenario of accelerating universe: role of phenomenological \(\varLambda\) models
- Accelerating Universe with a dynamic cosmological term
- The cosmological constant and dark energy
- Solving the main cosmological puzzles with a generalized time varying vacuum energy
- Can vacuum decay in our universe?
- Evolution of the Expanding Universe
- A Machian model of dark energy
- The evolution of the FRW universe with decaying metastable dark energy—a dynamical system analysis
- Measurements of Ω and Λ from 42 High‐Redshift Supernovae
- Cosmological models with Gurzadyan–Xue dark energy
- The Cosmological Constants
This page was built for publication: Phenomenological dark energy model with hybrid dynamic cosmological constant