Constrained evolution of effective equation of state parameter in non-linear $$\qquad\qquad f\left( {R,L_{m} } \right)$$ dark energy model: insights from Bayesian analysis of cosmic chronometers and Pantheon samples
N. MyrzakulovL. N. Gumilyov Eurasian National University, 010008, Astana, KazakhstanM. KoussourQuantum Physics and Magnetism Team, LPMC, Faculty of Science Ben M’sik, Casablanca Hassan II University, Casablanca, MoroccoAlnadhief H. A. AlfedeelCentre for Space Research, North-West University, Potchefstroom, 2520, South AfricaAmare AbebeCentre for Space Research, North-West University, Potchefstroom, 2520, South Africa
2023en
ABI
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Аннотация мавжуд эмас.
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