Observational Constraints on Hybrid Scale Factor in f(Q,T)$f(Q,T)$ Gravity with Anisotropic Space‐Time

In this paper, we present an accelerating cosmological model by constraining the free parameters using datasets in extended symmetric teleparallel gravity for flat and anisotropic space-time. We employ a time variable deceleration parameter that behaves early late acceleration form of Hybrid Scale Factor (HSF). obtain values analyse behavior Universe based on best-fit parameters. derive dynamical equation state at quintessence region; however it approaches to $\Lambda$CDM. The energy conditions are also analysed validate modified find strong condition is violating. establish importance hybrid scale factor cosmic phenomena issue.