Observational constrained Weyl type gravity cosmological model and the dynamical system analysis
arXiv:2402.18915 · doi:10.1016/j.astropartphys.2024.103011
Abstract
Using the cosmological date sets, the cosmological parameters are constrained in this paper, with some well known form of Hubble parameter. To understand the dynamics of the Weyl type , functional form has been introduced, where and respectively represents the nonmetricity scalar and trace of energy-momentum tensor. Using the constrained values of the parameters, the other geometrical parameters are analysed and the accelerating behaviour has been shown. Further to get the complete evolutionary behaviour of the Universe, the dynamical system analysis has been performed.
17 pages, 7 figures, 4 tables. Suggestions and comments are welcome
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Cited by in corpus (5)
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- Constraining Exponential f(Q) Gravity with Cosmic Chronometers and Supernovae: A Data-Driven Analysis
- Accelerating behavior from dynamical system analysis parameters
- Logarithmic and Strong Coupling Models in Weyl-Type Gravity
- Cosmological Dynamics of Exponential Quintessence Constrained by BAO, Cosmic Chronometers, and DES-SN5YR/Pantheon+ Data